PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2007-01-15 START_ORBIT_NUMBER = 1583 STOP_ORBIT_NUMBER = 35887 START_TIME = 1999-059T20:08:12.259 STOP_TIME = 2006-307T01:03:00 NOTE = " This document includes the Experimenter's Notebook (ENB) entries summarizing data collection by TES during Mapping; the ENB was originally produced by the TES Mission Planner to be available online throughout the duration of the mission. This document is appropriate for all available mapping orbits. Two types of information can be found in the ENB documents: the ENB_ORBIT.TXT contains blocks of TES orbits and starting time entries; the ENB_IMG.TXT contains the p*.img notes referenced in the ENB_ORBIT.TXT. TES data is organized by orbit which begins at the MGS descending equator crossing (times given in UTC). Orbits are labeled here with the TES orb number which is equivalent to ock (see obs.fmt OBJECT = ORBIT_COUNTER_KEEPER) except where deviations are noted. TES operations during a particular orbit are controlled by the p*.img file available onboard; key information from this file is provided in the p*.img notes." END_OBJECT = TEXT END p1583.img notes: 1) limbs all fore (neg angles), 100 km height with one pad at bottom angle, 1/2 degree steps, -90 space, -75 day, then limb set angles, all overlays a) normal = equator to 90N every 10 degrees b) spread = every 10 degrees for entire orbit (30 sets) c) polar = 40N dayside up over pole to 40N night (30 sets) d) hst = 60S dayside up over pole to 60N night (30 sets) - all limbs built using Michael's new tools 2) background sequences, all long packets a) normal = space/refs, stare at subsolar surface 15 min b) polar = space/refs/alb_ref, stare at Npole 15 min c) idle = space/refs, idle (used before & after COBE) d) COBE = long dwells at 6 angles (pos test and neg test) done during MOC star cal periods using star point or earth point orientation 3) only 63 orbits loaded - bug in tsl_loader constrains mplan entries (fixed by Michael after this nipc radiated) 4) spacecraft orientation = ~10 orbits nadir pointed, two orbits earth pointed, for first five days MOC star scan occurs during first earth pointed orbit - prior to earth point ish NOTE: limb angles were not changed to pnt_view=L, and are "D"s necessitating use of pfix_input during processing p1631.img notes: 1) limbs all fore (neg angles), 100 km height with one pad at bottom angle, 1/2 degree steps, -90 space, -75 day, then limb set angles, all overlays a) normal = equator to 90N every 10 degrees b) spread = every 10 degrees for entire orbit (30 sets) c) polar = 40N dayside up over pole to 40N night (30 sets) - limb from p1583.img: limb pnt_view changed from D to L 2) background sequences, all long packets a) normal = space/refs, stare at subsolar surface 15 min b) polar = space/refs/alb_ref, stare at Npole 15 min c) idle = space/refs, idle (used before & after COBE) d) COBE = long dwells at 6 angles (neg test) done during MOC star cal period using star point or earth point orientation 3) bug in tsl_loader fixed by Michael, loaded 120 orbits p1680.img notes: 1) limbs from previous orbit - spread and spread offset by 5 degrees for gore avoidance 2) surface - 60S to 70N, full 3) night - 1/2+h2o+co2_select spectral mask used 4) tables for HRC 5) space/ref sets - 5 per orbit, shifted every other orbit, alb_ref1 once a day on idle orbit (earth point) 6) set orbit command used to set orbit to ock number (1681) p1718.img notes: 1) limbs from previous orbit - added one EPF on "a" orbits 4 angles, 5 icks each, target 15 degrees north lat 2) moved space/ref sets away from limb overlay times 3) buffer management: surface - 50S to 50N, sdm 7 1, full_select night - 50N to 50S, sdm 7 1, half_h2o_co2_select poles - 50 to pole to 50, sdm 1 1, half_h2o_co2_select 4) loaded ocks 1718-1837 p1816.img notes: 1) limbs from previous orbit - no changes 2) buffer management: surface - 65S to 65N, sdm 7 1, full_select night - 65N to 65S, sdm 7 1, half_h2o_co2_select poles - 65 to pole to 65, sdm 1 1, half_h2o_co2_select 3) loaded ocks 1816-1959 4) HGA deployment during this period, ocks 1920-1959 are idles TES will be powered off prior to deployment WARNING: during earth point orbits, spacecraft in EOM mode - no time broadcasts sent to TES, instrument safed self - resumes when time broadcasts resume p1985.img notes: 1) TES powered on by LMA load and go command 2) uploaded ALGOR patch, wavenumber shift, temps, switch 00 3) set orb command to reset orbit number to ock 4) background sequences: day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 5) new spectral mask : "polar" for use during poles and night obs. 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) 7) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, one EPF (4 angles at 15N) 8) space/ref, space/alb_ref, space/ref/long space (10 extra icks of space to test stability) - all done as overlays to avoid limb looks 9) imc test loaded for later execution: find alb, positive angles, neg. angles - for use in analyzing IMC flight software patch functionality ERROR: TES did not appear to use the spacecraft broadcast equator crossings, stayed in PROM mode, can not find problem; no recording of data during equator crossing events NOTE: this upload got TES up and running from the tables loaded at p1985.img OCK 1987 notes: 1) LMA killed spacecraft broadcast equator-crossing script 2) loaded TES eqtrx cmd and set orbit command OCK 1998 notes: 1) memory dump request for 8 memory locations, necessary for checks prior to and after IMC flight software patch load OCK 2002 notes: - high gain antenna left in parked position, playback lost very little data for doy 1999-94 p2021.img notes: 1) rebuild of imc tests due to data lost when high gain antenna was unintentionally stowed 2) new eqtrx cmd 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) 5) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, one EPF (4 angles at 15N) 6) imc test: find alb, positive angles, neg.angles - for use in analyzing IMC flight software patch functionality p2022.img notes: 1) flight software patch - IMC 2) observations as in p2021.img, but all angles called out reversed 3) separate upload on memory dump (identical to ock 1998) OCK 2039 notes: - DSN problems, lost data ocks 2039 and 2040 p2045.img notes: 1) new eqtrx cmd 2) IMC patch on board, angles reversed 3) poles, night, and surface unchanged from 2022 upload 4) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, one EPF (4 angles at 15N) 7) limb_new changes: space_ref_long only on regular "a" orbits (five times a day); 100 icks stare at space (+90) with imc on at ick 1800 for ocks 2057 and 2059 real time pass - switch test 8) 10 days worth of orbits loaded OCK 2059 notes: 1) switch changed to 11 2) spacecraft equator-crossing broadcast re-enabled p2069.img notes: 1) IMC patch on board, angles reversed 2) optical switch reset to 00 3) PROM IMC table loaded 4) poles, night, and surface changed to turn on IMC 5) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) 7) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores 8) one EPF (4 angles) moved to ~9 degrees south lat, IMC turned on 9) space_ref_long only on regular "a" orbits (five times a day), moved to south polar space/ref time 10) interferogram test - 10 icks, detector 2, angle = -90 (space) starts at ick 1800 on ock 2079 - runs during real time SE_2A 11) 10 days worth of orbits loaded OCK 2080 notes: ERROR: instrument warmstart at equator crossing time, reason unknown OCK 2136 notes: Due to spacecraft problems (safed) after ock 2135 there is only partial data for ocks 2140 and 2145 (no other data) - prior to TES powered off p2146.img notes: 1) IMC patch on board, angles reversed 2) optical switch 00 3) PROM IMC table used 4) poles, night, and surface use IMC 5) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - for three consecutive non-realtime orbits testing buffer with poles set to spatial mask 5 (pairs of detectors averaged together) [ocks 2167, 2168, 2169] 6) for realtime orbits full spatial, full spectral data collected during entire realtime pass (~icks 1000 to 3000), rest of orbit use masks as outlined above 7) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface 8) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores 9) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle, - IMC turned on 10) 1 polar and 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time; 12) 10 days worth of orbits loaded ERROR: spacecraft safed ~5 hours after this upload, some data seen from this build (very little) p2318.img notes: 1) TES powered on by LMA command 2) new eqtrx cmd; in CSA-backup mode 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) 5) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, one EPF (4 angles at 15N) 6) imc test 3 times per day - planet/space alternates with interferograms on space looks once per day, idle rest of orbit 7) on HST orbits - no imc, regular limb orbit 8) 9 days worth of orbits loaded 9) simulated (siml'd) this upload ERROR: set_orbit command did not work, TES in PROM mode until ock 2329 p2329.img notes: 1) new set_orbit command sent (worked) NOTE: TES in PROM until ock 2329 p2355.img notes: 1) radiated in the blind before confirmation of set_orbit cmd 2) new eqtrx cmd; in CSA-backup mode 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) 5) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, one EPF (4 angles at 15N) 6) imc test 3 times per day - planet/space alternates with interferograms on space looks once per day, idle rest of orbit 7) on HST orbits - no imc, regular limb orbit 8) 6 days worth of orbits loaded 9) solar panel test - stare at -90 for 14 minutes ocks 2358 and 2376 spacecraft will halt solar panel movement on ock 2376 for 10 minutes p2367.img notes: 1) loaded IMC flight software patch 2) new eqtrx cmd; in CSA-backup mode 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - angles reversed due to patch 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - angles reversed due to patch 5) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, one EPF (4 angles at 15N) - angles reversed due to patch 6) imc test 3 times per day - planet/space alternates with interferograms on space looks once per day, idle rest of orbit - angles reversed due to patch 7) 7 days worth of orbits loaded 8) solar panel test - stare at -90 for 14 minutes ock 2376 spacecraft will halt solar panel movement on ock 2376 for 10 minutes ERROR: error of unknown origin during this upload (done during EOM - no visibility into instrument) caused TES to back up 2 orbits in its observation tables - ended up two orbits out of sync p2403.img notes: 1) IMC patch on board, angles reversed - no IMC used in upload 2) optical switch 00 3) set_orb command sent to recover from p2367.img error 4) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 5) for realtime orbits full spatial, full spectral data collected during entire realtime pass (~icks 1000 to 3000) - rest of orbit use masks as outlined above 6) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface 7) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 polar and 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 10) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time; 11) 10 days worth of orbits loaded NOTE: recovered from p2367.img errors with this upload p2488.img notes: 1) IMC patch on board, angles reversed - no IMC used in upload 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 4) for realtime orbits full spatial, full spectral for entire orbit 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 polar(N) and 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time; 10) 10 days worth of orbits loaded p2500.img notes: 1) IMC patch on board, angles reversed - IMC used in upload 2) PROM IMC table loaded and used 3) optical switch 00 4) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 5) for realtime orbits full spatial, full spectral for entire orbit 6) one orbit (not realtime) IMC used for all nadir observations except for epf; - test of IMC on ock 2506 7) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface 8) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 9) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 10) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) 1 equatorial mosaic added on alb_ref orbit (once per day) - pnt_angles = +-45, +-30, 0; ten icks at each angle, built by hand, removed equatorial space/ref set to accommodate mosaic 12) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 13) 10 days worth of orbits loaded ERROR: warmstart during upload (bad mission plan checksum), upload accepted by instrument - caused spectral mask to be applied to dayside nadir data p2548.img notes: 1) IMC patch on board, angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) 4) for realtime orbits full spatial, full spectral for entire orbit 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 5N and 15N once per day on consecutive orbits - pnt_angles = +-60,+-50,+-40,+-30,+-20,+-10,0; 5 icks each angle removed equatorial space/ref set to accommodate dense epf 10) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 11) 10 days worth of orbits loaded p2597.img notes: 1) IMC patch on board, angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ock 2607 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day - timing error detected, corrected by hand (moved all epf observations by adding 60 icks/120 sec to start ick) 10) dense epf- 5N and 15N once per day on consecutive orbits, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, multiple icks each angle as output by Michael's software: most looks right after each other, so built single overlay sequence instead of multiple individual overlays 11) trial new dense epf: 5N on ock 2599, 15N on ock 2600 12) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 13) shifted mosaic start icks by 20 in towards 0 degree look, trial by hand, not expected to work! 14) 10 days worth of orbits loaded ERROR: dense epf truncated by space/ref look, mosaic angles wrong p2647.img notes: 1) IMC patch on board, angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets; science campaign A ends during this upload will get less realtime coverage 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ock 2691 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt_angle = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) shifted mosaic times back to original, reversed angles 13) 10 days worth of orbits loaded p2744.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets; science campaign A ends during this upload will get less realtime coverage 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 2775 and 2859 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees; removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) mosaic identical to p2647.img 13) solar array motion test on ock 2803: will stop both SAM and SAP independently and together with HGA moving to assess noise effect on TES data; we will look at space for 5 min prior to start of test, for entire 31 minutes of test, and for ~5 minutes after test completes 14) 12 days worth of orbits loaded p2792.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets; science campaign A ends during this upload will get less realtime coverage 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ock 2859 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees; removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) mosaic removed 13) solar array motion test on ock 2803: will stop both SAM and SAP independently and together with HGA moving to assess noise effect on TES data; we will look at space for 5 min prior to start of test, for entire 31 minutes of test, and for ~5 minutes after test completes 14) 8 days worth of orbits loaded p2828.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 2859 and 2943 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees; removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) no mosaics 13) 12 days worth of orbits loaded p2914.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 2955 and 3039 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees; removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) no mosaics 13) 12 days worth of orbits loaded p3012.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 3039 and 3123 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) no mosaics 13) noise test: replace limb/epf looks on one orbit with 10 icks -90 degree pnt_angle throughout entire orbit; will assess solar panel rate differences (.051 dayside/.12 nightside) on noise - ocks 3014, 3026 14) 12 days worth of orbits loaded p3085.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 3123 and 3219 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt-angle = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) no mosaics 13) solar panel test trial-run: background seq stare -90 for 20 minutes then space/ref triplet - repeats for entire orbit; overlay of 4 sets of interferograms (detector 2, 5 consecutive icks) spaced to occur at times relative to when panels will be motionless and HGA will be stopped - testing on realtime ock 3088, and normal ock 3093 for buffer assessment of interferograms 14) 12 days worth of orbits loaded ERROR: limb scans ick 400-800 have been replaced by space/ref sets; decompiled upload commands indicate this scheduling error occurred during radiation of commands to TES p3147.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ock 3219 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt-angle = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) no mosaics 13) solar panel test : S&E1 data collection type, stare -90 for 20min then space/ref triplet - repeats for entire orbit; no interferograms (buffer problems in S&E1), will start data collection at 1999-190/13:30:00 and end at 1999-190/17:45:50, test times 190/13:36:08 to 190/17:38:44 according to mz011a.pef 14) 12 days worth of orbits loaded p3257.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets - limb fixes done to eliminate epf timing errors, truncations, and one space ref set error 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 3291 and 3387 on this build) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 10) doubles for ocks 3266-3289, moved dense epf's out of doubles 11) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, removed equatorial space/ref set to accommodate dense epf - moved one set of dense epf's out of doubles, this change was made for one set only 12) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 13) no mosaics 14) 12 days worth of orbits loaded WARNING: excessive number of warmstarts ocks 3266 - 3289, TES having lots of trouble with doubles (not enough icks for mirror movements); all observations were doubles -- surface, limbs, epf, refs; luckily - no coldstart occurred p3356.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt-angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) mosaics built by Michael's new tool, once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1 degree square coverage 13) only surface looks and space/refs for 12 orbits of polar offpoint [MOLA observations of geographic poles], will also be in CSA_backup mode for ~one day 14) 12 days worth of orbits loaded p3441.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface, - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 3459 and 3543) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt_angle = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) mosaics (5 x 13) built by Michael's new tool, once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1.5 lat x 1 long degree coverage 13) doubles on ock 3442 to test for warm start - added single idle after bb_ref 14) 12 days worth of orbits loaded p3526.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -30 to +90 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface, - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 3543 and 3627) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar, 1 nightside epf per day (on alb_ref orbit); 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) mosaics (5 x 13) done once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1.5 lat x 1 long degree coverage 13) OTM3 maneuver on ocks 3588 and 3589, doing space_ref looks for entire OTM (limb looks and EPFs removed) 14) doubles removed 15) 12 days worth of orbits loaded p3601.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -60 to +60 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface, - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) shift limbs by 5 degrees to avoid gores, limbs within 20 icks of epfs were removed 7) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 3639 and 3723) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 10) dense epf- 5N and 15N once every third day on consecutive orbits, - pnt_angle = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees, removed equatorial space/ref set to accommodate dense epf 11) space_ref_long only on regular "a" orbits (five times a day), at south polar space/ref time 12) mosaics (5 x 13) done once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1.5 lat x 1 long degree coverage 13) new solar panel array motion stepping implemented by spacecraft team removed limb looks occurring during .24 deg/sec motion times; moved nightside epf to orbit with no nightside Solar Array motion 14) OTM removed 15) 12 days worth of orbits loaded p3687.img notes: 1) IMC patch on board - angles reversed 2) imc test once per day - planet/space looks alternate with interferograms on space looks once per day - ock 3687 3) optical switch 00 4) surface = -60 to +60 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 5) for realtime orbits full spatial, full spectral for entire orbit - long packets 6) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface, - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 nadir looks between set for once per week repeat (ocks 3723 and 3807) 9) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 10) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- one dense epf targeted every third day, - pnt_angle = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 12) space_ref_long only on regular "a" orbits changed from being run five times a day to being run twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) 13) mosaics (5 x 13) done once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1.5 lat x 1 long degree coverage 14) reduced 10 ick space looks from 5 orbits per day to 1 orbit - 2 sets: one during Solar Array motion, one during quiet period 15) 12 days worth of orbits loaded ERROR: many limbs incorrectly observed as +60 degree epf set; decompiler shows upload file had no errors, indicating that error occurred during radiation of file to TES (error identified 10/1/99) p3773.img notes: 1) IMC patch on board - angles reversed 2) optical switch 00 3) day surface = -60 to +60 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: most forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - aft limbs at +10 lat (a orbit) and +70 lat (b orbit), 100 km height, 1/2 degree steps, padded by one look at surface, no space or +75 look angle at start, steps from top to surface, - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) 7) continuous limb look - with 3 nadir looks between set for once per week repeat cont_limb moved from 30S - 90N to 90S - 30N (ocks 3807 and 3891) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 10) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 11) space_ref_long only on regular "a" orbits changed from being run five times a day to being run twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) 12) mosaics (5 x 13) done once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1.5 lat x 1 long degree coverage 13) 12 days worth of orbits loaded p3857.img notes: 1) IMC patch deleted by coldstart - angles reversed back to nominal mapping spacecraft coordinates 2) optical switch 00 3) day surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 4) for realtime orbits full spatial, full spectral for entire orbit - long packets 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 6) limbs every 10 degrees, alternate orbits (a and b) 7) continuous limb look - with 3 nadir looks between set for once per week repeat cont_limb 90S - 30N (ocks 3891, 3975) 8) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 9) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 10) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 11) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion, one during HGA parked time 12) mosaics (5 x 13) done once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1.5 lat x 1 long degree coverage 13) imc test on ock 3867, using old imc (steps wrong way), test looks at nadir and -90, using imc on and off sets 14) 4 days of pre-set-orb contingency orbits, 12 days worth of orbits loaded for post set-orb p3944.img notes: 1) optical switch 00 2) surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 nadir looks between set for once per week repeat cont_limb 90S - 30N (ocks 3975,4059) 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angle = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion, one during HGA parked time 11) mosaics (5 x 13) done once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1.5 lat x 1 long degree coverage 12) 12 days loaded NOTE: forgot msc table edit to shift wavenumber sample return data reprocessed to accommodate error, p3969.img upload used to load wavenumber shift table edit p3969.img notes: 1) optical switch 00 2) surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 nadir looks between set for once per week repeat cont_limb 90S - 30N (ocks 3975, 4059) 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion, one during HGA parked time 11) mosaics (5 x 13) done once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1.5 lat x 1 long degree coverage 12) msc table edit added to adjust for wavelength shift in data 13) 12 days worth of orbits loaded NOTE: instrument warmstart - bad mission plan checksum; reprocessed data ocks 3995-4006; bad space looks relabeled "N" to exclude from calibration p4005.img notes: 1) optical switch 00 2) surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets - maximum 4 interferograms near subsolar point, detector 2, one minute between interferograms [for mini_tes] 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 nadir looks between set for once per week repeat cont_limb 90S - 30N (ocks 3975, 4059) 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion, one during HGA parked time 11) mosaics (5 x 13) done once per day, varying in latitude [-12,-9,-6,-3,0,3 degrees]; attempting 1.5 lat x 1 long degree coverage 12) white rock mosaic, minimizing emission angle changes, maximizing detector overlap, ock 4014 13) 12 days worth of orbits loaded NOTE: reprocessed data ocks 3995-4006; bad space looks relabeled "N" to exclude from calibration p4103.img notes: 1) optical switch 00 2) day surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets - maximum 4 interferograms near subsolar point, detector 2, one minute between interferograms [for mini_tes] 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle); - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 nadir looks between set for once per week repeat cont_limb 90S - 30N (ocks 3975, 4059) 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion and one during HGA parked time 11) mosaics - latitude band set 5 x 13, single scan, 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 attempting 1.5 lat x 1 long degree coverage 12) moved limb looks out of solar array motion periods; times change by ~3 icks/day, update every upload 13) 14 days worth of orbits loaded - trying to avoid conflict with MCO MOI and critical start of aerobraking p4214.img notes: 1) optical switch 00 2) day surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets - maximum 4 interferograms near subsolar point, detector 2, one minute between interferograms [for mini_tes] 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion and one during HGA parked time 11) mosaics - latitude band set 5 x 13, single scan, 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 attempting 1.5 lat x 1 long degree coverage 12) moved limb looks out of solar array motion periods; times change by ~3 icks/day, update every upload 13) 12 days worth of orbits loaded p4285.img notes: 1) optical switch 00 2) day surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets - maximum 4 interferograms near subsolar point, detector 2, one minute between interferograms [for mini_tes] 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion and one during HGA parked time 11) mosaics - latitude band set 5 x 13, single scan, 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 attempting 1.5 lat x 1 long degree coverage 12) moved limb looks out of solar array motion periods; times change by ~3 icks/day, update every upload 13) 12 days worth of orbits loaded p4359.img notes: 1) optical switch 00 2) day surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets - maximum 4 interferograms near subsolar point, detector 2, one minute between interferograms [for mini_tes] 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion and one during HGA parked time 11) mosaics - - latitude band set 5 x 13, single scan, dayside: 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 - new tools to target and build dayside (5x13) mosaics: W. Hematite, ock 4430; Aram Chaos, ock 4418 12) moved limb looks out of solar array motion periods; times change by ~3 icks/day, update every upload - AEM/pef times out of sync, will be fixed next week so added all limbs back into schedules and moved long ref to near equator crossing 13) 12 days worth of orbits loaded p4410.img notes: 1) optical switch 00 2) day surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets - maximum 4 interferograms near subsolar point, detector 2, one minute between interferograms [for mini_tes] 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion and one during HGA parked time 11) mosaics - - latitude band set 5 x 13, single scan, dayside: 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 - new tools to target and build dayside (5x13) mosaics: W. Hematite, ock 4430; Aram Chaos, ock 4418; White rock; Isisdis rim 12) moved limb looks out of solar array motion periods; times change by ~3 icks/day, update every upload - AEM/pef times out of sync, will be fixed next week so added all limbs back into schedules and moved long ref to near equator crossing 13) 12 days worth of orbits loaded ERROR: ACE radiated upload too early, instrument warmstarted due to bit hit during transmission, TES stared at nadir until correct equator crossing occurred [instrument recovered at that point] - staring at nadir with no reference looks because flush queue removed all previous commands and new ones had not been initiated p4457.img notes: 1) optical switch 00 2) day surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets - maximum 4 interferograms near subsolar point, detector 2, one minute between interferograms [for mini_tes] 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to have one set during HGA motion and one during HGA parked time 11) mosaics - - latitude band set 5 x 13, single scan, dayside: 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 - new tools to target and build dayside (5x13) mosaics: Hematite2, ock 4533 12) solar array motion periods times change by ~3 icks/day all limbs back into schedules and moved long ref to near equator crossing 13) 12 days worth of orbits loaded p4543.img notes: 1) optical switch 00 2) day surface = -80 to +40 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) - four dense epf's added to investigate dust activity Hellas, ock 4566; Argyre, ock 4545; bright terrain northern hemisphere, ock 4571; bright terrain southern hem, ock 4552 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - added additional set on orbit 9 (same places as above), hope to to have one set during HGA motion and one during HGA parked time 11) mosaics - - latitude band set 5 x 13, single scan, dayside: 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 - targeted 5 x 13, single scan, dayside: W. Hematite, ock 4581; Aram Chaos, ock 4594; Hebes Chasm, ock 4596; - targeted 5 x 13, single scan, nightside: W. hematite, ock 4550; Aram Chaos, ock 4625; 12) 12 days worth of orbits loaded p4630.img notes: 1) optical switch 00 2) day surface = -90 to +30 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) - fixed 60N dense epf (had been doing single set instead of full) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) mosaics - - latitude band set 5 x 13, single scan, dayside: 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 - targeted 5 x 13, single scan, dayside: Hebes Chasm, ock 4684; Viking2, ock 4689; Herschel, ock 4702; Dao Vallis, ock 4716 - TRIAL targeted 3 x 45, single scan, nightside, cloud: (3 strips of 45 icks at ~+/- 45 degrees emission angle and 0 emission angle, attempting a 5 degree latitude size mosaic with gores between columns) Olympus Mons, ock 4711 12) 12 days worth of orbits loaded p4704.img notes: 1) optical switch 00 2) day surface = -90 to +30 degrees lat, full spectral, full spatial night = +60 to -60 degrees lat, spectral mask, full spatial poles = rest of lats, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -62,-60,-45,0,45,60,62; 5 icks at each angle 8) 1 N-polar, 1 S-polar (alb_ref orbit), 1 nightside epf (orbit 11) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- one dense epf targeted every third day, - pnt_angles = +-60,+-58,+-55,+-54,+-50 etc to 0 degrees - it will take ~ 1 month to cycle through the full dayside latitudinal coverage (75S, 60S, 45S, 30S, 15S, 0, 15N, 30N, 45N, 60N, 75N) 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) mosaics - - latitude band set 5 x 13, single scan, dayside: 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 - targeted 5 x 13, single scan, dayside: Dao Vallis, ock 4716; Adamas Layrintis, ock 4753; Proctor Crater, ock 4756; Western Hematite, ock 4757; ML1, ock 4759; Nili, ock 4767; Hematite3, ock 4772; - targeted 5 x 13, single scan, nightside: Aram Chaos, ocks 47134714]; Hematite5, ock 4766; W. Hematite, ocks 4789 4790 - TRIAL targeted 3 x 45, single scan, nightside, cloud: (3 strips of 45 icks at ~+/- 45 degrees emission angle and 0 emission angle, attempting a 5 degree latitude size mosaic with gores between columns) Olympus Mons, ock 4711 12) 12 days worth of orbits loaded 13) spacecraft command sequence mm009 not released prior to upload, last five days contain no real time orbits (no info to assign these days) p4814.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) three orbits of double scan surface coverage (nadir only, limbs remain single-scan) every fourth day centered on MPL landing site closest groundtrack orbit that day 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 6) limb set orbits (a and b) moved back 2.5 degrees (-25 icks) 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 9) continuous limbs for MPL - fore set covers ~47 degrees latitude starting at sub-spacecraft latitude of -46(desc) then switching to aft set covering additional ~47 degrees latitude finishing at sub-spacecraft lat of -46(asc) - pnt_angles 70, 68.5 to 62.5 in 0.41 degree steps, 3 icks at 50 degrees 10) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref1 orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- removed from upload - scheduling conflicts with new MPL coverage strategy 13) MPL epf set - 2 double-sided (fore-nadir-aft) sets, one at -76(desc) degrees lat, one at -76(asc) degrees lat 14) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 15) mosaics - - latitude band set 5 x 13, single scan, dayside: replaced by double-scan mosaics (see next...) - latitude band set 5 x 7, double scan, column averaged (det_mask 5)dayside: 1 per day cycling through latitudes -25, -22, -19, -16, -13, 9 - targeted 5 x 13, single scan, dayside: Arsia Caldera, ock 4922; Hematite2, ock 4860; Gusev crater, ock 4952; - targeted 5 x 13, single scan, nightside: none 16) Multi day schedule to provide MPL landing site coverage/support: 1st day - normal (regular limb/epf/surface) 2nd day - MPL (regular orbit - MPL limb orbit - regular orbit - MPL epf orbit - regular orbit - etc) 3rd day - normal with 3 double surface orbits 4th day - MPL [2nd and 4th days alternate so closest groundtrack orbit to lander switches between MPL-limb and MPL-epf] 17) 12 days worth of orbits loaded ERROR: bit hit(?) during transmission affected double space/ref set - no double scan black body ref collected so cannot calibrate any double-scan observations from this upload ERROR: warmstart (1 per orbit for three orbits) at same location during space reference (double and single scans), did not occur in other locations where sequence was executing; will add additional idle ick in attempt to eradicate warmstart p4887.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) three orbits of double scan surface coverage (nadir only, limbs remain single-scan) every fourth day centered on MPL landing site closest groundtrack orbit that day 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 6) limb set orbits (a and b) moved back 2.5 degrees (-25 icks) 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 9) continuous limbs for MPL - fore set covers ~47 degrees latitude starting at sub-spacecraft latitude of -46(desc) then switching to aft set covering additional ~47 degrees latitude finishing at sub-spacecraft lat of -46(asc) - angles 70, 68.5 to 62.5 in 0.41 degree steps, 3 icks at 50 degrees - fixed stop time for limb, ends at ick 1375 now 10) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref1 orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- none in this upload 13) MPL epf set - 2 double-sided (fore-nadir-aft) sets, one at -76 degrees lat descending, one at -76 degrees lat ascending; fixed second set (ascending) to be centered on MPL latitude 14) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 15) mosaics - - latitude band set 5 x 13, single scan, dayside: replaced by double-scan mosaics (see next...) - latitude band set 5 x 7, double scan, column averaged (det_mask 5)dayside: 1 per day cycling through latitudes -25, -22, -19, -16, -13, 9 - targeted 5 x 13, single scan, dayside: Arsia Caldera, ock 4922; Gusev crater, ock 4952; - targeted 5 x 13, single scan, nightside: none 16) Multi day schedule to provide MPL landing site coverage/support: 1st day - normal (regular limb/epf/surface) 2nd day - MPL (regular orbit - MPL limb orbit - regular orbit - MPL epf orbit - regular orbit - etc) 3rd day - normal with 3 double surface orbits 4th day - MPL [2nd and 4th days alternate so closest groundtrack orbit to lander switches between MPL-limb and MPL-epf] 17) changed space/ref single/double set to address warmstarts and lack of blackbody looks - added additional idle icks between space and ref triplets 18) 12 days worth of orbits loaded ERROR: still no blackbody looks, TES unable to alternate between single and double scans within single sequence (?) no double scan black body ref collected so cannot calibrate any double- scan observations from this upload ERROR: warmstart (1 per orbit for three orbits) at same location during space reference (double and single scans), did not occur in other locations where sequence was executing p4954.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) three orbits of double scan surface coverage (nadir only, limbs remain single-scan) every fourth day centered on MPL landing site closest groundtrack orbit that day 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 6) limb removed from 76S lat position - for MPL surface viewing 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 9) continuous limbs for MPL - fore set covers ~47 degrees latitude starting at sub-spacecraft latitude of -46(desc) then switching to aft set covering additional ~47 degrees latitude finishing at sub-spacecraft lat of -46(asc) - angles 70, 68.5 to 62.5 in 0.41 degree steps, 3 icks at 50 degrees 10) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref1 orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- none in this upload 13) MPL epf set - 2 double-sided (fore-nadir-aft) sets, one at -76 degrees lat descending, one at -76 degrees lat ascending 14) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 15) mosaics - - latitude band set 5 x 13, single scan, dayside: replaced by double-scan mosaics (see next...) - latitude band set 5 x 7, double scan, column averaged (det_mask 5)dayside: 1 per day cycling through latitudes -25, -22, -19, -16, -13, 9 - targeted 5 x 13, single scan, dayside: Hematite4, ock 5003 - targeted 5 x 13, single scan, nightside: none - 3 strips x 45 icks, single scan, dayside cloud/volc: Elysium, ock 5003 - 3 strips x 45 icks, single scan, nightside cloud/volc: Elysium, ock 5009; Olympus, ock 5044 16) Multi day schedule to provide MPL landing site coverage/support: 1st day - normal (regular limb/epf/surface) 2nd day - MPL (regular orbit - MPL limb orbit - regular orbit - MPL epf orbit - regular orbit - etc) 3rd day - normal with 3 double surface orbits 4th day - MPL [2nd and 4th days alternate so closest groundtrack orbit to lander switches between MPL-limb and MPL-epf] 17) new space/ref single/double sequence: - 3 single space, 3 single bb_ref, 3 double space, 3 double bb_ref, 2 idle icks - hopefully will fix the missing bb_ref problem and the warmstart problem 18) 12 days worth of orbits loaded NOTE: this upload fixed the double-bb_ref and warmstart problem ERROR: error in Elysium, ock 5003 mosaic schedule caused TES to warmstart; no data collected for this cloud/volc mosaic p5082.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) three orbits of double scan surface coverage (nadir only, limbs remain single-scan) every fourth day centered on MPL landing site closest groundtrack orbit that day 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 6) limb removed from 76S lat position - for MPL surface viewing 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 9) continuous limbs for MPL - fore set covers ~47 degrees latitude starting at sub-spacecraft latitude of -46(desc) then switching to aft set covering additional ~47 degrees latitude finishing at sub-spacecraft lat of -46(asc) - angles 70, 68.5 to 62.5 in 0.41 degree steps, 3 icks at 50 degrees 10) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref1 orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- none in this upload 13) MPL epf set - 2 double-sided (fore-nadir-aft) sets, one at -76 degrees lat descending, one at -76 degrees lat ascending 14) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 15) mosaics - - latitude band set 5 x 7, double scan, column averaged (det_mask 5)dayside: 1 per day cycling through latitudes -25, -22, -19, -16, -13, 9 - targeted 5 x 13, single scan, dayside: none - targeted 5 x 13, single scan, nightside: none 16) Multi day schedule to provide MPL landing site coverage/support: 1st day - normal (regular limb/epf/surface) 2nd day - MPL (regular orbit - MPL limb orbit - regular orbit - MPL epf orbit - regular orbit - etc) 3rd day - normal with 3 double surface orbits 4th day - MPL [2nd and 4th days alternate so closest groundtrack orbit to lander switches between MPL-limb and MPL-epf] 17) new space/ref single/double sequence: - 3 single space, 3 single bb_ref, 3 double space, 3 double bb_ref, 2 idle icks - fixes the missing bb_ref problem and the warmstart problem 18) 26 days worth of orbits loaded p5132.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) three orbits of double scan surface coverage (nadir only, limbs remain single-scan) every fourth day centered on MPL landing site closest groundtrack orbit that day 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 6) limb removed from 76S lat position - for MPL surface viewing 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 9) continuous limbs for MPL - fore set covers ~47 degrees latitude starting at sub-spacecraft latitude of -46(desc) then switching to aft set covering additional ~47 degrees latitude finishing at sub-spacecraft lat of -46(asc) - angles 70, 68.5 to 62.5 in 0.41 degree steps, 3 icks at 50 degrees 10) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref1 orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- none in this upload 13) MPL epf set - 2 double-sided (fore-nadir-aft) sets, one at -76 degrees lat descending, one at -76 degrees lat ascending 14) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 15) mosaics - - latitude band set 5 x 7, double scan, column averaged (det_mask 5)dayside: 1 per day cycling through latitudes -25, -22, -19, -16, -13, 9 16) Multi day schedule to provide MPL landing site coverage/support: 1st day - normal (regular limb/epf/surface) 2nd day - MPL (regular orbit - MPL limb orbit - regular orbit - MPL epf orbit - regular orbit - etc) 3rd day - normal with 3 double surface orbits 4th day - MPL [2nd and 4th days alternate so closest groundtrack orbit to lander switches between MPL-limb and MPL-epf] 17) space/ref single/double sequence: - 3 single space, 3 single bb_ref, 3 double space, 3 double bb_ref, 2 idle icks 18) 21 days worth of orbits loaded NOTE: Spacecraft to CSA/backup mode on ock 5142: no more equator crossing broadcasts until MHSA mode resumes - timing will drift p5155.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) three orbits of double scan surface coverage (nadir only, limbs remain single-scan) every fourth day centered on MPL landing site closest groundtrack orbit that day 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 6) limb removed from 76S lat position - for MPL surface viewing 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 9) continuous limbs for MPL - fore set covers ~47 degrees latitude starting at sub-spacecraft latitude of -46(desc) then switching to aft set covering additional ~47 degrees latitude finishing at sub-spacecraft lat of -46(asc) - angles 70, 68.5 to 62.5 in .41 degree steps, 3 icks 50 deg. 10) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref1 orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- none in this upload 13) MPL epf set - 2 double-sided (fore-nadir-aft) sets, one at -76 degrees lat descending, one at -76 degrees lat ascending 14) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 15) mosaics - - latitude band set 5 x 7, double scan, column averaged (det_mask 5)dayside: 1 per day cycling through latitudes -25, -22, -19, -16, -13, 9 16) Multi day schedule to provide MPL landing site coverage/support: 1st day - normal (regular limb/epf/surface) 2nd day - MPL (regular orbit - MPL limb orbit - regular orbit - MPL epf orbit - regular orbit - etc) 3rd day - normal with 3 double surface orbits 4th day - MPL [2nd and 4th days alternate so closest groundtrack orbit to lander switches between MPL-limb and MPL-epf] 17) space/ref single/double sequence: - 3 single space, 3 single bb_ref, 3 double space, 3 double bb_ref, 2 idle icks 18) Due to MOC imaging of the MPL landing site, the following 7 ocks will stare at surface only and have the south polar space_ref look removed: 5155, 5159, 5160, 5167, 5172, 5179, 5180 19) EQTX command sent up due to eqtx broadcast being terminated until doy 1999-359 20) 19 days worth of orbits loaded NOTE: Spacecraft to CSA/backup mode on ock 5142: no more equator crossing broadcasts until MHSA mode resumes - timing will drift p5209.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) three orbits of double scan surface coverage (nadir only, limbs remain single-scan) every fourth day centered on MPL landing site closest groundtrack orbit that day 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 6) limb removed from 76S lat position - for MPL surface viewing 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 9) continuous limbs for MPL - fore set covers ~47 degrees latitude starting at sub-spacecraft latitude of -46(desc) then switching to aft set covering additional ~47 degrees latitude finishing at sub-spacecraft lat of -46(asc) - angles 70, 68.5 to 62.5 in .41 degree steps, 3 icks 50 deg. 10) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref1 orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- none in this upload 13) MPL epf set - 2 double-sided (fore-nadir-aft) sets, one at -76 degrees lat descending, one at -76 degrees lat ascending 14) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 15) mosaics - - latitude band set 5 x 7, double scan, column averaged (det_mask 5)dayside: 1 per day cycling through latitudes -25, -22, -19, -16, -13, 9 16) Multi day schedule to provide MPL landing site coverage/support: 1st day - normal (regular limb/epf/surface) 2nd day - MPL (regular orbit - MPL limb orbit - regular orbit - MPL epf orbit - regular orbit - etc) 3rd day - normal with 3 double surface orbits 4th day - MPL [2nd and 4th days alternate so closest groundtrack orbit to lander switches between MPL-limb and MPL-epf] 17) space/ref single/double sequence: - 3 single space, 3 single bb_ref, 3 double space, 3 double bb_ref, 2 idle icks 18) MOC stopped imaging MPL landing site, removed moc_orbits schedule 19) EQTX command sent up due to eqtx broadcast being terminated until doy 1999-359 20) 15 days worth of orbits loaded ERROR: typo in ground document led to incorrect timing/orbit number TES orb number out of sync with TES ock NOTE: Spacecraft to CSA/backup mode on ock 5142: no more equator crossing broadcasts until MHSA mode resumes - timing will drift p5217.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) three orbits of double scan surface coverage (nadir only, limbs remain single-scan) every fourth day centered on MPL landing site closest groundtrack orbit that day 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 6) limb removed from 76S lat position - for MPL surface viewing 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 9) continuous limbs for MPL - fore set covers ~47 degrees latitude starting at sub-spacecraft latitude of -46(desc) then switching to aft set covering additional ~47 degrees latitude finishing at sub-spacecraft lat of -46(asc) - angles 70, 68.5 to 62.5 in .41 degree steps, 3 icks 50 deg. 10) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref1 orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- none in this upload 13) MPL epf set - 2 double-sided (fore-nadir-aft) sets, one at -76 degrees lat descending, one at -76 degrees lat ascending 14) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 15) mosaics - - latitude band set 5 x 7, double scan, column averaged (det_mask 5)dayside: 1 per day cycling through latitudes -25, -22, -19, -16, -13, 9 16) Multi day schedule to provide MPL landing site coverage/support: 1st day - normal (regular limb/epf/surface) 2nd day - MPL (regular orbit - MPL limb orbit - regular orbit - MPL epf orbit - regular orbit - etc) 3rd day - normal with 3 double surface orbits 4th day - MPL [2nd and 4th days alternate so closest groundtrack orbit to lander switches between MPL-limb and MPL-epf] 17) space/ref single/double sequence: - 3 single space, 3 single bb_ref, 3 double space, 3 double bb_ref, 2 idle icks 18) Due to MOC imaging of the MPL landing site, the following 6 ocks will stare at surface only and have the south polar space_ref look removed: 5217, 5218, 5229, 5230, 5243, 5261 19) EQTX command sent up due to eqtx broadcast being terminated until doy 1999-361 20) 15 days worth of orbits loaded ERROR: TES orb number still out of sync with TES ock (due to ground document typo) NOTE: Spacecraft to CSA/backup mode on ock 5142: no more equator crossing broadcasts until MHSA mode resumes - timing will drift; Spacecraft back to MHSA mode prior to ock 5266: started receiving eqtrx broadcasts, no more timing drift p5368.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 8) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 75S to 75N, 15 degree steps, one every third day 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) mosaics - latitude band set 5 x 13, single scan, 1 per day cycling through latitudes -12, -9, -6, -3, 0, 3 12) 12 days worth of orbits loaded 13) set_orbit command sent to recover from out-of-sync problem NOTE: out-of-sync problem fixed by upload p5462.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 8) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 75S to 75N, 15 degree steps, one every third day 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) mosaics - latitude band set 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9 12) 12 days worth of orbits loaded 13) stare nadir only with space/reference sets on ock 5437: Pathfinder imaging opportunity, spacecraft will be slewed NOTE: did not have MPL imaging orbits prior to upload; atmospheric observations those four orbits will be useless NOTE: spacecraft will be in CSA/backup mode from doy 2000-009 to 2000-012, TES will not receive eqtrx broadcasts during that period; timing will drift. p5502.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 8) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 75S to 75N, 15 degree steps, one every third day 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) mosaics - latitude band set 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9 12) mosaics - - targeted 5 x 13, single scan, dayside: Korolev Crater, ock 5568; Viking1, ock 5601 13) 12 days worth of orbits loaded 14) stare nadir only with space/reference sets on ock 5525 (Pathfinder imaging opportunity) and on ocks 5532 and 5557 (MPL site imaging); spacecraft will be slewed NOTE: spacecraft will be in CSA/backup mode from doy 2000-016 to 2000-019, TES will not receive eqtrx broadcasts during that period; timing will drift - MOC imaging both MPL and MPF sites p5584.img notes: 1) optical switch 00 2) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 8) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 75S to 75N, 15 degree steps, one every third day 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) mosaics - latitude band set 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9 12) mosaics - - targeted 5 x 13, single scan, dayside: Viking1, ock 5601; Becquerel Cr., ock 5625; Aram Chaos, ock 5663; W. Candor Chasm, ock 5665 - 3 x 45, single scan, dayside, cloud/volc: Arsia, ock 5654; Elysium, ock 5657; Olympus, ock 5692; 13) 12 days worth of orbits loaded 14) no information on MPL/MPF targeting orbits, also nothing special done for MAG calibrations (affects only HGA and SA) p5670.img notes: 1) optical switch 00 2) MEDIUM data record rate (ocks 5670 - 5770) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets LOW data record rate (starting ock 5771 through next 9 months) day surface = -50 to +10 degrees lat, full spectral, full spatial night = +40 to -40 degrees lat descending orbit side, +10 to +50 degrees lat dayside, spectral mask, full spatial poles = -40 to -50(day) south pole, +50(day) to +40 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (20S) 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 8) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 75S to 75N, 15 degree steps, one every third day 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) mosaics - latitude band set 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9 12) mosaics - - targeted 5 x 13, single scan, dayside: Hebes Chasm, ock 5753 - 3 x 45, single scan, dayside, cloud/volc: Olympus, ock 5692 13) 12 days worth of orbits loaded 14) nothing done for MPL/MPF imaging or HGA testing p5756.img notes: 1) optical switch 00 2) MEDIUM data record rate (ocks 5756 - 5770) day surface = -66(desc) to +6(asc) degrees lat, full spectral, full spatial night = +54 to -66 degrees lat, spectral mask, full spatial poles = +6(asc) to +54(desc) degrees lat, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets LOW data record rate (starting ock 5771 through next 9 months) day surface = -50 to +10 degrees lat, full spectral, full spatial night = +40 to -40 degrees lat descending orbit side, +10 to +50 degrees lat dayside, spectral mask, full spatial poles = -40(desc) to -50(asc) south pole, +50(asc) to +40(desc) north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (20S) 3) for realtime orbits: full spatial, full spectral for entire orbit - long packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF NEW mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 8) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 75S to 75N, 15 degree steps, one every third day 10) space_ref_long twice per day on a single orbit: once in noise free zone (south pole) and once during Solar Array motion (nightside) - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) mosaics - - latitude band set 5 x 7, double scan, dayside: 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9 - latitude band set 5 x 13, single scan, nightside: build 6 per load, cycles from -60 to +30 lat in 3 degree steps 12) mosaics - - targeted 5 x 13, single scan, dayside: Gusev, ock 5782 - targeted 5 x 13, single scan, nightside: Ma'adim, ock 5776; Hebes, ocks 5784 5785; Viking2, ock 5802; Ophir, ocks 5809 5810; Hesp. windsteaks, ock 5816; 13) only 5 days of realtime orbits listed in pef's 14) 12 days worth of orbits loaded NOTE: buffer problems starting at ock 5771 - record to LRC, data loss due to full buffer on all ocks following 5771 p5818.img notes: 1) optical switch 00 2) buffer management trial period - changed from previous day surface = -50 to +10 degrees lat, full spectral, full spatial night = +30 to -30 degrees lat, spectral mask, full spatial poles = -30(desc) to -50(asc) south pole, +10(asc) to +30(desc) north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (20S) 3) for realtime orbits: full spatial, full spectral ick 0 to Npole, long packets; rest of orbit poles/short packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 8) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 75S to 75N, 15 degree steps, one every third day 10) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) mosaics - - latitude band set 5 x 7, double scan, dayside: 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - latitude band set 5 x 13, single scan, nightside: build 6 per load, cycles from -60 to +30 lat in 3 degree steps 12) mosaics - - targeted 5 x 7, double scan, dayside: Isidis, ock 5823 - targeted 5 x 13, single scan, dayside: W. Hematite, ock 5826 - targeted 5 x 13, single scan, nightside: Gusev, ock 5839; Hebes, ocks 5872 5873; W. Hematite, ock 5858; Hesp. windsteaks, ock 5841 13) only 7 days of realtime orbits listed in pef's 14) 12 days worth of orbits loaded NOTE: fixed double-scan reference set by removing epf look (second set was being truncated by epf look) p5903.img notes: 1) optical switch 00 2) buffer management trial period - changed from previous day surface = -45 to +5 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25(desc) to -45(asc) south pole, +5(asc) to +25(desc) north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (20S) 3) for realtime orbits: day surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 8) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 75S to 75N, 15 degree steps, one every third day 10) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) added double alb_ref to space_alb_ref sets - to calibrate bolometer data collected in double scan mode 12) mosaics - - latitude band set 5 x 7, double scan, dayside: 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - latitude band set 5 x 13, single scan, nightside: build 6 per load, cycles from -60 to +30 lat in 3 degree steps 13) mosaics - - targeted 5 x 7, double scan, dayside: Isidis, ock 5911 - targeted 5 x 13, single scan, dayside: Hematite2, ock 5929 - targeted 5 x 13, single scan, nightside: Viking1, ock 934; 14) only 7 days of realtime orbits listed in pef's 15) 12 days worth of orbits loaded NOTE: fixed limb set on orbit 4, no longer back to back at ick 205 WARNING: spacecraft anomaly resulted in loss of data for ocks 5906-5917 p5987.img notes: 1) optical switch 00 2) buffer management no change from previous day surface = -45 to +5 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25(desc) to -45(asc) south pole, +5(asc) to +25(desc) north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (20S) 3) for realtime orbits: day surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 5) limbs every 10 degrees, alternate orbits (a and b) 6) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 8) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 9) dense epf- 75S to 75N, 15 degree steps, one every third day 10) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 11) added double alb_ref to space_alb_ref sets - to calibrate bolometer data collected in double scan mode 12) mosaics - - latitude band set 5 x 7, double scan, dayside: 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - latitude band set 5 x 13, single scan, nightside: build 6 per load, cycles from -60 to +30 lat in 3 degree steps 13) mosaics - - targeted 5 x 7, double scan, dayside: Isidis, ock 5999 - targeted 5 x 13, single scan: none p6074.img notes: 1) optical switch 00 2) buffer management no change from previous day surface = -45 to +5 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (20S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) data loss: last day of beta supplement, three 4-orbit periods of earth point during fixed high gain (FHGA) - soft idle (sdm 0,1) used to keep empty buffer 5) one full day of nadir off pointing for MOLA polar coverage, - stare surface only with space/ref sets, daily surface-only double scan orbit during this period (ocks 6120-6131) 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 90S - 30N 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 13) added double alb_ref to space_alb_ref sets - to calibrate bolometer data collected in double scan mode 14) mosaics - - latitude band set 5 x 7, double scan, dayside: 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - latitude band set 5 x 13, single scan, nightside: build 6 per load, cycles from -60 to +30 lat in 3 degree steps [only 3 on this build] 15) mosaics - - targeted 5 x 7, double scan, dayside: Isidis, ock 6150 - targeted 5 x 13, single scan, dayside: White rock, ock 6152; W. Hematite, ock 6153; Korolev, ock 6166 16) 12 days worth of orbits loaded NOTE: spacecraft in CSA backup for duration of MOLA polar orbits and fixed high gain period. Timing will drift due to lack of equator crossing time broadcasts from PDS. This will affect ocks 6102 to ~6165. (See also p6098.img) p6098.img notes: 1) update of p6074.img ONLY CHANGE: record last day of beta supplement prior to start of MOLA polar orbits for playback on first day of next beta supplement sequence; according to p6074.img this period was going to be a data outage. p6161.img notes: 1) optical switch 00 2) buffer management no change from previous day surface = -45 to +5 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (20S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm018 FHGA (last day), mm020 beta supplement. (6 days), and mm022 FHGA (4 days). - soft idle (sdm 0,1) used to keep empty buffer during earth point periods of fixed high gain (FHGA) 5) double scan orbit, surface only ock 6199 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat. cont_limb 90S - 30N 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 13) added double alb_ref to space_alb_ref sets - to calibrate bolometer data collected in double scan mode 14) mosaics - - latitude band set 5 x 7, double scan, dayside: 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - latitude band set 5 x 13, single scan, nightside: build 6 per load, cycles from -60 to +30 lat in 3 degree steps [starting over at -60 on this build on last mosaic] 15) mosaics - - targeted 5 x 7, double scan, dayside: Isidis, ock 6238 - targeted 5 x 13, single scan, dayside: Korolev, ock 6166; Dao Vallis 2, ock 6200; Hesp. Paleolake, ock 6237 - targeted 5 x 13, single scan, nightside: Dusty, ock 6184; Sandy, ock 6202; Ma'adim Vallis, ock 6254 16) 12 days worth of orbits loaded NOTE: search mode command after FHGA did not get on board, spacecraft continues in CSA backup until sometime 2000-071 (3 extra days with no equator crossing broadcasts) -- timing will drift, mosaics will likely miss targets. p6232.img notes: 1) optical switch 00 2) moved to follow sub_solar_lat day surface = -35 to +15 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm022/mm023 beta supplement replan - soft idle (sdm 0,1) used to keep empty buffer during non-record/non-realtime periods - out of sync problems due to change from FHGA cause loss of data doy 2000-075 (all) and 2000-076 (parts) [ocks 6237-6251, 6254, 6255] 5) double scan orbit, surface only ock 6259 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N (changed) - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 13) added double alb_ref to space_alb_ref sets - to calibrate bolometer data collected in double scan mode 14) mosaics - - latitude band set 5 x 7, double scan, dayside: 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - latitude band set 5 x 13, single scan, nightside: mosaics removed from this upload in anticipation of 3 day double scan upload; will return to stepping on next single scan upload 15) mosaics - - targeted 5 x 7, double scan, dayside: Isidis, ock 6326 - targeted 5 x 13, single scan, dayside: Becquerel, ock 6279; Lobate Crater, ock 6325; Huygens, ock 6327 - targeted 5 x 13, single scan, nightside: Viking1, ock 6261; W. Hematite, ocks 6272 6273 16) 12 days worth of orbits loaded p6280.img notes: 1) optical switch 00 2) moved to follow sub_solar_lat day surface = -35 to +15 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial, short - short packets poles = rest of lats, spectral mask, spatial mask, short packets - short packets 4) upload covers spacecraft command sequences: mm023/mm024 beta supplement replan - soft idle (sdm 0,1) used to keep empty buffer during non-record/non-realtime periods 5) double scan orbits, includes limb observations ocks 6280 - 6318 6) double limbs: all forward looking, 1/2 degree steps from 68 to 63, 2 looks at each angle, 3 looks at 50 degrees - each limb in 100 sec in duration - "continuous" limb scan 3 times (12 orbits apart) - limb sets 20 degrees lat apart, alternating on orbit pairs 7) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 8) limbs every 10 degrees, alternate orbits (a and b) 9) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N (changed) - will alternate with cont_limb2 20S to 80N (nightside) 10) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- 75S to 75N, 15 degree steps, one every third day 13) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 14) added double alb_ref to space_alb_ref sets - to calibrate bolometer data collected in double scan mode 15) mosaics - - latitude band set 5 x 7, double scan, dayside: 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - latitude band set 5 x 13, single scan, nightside: mosaics removed from this upload in anticipation of 3 day double scan upload; will return to stepping on next single scan upload 16) mosaics - - targeted 5 x 7, double scan, dayside: Isidis, ock 6326 - targeted 5 x 13, single scan, dayside: Lobate Crater, ock 6325; Huygens, ock 6327 17) 8 days worth of orbits loaded p6332.img notes: 1) optical switch 00 2) moved to follow sub_solar_lat day surface = -35 to +15 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral, long - long packets night = +30 to -30 degrees lat, spectral mask, full spatial, short - short packets poles = rest of lats, spectral mask, spatial mask, short packets - short packets 4) upload covers spacecraft command sequences: mm024/mm025 beta supplement - testing detector/detector mask problems ocks 6334 - 6387 - using soft_idle for buffer management, no limb obs on test orbits, normal orbits between testing orbits for limited limb coverage during 4 day testing period 5) double scan orbit, surface only ock 6390 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N (changed) - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on orbit 9 (same places as above), one set during HGA motion and one during HGA parked time 13) added double alb_ref to space_alb_ref sets - to calibrate bolometer data collected in double scan mode 14) mosaics - - latitude band set 5 x 7, double scan, dayside: 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 15) mosaics - no single mosaics this upload (targeted or night bolo) 16) 12 days worth of orbits loaded p6368.img notes: 1) update of p6332.img ONLY CHANGE: additional detector/detector mask problem test (see item 4 above) to collect data with full spatial coverage and detector averaging. p6418.img notes: 1) optical switch 00 2) day surface = -35 to +15 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm026/mm027 beta supplement - MOC star imaging used for cobe5 test (off Mars nadir looks) - COBE5 = 35 icks at -90,-65,-40,-24,+24,+40 degrees pnt_angle and 70 icks at 0 degrees pnt_angle - MOC ocks 6426/27, 6452/53, 6480/81, 6504/05, 6528/29 - MOLA off points ocks 6536-6548 5) double scan orbit, surface only: ock 6474 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) added double alb_ref to space_alb_ref sets to calibrate bolometer data collected in double scan mode 14) mosaics - 5 x 7, double scan 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: Isidis, ock 6477 15) mosaics - no night bolo this upload due to location of MOC orbits - targeted 5 x 13, single scan, dayside: Herschel, ock 6425; Dao Vallis1, ock 6439; White Rock, ock 6479 16) 12 days worth of orbits loaded p6440.img notes: 1) update to p6418.img upload, ONLY CHANGES: polar detector mask changed from 1 to 2; testing indicates problem with mask 1, but no problem with mask 2 p6504.img notes: 1) optical switch 00 2) day surface = -35 to +15 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm028/mm029 beta supplement - MOC star imaging used for cobe5 test (off mars nadir looks) - COBE5 = 35 icks at -90,-65,-40,-24,+24,+40 degrees pnt_angle and 70 icks at 0 degrees pnt_angle - MOC ock 6504/05, 6528/29 - MOLA off points ock 6536-6548 5) double scan orbit, surface only: ock 6559 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode 14) new south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: Isidis, ock 6565 16) mosaics - no night bolo this upload due to location of MOC orbits - targeted 5 x 13, single scan, dayside: Dao Vallis2, ock 6527; Aram Chaos, ock 6556; Hesperian paleolake, ock 6564; W. Hematite, ock 6568; Viking1, ock 6582 - targeted 5 x 13, single scan, nightside: Gusev, ock 6581; "dusty", ock 6599 17) 12 days worth of orbits loaded p6534.img notes: 1) update to p6504.img upload 2) new strategy for MOLA polar offpoint orbits - full spatial, full spectral +/- 60 degrees lat (over poles); rest of orbit soft_idle (no spectra) for buffer management over course of 24 hours off pointing - space/ref sets in normal positioning - fore and aft limbsets targeted at each pole, no other limb data during orbit 3) mosaic targeting: changed from single scan mode to double scan mode Aram Chaos, ock 6556; W. Hematite, ock 6567 p6588.img notes: 1) optical switch 00 2) day surface = -35 to +15 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm030/mm031 beta supplement 5) double scan orbit, surface only: ock 6643 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: W. Hematite, ock 6631; Aram Chaos, ock 6644 16) mosaics - no night bolo this upload due to targets location - targeted 5 x 13, single scan, dayside: Becquerel, ock 6606; Korolev, ock 6637; Hebes, ock 6646 - targeted 5 x 13, single scan, nightside: "dusty", ock 6599; Ophir, ock 6639/6640 - targeted 3 x 45, single scan, dayside, cloud: Arsia Mons, ock 6635; Olympus Mons, ock 6673 - targeted 3 x 45, single scan, nightside, cloud: Arsia Mons, ock 6692; Olympus Mons, ock 6679 17) 12 days worth of orbits loaded p6671.img notes: 1) optical switch 00 2) day surface = -35 to +15 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm032/mm033 beta supplement - MOC star scans (mz050a) times used for COBE6 looks, loaded as contingency - occurs after next planned upload 5) double scan orbit, surface only: ock 6727 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: Isidis, ock 6716; W. Hematite, ock 6719 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30; first six in this upload - targeted 5 x 13, single scan, dayside: Viking 2, ock 739 - targeted 5 x 13, single scan, nightside: "sandy", ock 6768 - targeted 3 x 45, single scan, dayside, cloud: Elysium Mons, ock 6726 - targeted 3 x 45, single scan, nightside, cloud: Elysium Mons, ock 6732 17) 12 days worth of orbits loaded p6760.img notes: 1) optical switch 00 2) day surface = -35 to +15 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm034/mm035 beta supplement - MOC star scans (mz050a) times used for COBE6 looks, ock 6774/6775 and ock 6798/6799, eqtrx from mz050 seq 5) double scan surface and limb ocks 6806-6840 (3 days) 6) double limbs: all forward looking, 1/2 degree steps from 68 to 63 degrees, 2 looks at each angle, 3 looks at 50 degrees - each limb in 100 sec in duration - "continuous" limb scan 2 times (12 orbits apart) - limb sets 20 degrees lat apart, alternating on orbit pairs 7) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 8) limbs every 10 degrees, alternate orbits (a and b) 9) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 10) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 11) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 12) dense epf- 75S to 75N, 15 degree steps, one every third day 13) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 14) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode 15) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 17) mosaics - 5 x 7, double scan 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 18) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30 - no other targeting due to MOC slews and double days 19) 12 days worth of orbits loaded p6844.img notes: 1) optical switch 00 2) day surface = -35 to +15 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm036/mm037 beta supplement 5) double scan orbit, surface only: ock 6924 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" ock 6855 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: Aram Chaos, ock 6883; W. Hematite, ock 6895 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30 - targeted 5 x 13, single scan, dayside: Viking 1, ock 6909 - targeted 5 x 13, single scan, nightside: Viking 1, ock 6915; "dusty", ock 6926 17) 12 days worth of orbits loaded p6930.img notes: 1) optical switch 00 2) day surface = -30 to +20 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (5S); dayside wedge moved this upload for all non-realtime orbits 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm038/mm039 beta supplement - includes bi-static radar observations ocks 6976-6978; soft_idle during slew icks 245 to 2100 - includes MOLA polar offpoint (mz051a) or ocks 7014-7025; full spatial, full spectral 75 degrees day/night at both poles, soft_idle rest of orbit for buffer management, normal SR pairs, fore and aft limb sets at both poles 5) double scan orbit, surface only: ock 7008 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set added one idle ick between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: W. Hematite, ock 6958 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30 - targeted 5 x 13, single scan, dayside: Korolev, ock 6964; Lobate Cr., ock 6979; Huygens Cr., ock 6981; Gusev Cr., ock 7002; Acidalea Cr., ock 7009 - targeted 5 x 13, single scan, nightside: Gusev Cr., ock 6996 17) 12 days worth of orbits loaded p7014.img notes: 1) optical switch 00 2) day surface = -30 to +20 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (5S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm040/mm041 beta supplement - includes MOLA polar offpoint (mz051a) for ocks 7014-7024 full spatial, full spectral 75 degrees day/night at both poles, soft_idle rest of orbit for buffer management, normal SR pairs, fore and aft limb sets at both poles - includes Radio Science egress observations (mz052b) on ocks 7053-7061, 7074-7076; soft-idle icks 240 to 820, surface and space/ref observations for remainder of orbit 5) double scan orbit, surface only: ock 7092 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set added one idle ick between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30 (no change to night bolo mosaics and no targeted mosaics this upload due to MOLA and RS slew observations) 17) 12 days worth of orbits loaded p7101.img notes: 1) optical switch 00 2) day surface = -30 to +20 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (5S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm042/mm043 beta supplement 5) double scan orbit, surface only: ock 7178 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set added one idle ick between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: Isidis, ock 7131; W. Hematite, ock 7134 and ock 7197 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30; - targeted 5 x 13, single scan, dayside: White rock, ock 7133 - targeted 3 x 45, single scan, dayside, cloud/volc: Olympus Mons, ock 7176 - targeted 3 x 45, single scan, nightside, cloud/volc: Olympus Mons, ock 7182 17) 12 days worth of orbits loaded p7188.img notes: 1) optical switch 00 2) day surface = -30 to +20 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (5S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm044/mm045 beta supplement 5) double scan orbit, surface only: ock 7262 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set added one idle ick between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: Isidis, ock 7219; Aram Chaos, ock 7298 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30; six in this upload, +9 to +24 degree set; skipped -6 to +6 due to schedule constraints - targeted 5 x 13, single scan, dayside: Hesp. paleolake, ock 7218; Viking1, ock 7236; ML2, ock 7286 - targeted 5 x 13, single scan, nightside: Viking1, ock 7242 - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded NOTE: day of year 158 data lost due to DSN coverage being moved from MGS to DS1(emergency) p7285.img notes: 1) optical switch 00 2) day surface = -30 to +20 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (5S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm046/mm047 beta supplement, last normal upload before solar conjunction 5) double scan orbit, surface only: ock 7346 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set added one idle ick between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: Isidis, ock 7370; Aram Chaos, ock 7298 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30; six in this upload, +9 to +24 degree set; skipped -6 to +6 due to schedule constraints - targeted 5 x 13, single scan, dayside: ML2, ock 7286; Huygens, ock 7308; Becquerel, ock 7348; Korolev, ock 7379; Nili, ock 7383 - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p7358.img notes: 1) optical switch 00 2) day surface = -30 to +20 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (5S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm048/mm049 beta supplement, last normal orbits before solar conjunction; also covers part of spacecraft command sequences: mm050/051 solar conjunction 5) double scan orbit: (no double scan orbit until after conjunction) 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set added one idle ick between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: Isidis, ock 7370 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30; six in this upload, +9 to +24 degree set; skipped -6 to +6 due to schedule constraints - targeted 5 x 13, single scan, dayside: Korolev, ock 7379; Nili, ock 7383 - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) ocks 7448 to ~7704 will be solar conjunction - no data collection, but TES powered on and mirror moving - soft idle staring nadir, with triple space looks every 18 minutes, and five space/ref sets per orbit 18) 19.5 days worth of orbits loaded p7422.img notes: 1) optical switch 00 2) day surface = -30 to +20 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -45 south pole, +5 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (5S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers end of spacecraft command sequences: mm049 beta supplement, last normal orbits before solar conjunction; also covers all of spacecraft command sequences: mm050/051 solar conjunction 5) double scan orbit: (no double scan orbit until after conjunction) 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long twice per day on a single orbit: once near south pole and once on nightside - not sure where HGA and Solar Array motions are occurring since start of Beta Supplement - set on 9th orbit (same places as above), one set during HGA motion, one during HGA parked time 13) double alb_ref included in space_alb_ref sets to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set added one idle ick between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30; six in this upload, +9 to +24 degree set; skipped -6 to +6 due to schedule constraints - targeted 5 x 13, single scan, dayside: none - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) ocks 7448 to ~7704 will be solar conjunction - no data collection, but TES powered on and mirror moving - soft idle staring nadir, with triple space looks every 18 minutes, and five space/ref sets per orbit 18) ock 7705 start data output, using regular record surface layout with 5 space/ref sets (sng/dbl scans) - no limbs or epfs will be added until mm052 seq confirmed and record/playbacks underway 19) 28 days worth of orbits loaded p7726.img notes: 1) optical switch 00 2) day surface = -30 to +20 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -30 south pole, +20 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (5S) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers end of spacecraft command sequence: mm053b beta supplement 5) double scan orbit, surface only: ock 7744 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 600, 3125, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -60, cycle in 3 degree steps to +30; six in this upload, +9 to +24 degree set, skipped -6 to +6 due to schedule constraints - targeted 5 x 13, single scan, dayside: none - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p7788.img notes: 1) optical switch 00 2) day surface = -15 to +35 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -15 south pole, +35 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10N) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm054/mm055 normal beta supplement 5) double scan orbit, surface only: ock 7828 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set for once per week repeat cont_limb 70S to 50N - will alternate with cont_limb2 20S to 80N (nightside) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 600, 3125, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, -58.5 to -43.5 degree set - targeted 5 x 13, single scan, dayside: Becuerel Cr, ock 7788; Crommelin2, ock 7851 - targeted 5 x 13, single scan, nightside: Pathfinder, ock 7820; Nili Patera, ock 7829; debris4, ock 7866 - targeted 3 x 45, single scan, dayside, cloud/volc: Kasei Vallis, ock 7853 - targeted 3 x 45, single scan, nightside, cloud/volc: Kasei Vallis, ock 7859 17) 12 days worth of orbits loaded p7874.img notes: CLOUD WEEK UPLOAD (CONCENTRATING ON CLOUDS OCK 7874 to 7956) 1) optical switch 00 2) day surface = -15 to +35 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -15 south pole, +35 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10N) - "fixed" night sequence to shift space triplet that has caused a data gap on icks 15 to 20 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm056/mm057 normal beta supplement 5) double scan orbit: none this upload 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) and cont_limb2 (30S to 90N) pairs twice per orbit except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, cycle thru entire set in one day (ock 7910 - 7920); then any orbit 6th, 7th, 8th, or 9th not used for cloud mosaics or cont_limb(2) pairs; lats for orbits 6,7,8,9 = lats 15S, 0, 15N, 30N 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 600, 3125, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, no double mosaics this upload 16) mosaics - no night bolo this upload all cloud mosaics are 12 hour day/night pairs - targeted 5 x 13, single scan, dayside: none - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: Olympus Mons1, ock 7893; Elysium Mons1, ock 7896; Chryse, ock 7915; Elysium Mons2, ock 7921; Olympus Mons2, ock 7931; Elysium-control, ock 7935; Kasei Vallis, ock 7941 - targeted 3 x 45, single scan, nightside, cloud/volc: Olympus Mons1, ock 7899; Elysium Mons1, ock 7902; Chryse, ock 7921; Elysium Mons2, ock 7927; Olympus Mons2, ock 7937; Elysium-control, ock 7941; Kasei Vallis, ock 7947 17) 12 days worth of orbits loaded ERROR: sequence error inserts single epf look for limb scan #6 (bug in ground command tool - fixed 8/1/00) dense epf on 0N, 15N, 30N, 45N (not 15S as intended) p7959.img notes: BACK TO NOMINAL MAPPING ROUTINES; RADIO SCIENCE SLEWS 1) optical switch 00 2) day surface = -15 to +35 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -15 south pole, +35 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10N) - "fixed" night sequence to shift space triplet that has caused a data gap on icks 15 to 20 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm058/mm059 normal beta supplement - Radio Science spacecraft slews ocks 8029-8040 idle ick 450 - 1050, surface and space/ref observations for remainder of orbit 5) double scan orbit, surface only: ock 7973 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) - cont_limb2 (30S to 90N) pairs twice per orbit except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 600, 3200, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrater bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; - targeted: W. Hematite, ock 7964 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, -40.5 to -25.5 degree set - targeted 5 x 13, single scan, dayside: Viking1, ock 7978; Hematite2, ock 7979; W. Candor, ock 8042 - targeted 5 x 13, single scan, nightside: W. Acidalea, ock 7959; Viking1, ock 7984; S. Isidis, ock 8004 - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded ERROR: W. Hematite double scan mosaic did not get doubles mode space/ref sets - can not calibrate the data p8044.img notes: EPF WEEKLY ALTERNATING CYCLE (-67 degree set) 1) optical switch 00 2) day surface = -15 to +35 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -15 south pole, +35 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10N) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm060/mm061 normal beta supplement 5) double scan orbit, surface only: orbit 8057 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) - cont_limb2 (30S to 90N) pairs twice per orbit except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbit; 10 icks at ick 600, 3200, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; -targeted: Isidis, ock 8049; Aram Chaos, ock 8071/8072 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, -22.5 to -7.5 degree set - targeted 5 x 13, single scan, dayside: Kaiser Cr., ock 8064; Korolev Cr., ock 8121 - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: Elysium Mons, ock 8122 - targeted 3 x 45, single scan, nightside, cloud/volc: Elysium Mons, ock 8128 17) 12 days worth of orbits loaded ERROR: typo in next (p8130.img) radiation window open time results in unintended early radiation; loss of 1 orbit of data (ock 8129): no ref looks, surface only p8130.img notes: EPF WEEKLY ALTERNATING CYCLE (-75 degree set) 1) optical switch 00 2) day surface = -15 to +35 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -15 south pole, +35 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - dayside wedge centered on sub_solar latitude (10N) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm062/mm063 normal beta supplement 5) double scan orbit, surface only: ock 8142 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) - cont_limb2 (30S to 90N) pairs twice per orbit except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbit; 10 icks at ick 600, 3200, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, -4.5 to 10.5 degree set - targeted 5 x 13, single scan, dayside: Pathfinder, ock 8141; Herschel Cr., ock 8148 - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: Olympus Mons, ock 8157 (includes fore and aft limbsets) - targeted 3 x 45, single scan, nightside, cloud/volc: Olympus Mons, ock 8163 (includes fore and aft limbsets) 17) 12 days worth of orbits loaded p8159.img notes: 1) update of p8130.img upload, ONLY CHANGES: load new equalization table, patch, and reference detector (2) for spatial masks - anticipate better onboard compression with new table ERROR: tables not working for spatially or spectrally averaged data p8216.img notes: EPF WEEKLY ALTERNATING CYCLE (-67 degree set) 1) optical switch 00 2) day surface = 0 to +90 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -15 south pole, +35 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude (~15N), increased buffer space from eqz table upload; buffer trial in increasing surface coverage in full spatial/full spectral 3) for realtime orbits: surface = -90 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm064/mm065 normal beta supplement - MOLA polar slews ocks 8301 to 8337 full spatial, full spectral 75 degrees day/night at both poles, soft_idle rest of orbit for buffer management, normal space/ref pairs, fore and aft limb sets at both poles 5) double scan orbit, surface only: ock 8226 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) - cont_limb2 (30S to 90N) pairs twice per orbit except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbit; 10 icks at ick 600, 3200, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, 13.5 to 28.5 degree set - targeted 5 x 13, single scan, dayside: Hebes Chasm, ock 8218; Viking2, ock 8223; Pathfinder, ock 8229; Isidis, ock 8288; Becquerel Cr., ock 8291 - targeted 5 x 13, single scan, nightside: Debris3, ock 8256; Viking2, ock 8267; Debris4, ock 8281 - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p8277.img notes: 1) overwritting of equalization tables: which are not working for spatially or spectrally averaged data - returned normal and realtime surface full spatial/full spectral coverage to pre-equalization table values - precompressor reference detector left at detector 2 2) 10 days worth of orbits loaded ERROR: equalization table overwrite apparently did not work: no problem in upload, instrument accepted full upload - but no change seen in data to indicate change in equalization tables p8312.img notes: NIPCE1- TES INITIATION SEQUENCE (STARTING RESET OF TES) 1) optical switch 00 2) day surface = 0 to +90 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -15 south pole, +35 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude (~15N), increased buffer space from eqz table upload; buffer trial in increasing surface coverage in full spatial/full spectral 3) no overlays (no blackbody refs - just space triplets 4) 4 days worth of orbits loaded: - 2 days with PROM entries, - 2 days with set_orb entries p8313.img notes: NIPCE2- TES INITIATION SEQUENCE (SET_ORB to 8313) EPF WEEKLY ALTERNATING CYCLE (-75 degree set); RADIO SCIENCE SLEWS 1) optical switch 00 2) day surface = -15 to +35 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -15 south pole, +35 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude (~15N) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm066/mm067 normal beta supplement - MOLA polar slews ocks 8301 to 8337 full spatial, full spectral 75 degrees day/night at both poles, soft_idle rest of orbit for buffer management, normal SR pairs, fore and aft limb sets at both poles - Radio Science egress slews ocks 8409-8420 idle icks 800 to 1130, surface and space/ref observations for remainder of orbit 5) double scan orbit, surface only: ock 8313 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) - cont_limb2 (30S to 90N) pairs twice per orbit except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) no dense epf seq or schedules in this load 12) space_ref_long: on 4th and 9th orbit; 10 icks at ick 600, 3200, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, 13.5 to 28.5 degree set - targeted 5 x 13, single scan, dayside: none - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 9 days worth of orbits loaded p8388.img notes: EPF WEEKLY ALTERNATING CYCLE (-75 degree set, no changes); RADIO SCIENCE SLEWS 1) optical switch 00 2) day surface = -15 to +35 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -15 south pole, +35 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude (~15N) 3) for realtime orbits: surface = -60 to +60 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers mm068/mm069 normal beta supplement - Radio Science egress slews 8409-8420 idle icks 800 to 1130, surface and space/ref observations for remainder of orbit 5) double scan orbit, surface only: ock 8390 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) - cont_limb2 (30S to 90N) pairs twice per orbit except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 600, 3200, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, 31.5 and -58.5 to -46.5 degree set - targeted 5 x 13, single scan, dayside: none - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p8473.img notes: EPF WEEKLY ALTERNATING CYCLE (-67 degree set) 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude ~18N, centered wedge on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm070/mm071 normal beta supplement - MOC focus cal #1 eclipse ocks 8535/8536 idle icks 3170 to end and 15 to 450 rest of orbit surface only with refs 5) double scan orbit, surface only: ock 8477 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) - cont_limb2 (30S to 90N) pairs twice per orbit except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 600, 3200, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, -43.5 to -28.5 degree set - targeted 5 x 13, single scan, dayside: Hematite2, ock 8482; Isidis, ock 8552 - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p8558.img notes: EPF WEEKLY ALTERNATING CYCLE (-75 degree set) 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude ~18N, centered wedge on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers mm072/mm073 normal beta supplement - MOC focus cals #2,3,4 eclipse ocks 8584/85; 8608/09; 8633/34 idle icks 3170 to end and 15 to 450 rest of orbit surface only with refs 5) double scan orbit, surface only: ock 8561 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) - cont_limb2 (30S to 90N) pairs twice per orbit except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 600, 3200, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, 22, 19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, -25.5 to -10.5 degree set - targeted 5 x 13, single scan, dayside: Nili, ock 8565; Kaiser, ock 8567; ML2, ock 8619; Korolev, ock 8624; W. Candor, ock 8633; Huygens, ock 8641 - targeted 5 x 13, single scan, nightside: Kasei Valles, ock 8563; Viking1, ock 8575; W. Acidalea, ock 8638 - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p8644.img notes: EPF WEEKLY ALTERNATING CYCLE (-67 degree set) 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude ~18N, centered wedge on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm074/mm075 normal beta supplement - MOC focus cal #5 eclipse ocks 8657/58 idle icks 3170 to end and 15 to 500 rest of orbit surface only with refs 5) double scan orbit, surface only: ock 8646 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) - cont_limb2 (30S to 90N) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day p8729.img notes: EPF WEEKLY ALTERNATING CYCLE (-75 degree set) 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude ~18N, centered wedge on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequence: mm076/mm077 normal beta supplement 5) double scan orbit, surface only: ock 8730 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set cont_limb (70S to 50N) - cont_limb2 (30S to 90N) one per week, alternated between cont_limb and cont_limb2 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbit; 10 icks at ick 600, 3200, and 3400 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, -22, -19, -16, -13, -9; 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, +10.5 to +25.5 degree set - targeted 5 x 13, single scan, dayside: Pathfinder, ock 8732; Herschel Cr., ock 8739; Hematite5, ock 8746; Acidalea Cr., ock 8757; Isidis, ock 8791; ML1, ock 8796 - targeted 5 x 13, single scan, nightside: Hematite4, ock 8803 - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded ERROR: did not account for MOLA polar scans on ocks 8766-8770, 8782-8784,8799-8803,8809-8811; all atmospheric limbscans will be affected by spacecraft slew, epfs will likely be affected as well p8815.img notes: EPF WEEKLY ALTERNATING CYCLE (-67 degree set); RADIO SCIENCE AND Ls 60 CLOUD OBSERVATIONS 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude ~18N, centered wedge on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm078/mm079 normal beta supplement - Radio Science egress slews ocks 8837-8849 (mz061a) - idle ick 540 to 1150; surface and space/ref observations for remainder of orbit 5) double scan orbit, surface only: ock 8817 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set cont_limb (70S to 50N) - cont_limb2 (30S to 90N) pairs twice per day (if space) except for dense epf day 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day full cycle in single day for cloud observations ocks 8858 - 8868 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, -22, -19, -16, -13, -9; none during five days of cloud observations 16) mosaics - night bolo this upload, start at -58.5, cycle in 3 degree steps to +31.5; six in this upload, +28.5 and 31.5 none during five days of cloud observations - targeted 5 x 13, single scan, dayside: none - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: W. Olympus Mons, ocks 8874 8899; W. Elysium Mons, ock 8902; Elysium control, ock 8878 - targeted 3 x 45, single scan, nightside, cloud/volc: W. Olympus Mons, ocks 8880 8905; W. Elysium Mons, ock 8908; Elysium control, ock 8884 17) 12 days worth of orbits loaded p8901.img notes: EPF WEEKLY ALTERNATING CYCLE (-67 degree set) FINISHING Ls 60 CLOUD OBSERVATIONS 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude ~18N, centered wedge on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm080/mm081 normal beta supplement 5) double scan orbit, surface only: ock 8918 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set cont_limb (70S to 50N) - cont_limb2 (30S to 90N) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, -22, -19, -16, -13, -9; none during five days of cloud observations 16) mosaics - no night bolo this upload - targeted 5 x 13, single scan, dayside: Hematite4, ock 8922; Dao Vallis1, ock 8929; Crommelin1, ock 8945; Becuqerel, ock 8970; Nili, ock 8980; Hematite3, ock 8985 - targeted 5 x 13, single scan, nightside: Debris3, ock 8935; Hematite5, ock 8979 - targeted 3 x 45, single scan, dayside, cloud/volc: Elysium control, ock 8878 - targeted 3 x 45, single scan, nightside, cloud/volc: W. Elysium Mons, ock 8908; Elysium control, ock 8884 17) 12 days worth of orbits loaded p8985.img notes: EPF WEEKLY ALTERNATING CYCLE (-75 degree set) 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude wedge centered on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm082/mm083 normal beta supplement 5) double scan orbit, surface only: ock 9002 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set cont_limb (70S to 50N) - cont_limb2 (30S to 90N) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, -22, -19, -16, -13, -9; none during this upload due to ground software bug (fixed) 16) mosaics - no night bolo this upload - targeted 5 x 13, single scan, dayside: Hematite3, ock 8985 - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p9071.img notes: EPF WEEKLY ALTERNATING CYCLE (-67 degree set) 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude wedge centered on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm084/mm085 normal beta supplement 5) double scan orbit, surface only: ock 9086 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) and cont_limb2 (30S to 90N) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -25, -22, -19, -16, -13, -9 16) mosaics - no night bolo this upload - targeted 5 x 13, single scan, dayside: Viking2, ock 9078; Arcadia, ock 9088; Dao Vallis2, ock 9105; Crommelin1, ock 8121; Isidis, ock 9143; Proctor, ock 9145; Becquerel, ock 9146 - targeted 5 x 13, single scan, nightside: Proctor, ock 9101; Debris4, ock 9136 - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p9160.img notes: EPF WEEKLY ALTERNATING CYCLE (-75 degree set) 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude wedge centered on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm086/mm087 normal beta supplement MOLA polar scans (mz062) ocks 9194-9201, 9216-9219, 9224-9227 5) double scan orbit, surface only: ock 9170 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) and cont_limb2 (30S to 90N) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day north polar observation, same parameters, centered on ick 2647 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -9, -6, -3, 0, 3, 6 (new latitudes) 16) mosaics - no night bolo this upload - targeted 5 x 13, single scan, dayside: Arcadia, ock 9176; Crommelin2, ock 9209; Korlev, ock 9215; Isidis, ock 9231; Nili, orb9244 - targeted 5 x 13, single scan, nightside: Nili, ock 9187; W. Acidalea, ock 9229 - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p9255.img notes: EPF WEEKLY ALTERNATING CYCLE (-67 degree set); RADIO SCIENCE SLEWS 1) optical switch 00 2) day surface = -5 to +45 degrees lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask, spatial mask (all detectors averaged together) - short packets except for space/reference sets - sub_solar latitude wedge centered on 20N 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets 4) upload covers spacecraft command sequences: mm088/mm089 normal beta supplement - Radio Science egress scans ocks 9265-9276, 9290-9301 (mz063/64) 5) double scan orbit, surface only: ock 9255 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set; cont_limb (70S to 50N) and cont_limb2 (30S to 90N) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day north polar observation, same parameters, centered on ick 2647 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -9, -6, -3, 0, 3, 6 (new latitudes) 16) mosaics - no night bolo this upload - targeted 5 x 13, single scan, dayside: Nili, ock 9244; Arcadia, ock 9264; Dao Vallis2, ock 9281; Cromellin1, ock 9297; Korolev, ock 9303; Isidis, ock 9319 - targeted 5 x 13, single scan, nightside: S. Isidis, ock 9274; Hematite2, ock 9306; Cromellin2, ock 9328 - targeted 3 x 45, single scan, dayside, cloud/volc: Elysium Mons, ock 9304/0305 - targeted 3 x 45, single scan, nightside, cloud/volc: Elysium Mons, ock 9310 17) 12 days worth of orbits loaded ERROR: station/spacecraft error during uplink window results in upload not getting on board NOTE: p9255.img actually a rebuild of p9243.img with appropriate modifications p9329.img notes: EPF WEEKLY ALTERNATING CYCLE (-75 degree set) 1) optical switch 00 2) Low Record Rate (LRC): day surface = -5 to +45 deg lat, full spectral, full spatial night = +25 to -25 degrees lat, spectral mask, full spatial poles = -25 to -5 south pole, +45 to +25 north pole, spectral mask, spatial mask - short packets except for space/reference sets - sub_solar latitude wedge centered on 20N Medium Record Rate (MRC) starting on ock 9369: day surface = +20 to +90 deg lat, full spectral, full spatial night = +45 to -45 deg lat, spectral mask, full spatial poles = -45 to +20 south pole, +90 to +45 north pole, spectral mask, spatial mask 3) for realtime orbits: surface = -30 to +90 degrees lat, full spatial, full spectral - long packets night = +30 to -30 degrees lat, spectral mask, full spatial - short packets poles = rest of lats, spectral mask, spatial mask - short packets Changes for MRC: full spatial, full spectral for entire orbit, long packets on ascent, short packets on descent 4) upload covers spacecraft command sequences: mm090/mm091 normal beta supplement 5) double scan orbit, surface only: ock 9339 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set cont_limb (70S to 50N) - cont_limb2 (30S to 90N) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day north polar observation, same parameters, centered on ick 2647 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -9, -6, -3, 0, 3, 6 16) mosaics - no night bolo this upload - targeted 5 x 13, single scan, dayside: Nili, ock 9332; Russell, ock 9372; Holden, ock 9386; Korolev, orb9391; Lyot, ock 9396; Hesp. Paleolake, ock 9406; Proctor, orb9409 - targeted 5 x 13, single scan, nightside: Korolev, ock 9335; Nili, ock 9363; Hematite3, ock 9394 - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p9415.img notes: EPF WEEKLY ALTERNATING CYCLE (-67 degree set) 1) optical switch 00 2) day surface = +20 to +90 deg lat, full spectral, full spatial night = +45 to -45 deg lat, spectral mask, full spatial poles = -45 to +20 south pole, +90 to +45 north pole, spectral mask, spatial mask - short packets except for space/reference sets - sub_solar latitude wedge centered on 20N 3) for realtime orbits: full spatial, full spectral for entire orbit; long packets on ascent, short packets on descent 4) upload covers spacecraft command sequences: mm092/mm093 normal beta supplement 5) double scan orbit, surface only: ock 9423 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate orbits (a and b) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set cont_limb (70S to 50N) and cont_limb2 (30S to 90N) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -67 lat to +82 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf- 75S to 75N, 15 degree steps, one every third day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) double alb_ref included in space_alb_ref sets - to calibrate bolometer data collected in double scan mode - testing alb lamp 2, on "cont_limb" every second week 5 icks alb_ref2 prior to regular alb_ref1 sng/dbl set 10 idle icks between alb_ref2 and alb_ref1 sets 14) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day north polar observation, same parameters, centered on ick 2647 15) mosaics - 5 x 7, double scan, 1 per day cycling through latitudes -9, -6, -3, 0, 3, 6 16) mosaics - no night bolo this upload - targeted 5 x 13, single scan, dayside: Baldet, ock 9420; Rabe, ock 9434; Arcadai, ock 9440; Pettit, ock 9441; Dao Vallis2, ock 9457; Russell, ock 9560; Crommellin2, ock 9473; Rutherford, ock 9473; Holden, ock 9474; Lyot, ock 9484 - targeted 5 x 13, single scan, nightside: Crommellin2, ock 9416 - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 17) 12 days worth of orbits loaded p9501.img notes: START FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE RADIO SCIENCE/CAMPAIGN F 1) optical switch 00 2) day surface = -60 to +60(desc) deg lat, full spectral, spatial mask night = +60 to -60 deg lat, spectral mask, spatial mask poles = -60 to -60 south pole, spectral mask, spatial mask - short packets except for space/reference sets 3) for realtime orbits: spatial mask, full spectral for entire orbit; long packets on ascent, short packets on descent 4) upload covers spacecraft command sequences: mm094/mm095 normal beta supplement 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternate cycles (3rd orbit) 7) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +70 (descending) - for coincident coverage with the Radio Science experiment during 0 earth beta angle time (Campaign F/ December); - full spatial 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, spatial mask used 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf on cont_limb orbits (1st and 2nd orbits) 10) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) south polar observation, 15 icks full spatial, full spectral centered on ick 882 12) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 13) 12 days worth of orbits loaded WARNING: many blackbody reference looks lost due to instrument warmstart events (~1/3 of time); not enough time in double scan mode for mirror motion, will add idle ick in next build p9573.img notes: RADIO SCIENCE SLEWS and CAMPAIGN F 1) optical switch 00 2) for all orbits: spatial mask, full spectral for entire orbit, long packets on ascent, short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm096/mm097 normal beta supplement - mz065 and mz066: radio science egress slews 4) Radio Science egress slew, special observations for Campaign F: - ocks 9644-9655, 9657, 9669-9674 - starting at ick 810, look forward 47 degrees and then step in 1 degree steps to 0 pnt over 16 minute duration - attempting to keep "nadir" view of surface during spacecraft motion - three orbit cycle: 1st orbit) cont_limb_dbl 2nd orbit) cont_limb_sng 3rd orbit) regular limbs - no epfs on egress slew orbits 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternate cycles (3rd orbit) 7) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +70 (descending) - for coincident coverage with the Radio Science experiment during 0 earth beta angle time (Campaign F/ December); - full spatial 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, spatial mask used 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf on cont_limb orbits (1st and 2nd orbits) 10) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) south polar observation, 15 icks full spatial, full spectral centered on ick 882 12) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 13) 12 days worth of orbits loaded NOTE: tried adding double scan idle ick to solve warmstart problem WARNING: most blackbody reference looks lost due to instrument warmstarts; idle ick did not work, will try single scan idle ick at different angle in next upload p9622.img notes: RADIO SCIENCE SLEWS and CAMPAIGN F 1) optical switch 00 2) for all orbits: spatial mask, full spectral for entire orbit, long packets on ascent, short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm096/mm097 normal beta supplement - mz065, mz066, and mz067: radio science egress slews 4) Radio Science egress slew, special obs for Campaign F: - ocks 9644-9655, 9657, 9669-9680 - starting at ick 810, continual aft limb scans, 16 limb scans in all: 6 looks, 2 obs length duration, one degree steps, then 3 obs at 50 degree emission angle equivalent 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternate cycles (3rd orbit) 7) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +70 (descending) - for coincident coverage with the Radio Science experiment during 0 earth beta angle time (Campaign F/ December); - full spatial 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, spatial mask used 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf on cont_limb orbits (1st and 2nd orbits) 10) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) south polar observation, 15 icks full spatial, full spectral centered on ick 882 12) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 13) 12 days worth of orbits loaded NOTE: tried adding single scan idle ick at pnt_angle 180 to solve warmstart problem WARNING: all double scan blackbody looks lost due to unknown sequencing problem; will return to single scan operations while problem is investigated; data cannot be calibrated due to missing blackbody looks p9671.img notes: RETURN TO FULL TIME 10cm-1 (SINGLE SCAN) MODE; RADIO SCIENCE SLEWS and CAMPAIGN F; EPF WEEKLY ALTERNATING CYCLE (-75 degree set) 1) optical switch 00 2) day surface = -40 to +90 deg lat, full spectral, full spatial - long packets night = +90 to -60 deg lat, spectral mask, full spatial - short packets poles = -60 to -40 south pole, spectral mask, spatial mask - short packets 3) for realtime orbits: (same as above) 4) upload covers spacecraft command sequences: mm098/mm099 normal beta supplement - mz067: radio science egress slews 5) Radio Science egress slew, special obs for campaign F: - ocks 9671-9680 - starting at ick 810, continual aft limb scans, 16 limb scans in all: 6 looks, 2 obs length duration, one degree steps, then 3 obs at 50 degree emission angle equivalent 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate cycles (3rd orbit) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating scan mode (single then double) of cont_limb each orbit - centered on radio science ingress occultation (lats +85 to +55 descending) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf: 75S to 75N, 15 degree steps, one every day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 14) mosaics - 5 x 7, double scan, none 15) mosaics - no night bolo this upload - targeted 5 x 13, single scan, dayside: none - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 16) 12 days worth of orbits loaded p9757.img notes: EPF WEEKLY ALTERNATING CYCLE (-75 degree set); RADIO SCIENCE/ CAMPAIGN F; TESTING 5cm-1 SPACE/REF SETS 1) optical switch 00 2) surface = -40 to +90 deg lat, full spectral, full spatial - long packets night = +90 to -60 deg lat, spectral mask, full spatial - short packets poles = -60 to -40 south pole, spectral mask, spatial mask - short packets 3) for realtime orbits: (same as above) 4) upload covers spacecraft command sequences: mm100/mm101 normal beta supplement 5) space/ref tests using single scan idles in two different locations and at two different angles; testing on three different orbits utilizing different icks per test - background sequence is double scan nadir 6) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets 7) limbs every 10 degrees, alternate cycles (3rd orbit) 8) continuous limb look - with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating scan mode (single then double) of cont_limb each orbit - centered on Radio Science ingress occultation (lats +85 to +55 descending) 9) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 5 icks at each angle 10) 1 N-polar, 1 S-polar, and 1 nightside epf (alb_ref orbit) per day; 1 dayside epf per orbit - steps from -75 lat to +75 lat in 15 deg lat steps to cycle through dayside completely in a single day 11) dense epf: 75S to 75N, 15 degree steps, one every day 12) space_ref_long: on 4th and 9th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 13) south polar observation, 30 icks full spatial, full spectral centered on ick 882, 11 orbits per day 14) mosaics - 5 x 7, double scan, none 15) mosaics - no night bolo this upload - targeted 5 x 13, single scan, dayside: none - targeted 5 x 13, single scan, nightside: none - targeted 3 x 45, single scan, dayside, cloud/volc: none - targeted 3 x 45, single scan, nightside, cloud/volc: none 16) 12 days worth of orbits loaded p9843.img notes: START FULL TIME 5cm-1 (DOUBLE SCAN) MODE; IMPLEMENTING 18 ORBIT OBSERVATION CYCLE; RADIO SCIENCE/CAMPAIGN F 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm102/mm103 normal beta supplement 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 5) limbs every 20 degrees, alternating on 3rd orbit 6) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +70 (descending) - for coincident coverage with the Radio Science experiment during 0 earth beta angle time (Campaign F/ December); full spatial 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, spatial mask used 8) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 9) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 780, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 10) south polar observation, 15 icks full spatial, full spectral centered on ick 882 11) mosaics - - targeted 5 x 7, double scan, dayside: Proctor, ock 9849; Becuqerel, ock 9850; Baldet, ock 9860; Korolev, ock 9863; Arcadia, ock 9880; Pettit, ock 9881; Fournir, ock 9885; Dao Vallis2, ock 9897; Russell, ock 9900; Crommelin2, ock 9913; Lyot, ock 9924 - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 13) 12 days worth of orbits loaded p9930.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE RADIO SCIENCE SLEWS and CAMPAIGN F 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm104/mm105 normal beta supplement, and mz068/mz069 - Radio Science egress slews (mz068 and mz069) not doing anything with TES (no soft idle) 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 5) limbs every 20 degrees, alternating on 3rd orbit 6) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +70 (descending) - for coincident coverage with the Radio Science experiment during 0 earth beta angle time (Campaign F/ December); full spatial 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 9) dense epf: one dense epf every third day (36 orbits), only on continuous limb orbits 10) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 11) albedo lamp 2 test - will test twice per month, this time only includes both single and double scan modes 12) south polar observation, 15 icks full spatial, full spectral centered on ick 882 13) mosaics - - targeted 5 x 7, double scan, dayside: Baldet Cr, ock 9948; Hematite-3, ock 9953; Pettit Cr, ock 9969; Fournir Cr, ock 9973; Crommelin1, ock 10001; Lyot Cr, ock 10012 - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 14) 12 days worth of orbits loaded p10027.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm106/mm107 normal beta supplement, and mz070 for MOLA polar scans - stare at nadir for full orbit; fore and aft limb sets at highest latitude 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 5) limbs every 20 degrees, alternating on 3rd orbit 6) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +70 (descending); full spatial 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 9) dense epf: one dense epf every third day (36 orbits), only on continuous limb orbits 10) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3385 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 11) albedo lamp 2 test - will test twice per month, this time only includes both single and double scan modes 12) south polar observation, 15 icks full spatial, full spectral centered on ick 882 13) mosaics - - targeted 5 x 7, double scan, dayside: Baldet Cr, ock 10036; Hematite-3, ock 10041; Fournir Cr, ock 10061; Crommelin1, ock 10089 - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 14) 12 days worth of orbits loaded NOTE1: DSN transmission errors necessitated rebuild of this as p10027.img {was p10015.img}; missed first three MOLA observation orbits NOTE2: Reaction wheel anomaly on DOY 2001-018 caused cancellation of MOLA scans p10100.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm108/mm109 normal beta supplement; - x-reaction wheel test on ock 10100 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 5) limbs every 20 degrees, alternating on 3rd orbit 6) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +70 (descending); full spatial 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 9) dense epf: one dense epf every third day (36 orbits), only on continuous limb orbits 10) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3385 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 11) albedo lamp 2 test - will test twice per month, this time only includes both single and double scan modes 12) south polar observation, 15 icks full spatial, full spectral centered on ick 882 13) mosaics - - targeted 5 x 7, double scan, dayside: lobate Cr, ock 10135; Pasteur Cr, ock 10138; Arcadia2, ock 10144; Galilaei Cr, ock 10165; Mutch Cr, ock 10166 - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 14) 12 days worth of orbits loaded p10161.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm109/mm110/mm111 normal beta supplement 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 5) limbs every 20 degrees, alternating on 3rd orbit 6) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +70 (descending); full spatial 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 9) dense epf: one dense epf every third day (36 orbits), only on continuous limb orbits 10) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3385 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 11) albedo lamp 2 test - will test twice per month, this time only includes both single and double scan modes 12) south polar observation, 15 icks full spatial, full spectral centered on ick 882 13) mosaics - - targeted 5 x 7, double scan, dayside: Galilaei Cr, ock 10165; Mutch Cr, ock 10166 - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 14) 12 days worth of orbits loaded p10271.img notes: CLOUD WEEK OBSERVATIONS FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm112/mm113 normal beta supplement 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 5) limbs every 20 degrees, alternating on 3rd orbit 6) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +55 (descending); full spatial 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 9) dense epf: on every available orbit not used for cloud mosaics (all except 3rd, 6th, 9th, 12th, 15th, 17th, and 18th orbits) - targeted dense epf on W. Hematite, ock 10290 and at Aram Chaos, ock 10303 10) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 11) albedo lamp 2 test - will test twice per month, includes both single and double scan modes 12) south polar observation, 15 icks full spatial, full spectral centered on ick 882 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: Elysium control1, ock 10286; Kasei, ock 10292; W. Olympus Mons, ock 10307; Chryse control1, ock 10329; W. Elysium Mons1, ock 10335; Elysium control2, ock 10349; Chryse control2, ock 10354;W. Elysium Mons2, ock 10360 - targeted 3 x 23, double scan, nightside, cloud/volc: Elysium control1, ock 10292; Kasei, ock 10298; W. Olympus Mons, ock 10313; Chryse control1, ock 10335; W. Elysium Mons1, ock 10341; Elysium control2, ock 10355; Chyrse control2, ock 10360; W. Elysium Mons2, ock 10366 14) Ascending cloud mosaics bracketed fore at aft with limbsets at the target latitude; descending could mosaics have fore limbset at target latitude 15) 12 days worth of orbits loaded p10357.img notes: CLOUD WEEK OBSERVATIONS ROTO DEMONSTRATION FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] - moved space triplet off ick 15 to avoid gore building up 3) upload covers spacecraft command sequences: mm114/mm115 normal beta supplement, and mz072a ROTO (Roll maneuver) demonstration 4) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 5) limbs every 20 degrees, alternating on 3rd orbit 6) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +55 (descending); full spatial 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 9) dense epf: on every available orbit not used for cloud mosaics (all except 3rd, 6th, 9th, 12th, 15th, 17th, and 18th orbits) 10) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 11) albedo lamp 2 test - will test twice per month, includes both single and double scan modes 12) south polar observation, 15 icks full spatial, full spectral centered on ick 882 13) mosaics - - targeted 5 x 7, double scan, dayside: Moreux Cr, ock 10376; Korolev Cr, ock 10384; W. Candor, ock 10393 - targeted 5 x 7, double scan, nightside: W. Acidalea, ock 10398; Richardson Cr, ock 10428 - targeted 3 x 23, double scan, dayside, cloud/volc: W. Elysium Mons2, ock 10360 - targeted 3 x 23, double scan, nightside, cloud/volc: W. Elysium Mons2, ock 10366 14) Ascending cloud mosaics bracketed fore at aft with limbsets at the target latitude; descending cloud mosaics have fore limbset at target latitude 15) 12 days worth of orbits loaded p10443.img notes: INTERFEROGRAM ORBIT START NOMINAL ROTO OPERATIONS FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm116/mm117 normal beta supplement - ROTO orbits and times prelims provided by E. Jensen 4) ROTO orbits and slew start icks - ock 10359 slew starts at ick 970 - ock 10469 slew starts at ick 1315 - ock 10370 slew starts at ick 1654 - ock 10481 slew starts at ick 1319 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +55 (descending); full spatial 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 10) dense epf: one every third day (36 orbits), cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 12) albedo lamp 2 test - will test twice per month, includes both single and double scan modes 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: Lomonosov Cr, ock 10453; Rutherford Cr, ock 10466; Holden Cr, ock 10467; W. Hematite, ock 10491; Baldet Cr, ock 10501; Pettit Cr, ock 10522 - targeted 5 x 7, double scan, nightside: S. Isidis, ock 10506 - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) Interferograms for "glitch 1" noise study, detector 2, single scan mode - ock 10443, start ick 1216, end ick 2647, rest of orbit idle for buffer control 16) 12 days worth of orbits loaded p10480.img notes: 1) Mid-cycle ROTO update to p10443.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 10507 slew starts at ick 996 - ock 10530 slew starts at ick 1150 p10528.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm118/mm119 normal beta supplement - ROTO orbits and times provided by E. Jensen 4) ROTO orbits and slew start icks - ock 10530 slew starts at ick 1150 - ock 10541 slew starts at ick 881 - ock 10542 slew starts at ick 1615 - ock 10544 slew starts at ick 1334 - ock 10545 slew starts at ick 1418 - ock 10546 slew starts at ick 1299 - ock 10566 slew starts at ick 883 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +55 (descending); full spatial 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 10) dense epf: one every third day (36 orbits), cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 12) albedo lamp 2 test - will test twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: Crommelin1, ock 10554; Becquerel Cr, ock 10579; Arcadia2, ock 10609 - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days worth of orbits loaded p10564.img notes: 1) Mid-cycle ROTO update to p10528.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 10593 slew starts at ick 1464 - ock 10594 slew starts at ick 1349 - ock 10595 slew starts at ick 1394 - ock 10604 slew starts at ick 948 p10613.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm120/mm121 normal beta supplement, and mz077 ROTO orbits and times 4) ROTO orbits and slew start icks - ock 10625 slew starts at ick 1773 - ock 10627 slew starts at ick 1792 - ock 10628 slew starts at ick 984 - ock 10640 slew starts at ick 1852 - ock 10641 slew starts at ick 965 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +55 (descending); full spatial 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 10) dense epf: one every third day (36 orbits), cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 12) albedo lamp 2 test - will test twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: Fournir Cr, ock 10614; Lomonosov Cr, ock 10629; Mutch Cr, ock 10631; Trouvelot Cr, ock 10642 - targeted 5 x 7, double scan, nightside: Kasei Vallis, ock 10675 - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days worth of orbits loaded p10649.img notes: 1) Mid-cycle ROTO update to p10613.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 10654 slew starts at ick 889 - ock 10655 slew starts at ick 1447 - ock 10664 slew starts at ick 1629 - ock 10687 slew starts at ick 1368 - ock 10690 slew starts at ick 1202 p10699.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm122/mm123 normal beta supplement, and mz079 ROTO orbits and times 4) ROTO orbits and slew start icks - ock 10712 slew starts at ick 1895 - ock 10714 slew starts at ick 1465 - ock 10726 slew starts at ick 1874 - ock 10736 slew starts at ick 1276 - ock 10737 slew starts at ick 1760 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb look - 2 icks at each angle, 1/2 degree steps, with 3 looks at ~60 degree emission angle (50 degrees pnt_angle) between each set, alternating double scan mode (1st orbit) and single scan mode (2nd orbit); 30 degrees of latitude coverage centered on +55 (descending); full spatial 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 10) dense epf: one every third day (36 orbits), cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 12) albedo lamp 2 test - will test twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - TARGETING TOOL BROKEN - NO MOSAICS THIS BUILD - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days worth of orbits loaded p10734.img notes: 1) Mid-cycle ROTO update to p10699.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 10750 slew starts at ick 1361 - ock 10751 slew starts at ick 976 - ock 10762 slew starts at ick 1668 - ock 10763 slew starts at ick 1819 - ock 10776 slew starts at ick 2114 p10785.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm124/mm125 normal beta supplement, and mz081c pitch22 config test - no ROTOs 4) pitch 22 test - spacecraft pitch 22 in +x direction, stare at 0 pnt_angle with space/ref sets for ocks 10808 - 10813 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb looks - all removed 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (cont_limb orbits) 10) dense epf: one every third day (36 orbits), cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 12) albedo lamp 2 test - will test twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: Lomonosov Cr, ock 10830; Cromellin1, ock 10843; W. Hematite, ock 10868 - targeted 5 x 7, double scan, nightside: Cromellin1, ock 10786; West Olympus Mons, ock 10816; SE Arsia Mons, ock 10841; Phlegra Montes, ock 10843; Viking2, ock 10844; Arda Valles, ock 10863; Coprates Chasma, ock 10864 - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days worth of orbits loaded p10822.img notes: 1) Mid-cycle ROTO update to p10785.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 10826 slew starts at ick 1695 - ock 10827 slew starts at ick 1463 - ock 10861 slew starts at ick 1010 - ock 10864 slew starts at ick 1807 p10869.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE; RADIO SCIENCE SLEWS; LONG UPLOAD - DOY 087 to 104 (ODYSSEY LAUNCH COVERAGE) 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets on ascent; short packets on descent [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm126/mm127 normal beta supplement, and mz083 ROTO orbits and times - also includes mm128/129/130, more ROTO mz minisequences and Radio Science minisequences which are not available yet 4) all possible roto orbits have been supplied by Elsa of MOC and TES will stare nadir with space/ref sets for those orbits; nothing different will be done for the Radio Science egress slews - so nightside south polar data will be affected by the slew maneuver 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternate orbits (3a and 3b) 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per orbits 1 and 2 (epf-only orbits) 10) dense epf: one every third day (36 orbits), cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 12) albedo lamp 2 test - will test twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 20 days worth of orbits loaded, will use 18 days p11076.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm131 normal beta supplement, and mz089 ROTO orbits and times 4) ROTO orbits and slew start icks - ock 11090 slew starts at 1387 - ock 11093 slew starts at 1012 - ock 11103 slew starts at 1018 - ock 11127 slew starts at 1689 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternate on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed periods [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 6 days worth of orbits loaded ERROR: incorrect previous image used in shell, TES discarded upload; TES lost all overlay schedules and collected only surface and space looks (no reference looks) until p11113 upload; cannot calibrate spectral data without reference looks. p11113.img notes: CLOUD WEEK OBSERVATIONS (ock 11113 to 11199) FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit [buffer has been underutilized in double scan mode] 3) upload covers spacecraft command sequences: mm132/mm133 normal beta supplement - ROTO orbits and times provided by E. Jensen 4) ROTO orbits and slew start icks - ock 11127 slew starts at ick 1689 - ock 11143 slew starts at ick 2070 - ock 11144 slew starts at ick 2550 - ock 11145 slew starts at ick 1770 - ock 11154 slew starts at ick 1200 - ock 11163 slew starts at ick 1380 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: on every available orbit, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - cloud mosaics include bounding fore and aft limbsets - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: W. Elysium Mons, ock 11114; Chryse control, ock 11133; W. Elysium Mons, ock 11139; W. Olympus Mons, ock 11149; Elysium control, ock 11153; Kasei Vallis, ock 11159; W. Olympus Mons, ock 11174; Elysium control, ock 11178; - targeted 3 x 23, double scan, nightside, cloud/volc: W. Elysium Mons, ock 11120; Chyrse control, ock 11139; W. Olympus Mons, ock 11155; Elysium control, ock 11159; Kasei Vallis, ock 11165; W. Olympus Mons, ock 11180; Elysium control, ock 11184 15) 12 days loaded p11131.img notes: 1) Mid-cycle ROTO update to p11113.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 11177 slew starts at ick 1362 - ock 11178 slew starts at ick 2186 - ock 11179 slew starts at ick 1460 - ock 11181 slew starts at ick 1338 - ock 11192 slew starts at ick 1503 p11213.img notes: MOC FOCUS TEST and TES COBE TEST FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers command sequences: mm134/mm135 normal beta supplement, and mz092a ROTO orbits and times 4) ROTO orbits and slew start icks - ock 11217 slew starts at ick 848 - ock 11226 slew starts at ick 1274 - ock 11227 slew starts at ick 670 - ock 11236 slew starts at ick 1654 - ock 11237 slew starts at ick 1709 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) COBE - background instrument response test at different angles testing angles that will be used in new fuel-saving spacecraft attitude - done twice during each MOC star slew [Mars out of the field of view]; 10 icks each (double-scan) at pnt_angles -16,-17,-19,-22,-79,-84 15) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 16) 12 days loaded p11247.img notes: 1) Mid-cycle ROTO update to p11213.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 11253 slew starts at ick 2115 - ock 11276 slew starts at ick 2141 - ock 11287 slew starts at ick 1362 - ock 11288 slew starts at ick 1004 p11495.img notes: NIPCE1- TES INITIATION SEQUENCE 1) optical switch 00 2) ALGOR patch loaded 3) stare nadir in double scan mode with space/reference looks 4) 10 orbits loaded p11496.img notes: NIPCE2- TES INITIATION SEQUENCE FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: mm140/mm141 normal beta supplement - ROTO orbits and times provided by E. Jensen 4) ROTO orbits; stare nadir entire orbit - ock 11510 - ock 11511 - ock 11529-11536 - ock 11554-11556 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days loaded p11553.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: mm142/mm143 normal beta supplement, and mz102a ROTO orbits and times 4) ROTO orbits and slew start icks - ock 11554 slew starts at 667 - ock 11569 slew starts at 1503 - ock 11571 slew starts at 954 - ock 11572 slew starts at 720 - ock 11592 slew starts at 758 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: Moreux Cr., ock 11557; JJ7, ock 11563; JJ4, ock 11581; Fournir Cr., ock 11594; Vicky1, ock 11607; Lomonosov, ock 11609 - targeted 5 x 7, double scan, nightside: Arda Vallis, ock 11554; Coprates Chasm, ocks 11555 and 11580; NW Tyrrhena, ock 11612 - targeted 3 x 23, double scan, dayside, cloud/volc: Arsia Mons, ock 11563; Elysium Mons, ock 11566; Olympus Mons, ock 11601 - targeted 3 x 23, double scan, nightside, cloud/volc: Elysium Mons, ock 11572 15) 12 days loaded p11591.img notes: 1) Mid-cycle ROTO update to p11553.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 11593 slew starts at ick 882 - ock 11597 slew starts at ick 1296 - ock 11606 slew starts at ick 1327 - ock 11609 slew starts at ick 1435 - ock 11610 slew starts at ick 1604 - ock 11642 slew starts at ick 1352 p11641.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: mm144/mm145 normal beta supplement, - ROTO orbits and times provided by E. Jensen 4) ROTO orbits and slew start icks - ock 11642 slew starts at ick 1352 - ock 11659 - ock 11677 - ock 11679 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days loaded p11676.img notes: 1) Mid-cycle ROTO update to p11641.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 11677 slew starts at ick 1355 - ock 11679 slew starts at ick 1503 - ock 11682 slew starts at ick 1491 - ock 11692 slew starts at ick 1455 - ock 11714 slew starts at ick 1594 - ock 11715 slew starts at ick 837 - ock 11716 slew starts at ick 1269 - ock 11717 slew starts at ick 665 p11727.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: mm146/mm147 normal beta supplement, and mz106 ROTO orbits and times 4) ROTO orbits and slew start icks - ock 11740 slew starts at 1295 - ock 11743 slew starts at 1470 - ock 11755 slew starts at 1892 - ock 11756 slew starts at 1408 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days loaded p11763.img notes: 1) Mid-cycle ROTO update to p11727.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 11790 slew starts at ick 1692 - ock 11791 slew starts at ick 1619 - ock 11792 slew starts at ick 1482 - ock 11800 slew starts at ick 162 - ock 11805 slew starts at ick 1896 - ock 11814 slew starts at ick 605 p11811.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: mm148/mm149 normal beta supplement, and mz108 ROTO orbits and times - NOTE: LAST BETA SUPPLEMENT UPLOAD 4) ROTO orbits and slew start icks - ock 11814 slew starts at 605 - ock 11827 slew starts at 1760 - ock 11829 slew starts at 1278 - ock 11837 slew starts at 1350 - ock 11849 slew starts at 1161 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: Korolev Cr, ock 11854 - targeted 5 x 13, single scan, dayside: JJ1, ock 11842 - targeted 5 x 7, double scan, nightside: Gale Cr Landing site, ocks 11811/11812; W. Hematite landing site #3, ocks 11816/11817 - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days loaded p11846.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: mm149 normal beta supplement, and mz109 ROTO orbits and times - NOTE: LAST BETA SUPPLEMENT UPLOAD 4) ROTO orbits and slew start icks - ock 11849 slew starts at 1161 - ock 11862 slew starts at 1472 - ock 11863 slew starts at 1336 - ock 11864 slew starts at 1431 - ock 11865 slew starts at 1579 - ock 11897 slew starts at 1322 - ock 11898 slew starts at 1398 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: Korolev Cr, ock 11854 - targeted 5 x 13, single scan, dayside: none - targeted 5 x 7, double scan, nightside: SE Arsia, ock 11846; Gusev landing site, ock 11886; Deuteronilus A p11891; NW Tyrrhena p11901; Nilosyrtus, ock 11914 - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days loaded p11896.img notes: 1) Mid-cycle ROTO update to p11846.img - upload covers spacecraft command sequences: mm150, first nominal mapping sequence ONLY CHANGES: added ROTO orbits and slew start icks - ock 11897 slew starts at ick 1322 - ock 11898 slew starts at ick 1398 - ock 11902 slew starts at ick 1586 - ock 11910 slew starts at ick 963 - ock 11915 slew starts at ick 1726 - ock 11923 slew starts at ick 1431 p11933.img notes: 1) Mid-cycle ROTO update to p11896.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 11939 slew starts at ick 1660 - ock 11948 slew starts at ick 888 - ock 11949 slew starts at ick 900 - ock 11950 slew starts at ick 1464 2) 12 days uploaded NOTE: mz112 - UHF test on 2001-177,178,179; - days 177 and 179 in nadir orientation - day 178 in 16 degree relay roll position - no changes in TES observation plans; obs on 2001-178 will be oblique p11983.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: partial mm150 normal mapping, and mz113b ROTO orbits and times 4) ROTO orbits and slew start icks - ock 11994 slew starts at 1200 - ock 11995 slew starts at 1196 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40S latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf in 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 80, 830, and 3380 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 13, single scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 15) 12 days loaded 16) memory dump on ALGOR and IMC flight software patch locations immediate action commands when upload reaches TES p12068.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 18 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: partial mm150 normal mapping; NO ROTOs DUE TO DUST STORM 4) ROTO orbits and slew start icks: NONE 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 3rd orbit 7) continuous limb scan in double mode placed in southern hemisphere to cover 90-40 south latitude ascending (9 complete limb scans total) - limbs collected on every third orbit set (orbits 37-54) 8) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 18 orbits in full cycle; 2 dayside epf per 1st and 2nd orbits (epf-only orbits) 10) dense epf: one every third day, cycles from -75 to +75 lat 11) space_ref_long: on 5th and 14th orbits; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) albedo lamp 2 test - will be twice per month, includes only double scan mode 13) south polar observation, 15 icks full spatial, full spectral centered on ick 882 14) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 13, single scan, dayside: none - targeted 5 x 7, double scan, nightside: none - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: 15) 12 days loaded ERROR: upload not accepted - edit table close error TES only collecting nadir and space looks due to error state; will not be able to calibrate data in ocks 12068-12103 due to lack of blackbody reference looks p12020.img notes: 1) Mid-cycle ROTO update to p11983.img ONLY CHANGES: added ROTO orbits and slew start icks - ock 12024 slew starts at ick 1460 - ock 12025 slew starts at ick 1283 - ock 12033 slew starts at ick 1457 - ock 12035 slew starts at ick 1538 - ock 12042 slew starts at ick 1018 - ock 12044 slew starts at ick 1351 - ock 12047 slew starts at ick 1729 - ock 12071 slew starts at ick 1448 2) Upload attempt during ock 12068 ERROR: upload not accepted - edit table close error TES only collecting nadir and space looks due to error state will not be able to calibrate 2 directories of data due to lack of blackbody reference looks p12104.img notes: DUST STORM MONITORING 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: partial mm150 normal mapping 4) ROTO orbits and slew start icks: NO ROTOs DUE TO DUST STORM 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: NONE UNTIL END OF STORM 10) space_ref_long: on 12th orbit, 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - will be twice per month, includes only double scan mode 12) mosaics - NONE UNTIL END OF STORM 13) 12 days loaded p12154.img notes: DUST STORM MONITORING 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm150 normal mapping 4) ROTO orbits and slew start icks: NO ROTOs DUE TO DUST STORM 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating on 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: NONE UNTIL END OF STORM 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - will be twice per month, includes only double scan mode 12) mosaics - NONE UNTIL END OF STORM 13) 12 days loaded 14) additional space/blackbody reference sets added to limb orbits p12238.img notes: DUST STORM MONITORING 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm151 normal mapping 4) ROTO orbits and slew start icks: NO ROTOs DUE TO DUST STORM 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: NONE UNTIL END OF STORM 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - will be twice per month, includes only double scan mode 12) mosaics - NONE UNTIL END OF STORM 13) 24 days loaded p12361.img notes: DUST STORM MONITORING 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm151 normal mapping 4) ROTO orbits and slew start icks - ock 12365 slew starts at 603 - ock 12366 slew starts at 624 - ock 12411 slew starts at 495 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: NONE UNTIL END OF STORM 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - will be twice per month, includes only double scan mode 12) mosaics - NONE UNTIL END OF STORM 13) 12 days loaded p12410.img notes: DUST STORM MONITORING 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm151 normal mapping 4) ROTO orbits and slew start icks - ock 12411 slew starts at 495 - ock 12425 slew starts at 766 - ock 12426 slew starts at 562 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: NONE UNTIL END OF STORM 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - will be twice per month, includes only double scan mode 12) mosaics - NONE UNTIL END OF STORM 13) 12 days loaded p12433.img notes: DUST STORM MONITORING - bistatic radar maneuver protection 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm151 normal mapping 4) ROTO orbits and slew start icks - ock 12472 slew starts at 464 - ock 12482 slew starts at 651 - ock 12487 slew starts at 666 - ock 12491 slew starts at 675 - ock 12493 slew starts at 587 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: NONE UNTIL END OF STORM 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - will be twice per month, includes only double scan mode 12) mosaics - NONE UNTIL END OF STORM 13) no additional days from p12410 upload 14) bistatic radar maneuver on ocks 12455-12456; TES commanded to stare nadir p12496.img notes: DUST STORM MONITORING - complete table overwrite 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm151 normal mapping 4) ROTO orbits and slew start icks - ock 12510 slew starts at 656 - ock 12511 slew starts at 631 - ock 12522 slew starts at 625 - ock 12533 slew starts at 708 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - will be twice per month, includes only double scan mode 12) mosaics - NONE UNTIL END OF STORM 13) 12 days loaded 14) used new tsl_loader with F option to force an overwrite of all table memory locations; trying to "fix" gremlin in memory that has truncated the albedo ref sequence, effectively removing the albedo lamp looks p12532.img notes: DUST STORM MONITORING 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm151 normal mapping 4) ROTO orbits and slew start icks - ock 12533 slew starts at 708 - ock 12547 slew starts at 708 - ock 12559 slew starts at 511 - ock 12560 slew starts at 700 - ock 12572 slew starts at 465 - ock 12582 slew starts at 687 5) limb: all forward looking, space, +75 degrees, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - will be twice per month, includes only double scan mode 12) mosaics - NONE UNTIL END OF STORM 13) 12 days loaded NOTE: spacecraft attitude error lead to timing error for ocks 12569-12572 p12581.img notes: DUST STORM MONITORING - MOVE TO 16 DEGREE RELAY ORIENTATION 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm152 16 degree offpoint mapping 4) ROTO orbits and slew start icks - ock 12606 slew starts at 1593 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -59.5,-54.5,-47,-26.5,0,26.5,47,54.5,59.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - not executing due to flight software logic error 12) mosaics - NONE UNTIL END OF STORM 13) all observations changed angles for 16 degree pitch (nadir now will be at mirror angle of -16), limbs to aft facing, space looks to aft (had been fore looking) 14) 12 days loaded 15) 16 degree pitch start on ock 12586; ocks 12581-12582 stare nadir with space/ref sets only 16) move to 16 degree orientation discontinues autonomous equator crossing broadcast - software under development to rectify problem will not be completed for another ~month; equator crossing commands will need to be issued in TES NIPCE's; - using last set broadcast prior to maneuver for course of the first several days of this upload because it has more accurate timing than that of ground predict [will start using ground predicts in p12618.img] p12618.img notes: ROTO UPDATE; SET_ORB COMMAND; START EQTRX FROM GROUND 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm152 16 degree offpoint mapping 4) ROTO orbits and slew start icks - ock 12631 slew starts at 1598 - ock 12644 slew starts at 1623 - ock 12658 slew starts at 649 - ock 12659 slew starts at 516 - ock 12667 slew starts at 699 - ock 12669 slew starts at 1593 - ock 12670 slew starts at 676 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test - not executing due to flight software logic error 12) mosaics - NONE UNTIL END OF STORM 13) all observations changed angles for 16 degree pitch (nadir now will be at mirror angle of -16), limbs to aft facing, space looks to aft (had been fore looking) 14) no additional schedules reused from p12581.img 15) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet; timing drifts will occur 16) set_orbit command being set to fix MGS-orbit/TES-ock number from MGS-PDS problem on 2001-226 NOTE: calculation error for equator crossing caused orbit period to be too long. Equator crossing not accurate, moving in latitude; calculated geometry data correct, but icks not occurring at "normal" latitude locations. ROTO observations therefore not all protected. ERROR: timing error of 2 minutes per orbit in the length of the orbit causing very fast drift and large disconnect with predicted equator crossing times. p12676.img notes: RESET COLDSTART AND RELOAD 1) coldstart command to power cycle TES p12678.img notes: NIPCE1- TES INITIATION SEQUENCE 1) equator crossing command and orbit period sent from ground 2) stare nadir (-16 degree) with space/reference sets 3) new space/albedo lamp sequence included 4) ALGOR flight software patch loaded p12679.img notes: NIPCE2- TES INITIATION SEQUENCE SET_ORB COMMAND; EQTRX FROM GROUND FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: partial mm152 16 degree offpoint mapping 4) ROTO orbits and slew start icks: NO ROTO's 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 1 and 2 collection 12) mosaics - NONE UNTIL END OF STORM 13) 12 days loaded 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur 15) set_orbit command set to fix orbit/ock number from cold start p12703.img notes: ROTO UPDATE; EQTRX FROM GROUND 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm152 16 degree offpoint mapping 4) ROTO orbits and slew start icks - ock 12719 slew starts at 424 - ock 12729 slew starts at 595 - ock 12731 slew starts at 1422 - ock 12754 slew starts at 692 - ock 12755 slew starts at 624 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set 12) mosaics - NONE UNTIL END OF STORM 13) no additional schedules from reset-NIPCE3 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur p12752.img notes: ROTO UPDATE; EQTRX FROM GROUND FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm152 16 degree offpoint mapping 4) ROTO orbits and slew start icks - ock 12754 slew starts at 692 - ock 12755 slew starts at 624 - ock 12767 slew starts at 628 - ock 12769 slew starts at 738 - ock 12771 slew starts at 631 - ock 12772 slew starts at 479 - ock 12773 slew starts at 774 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set 12) mosaics - NONE UNTIL DUST DISSIPATES 13) 12 days loaded 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur 15) fixed typo in limb scan angles p12788.img notes: ROTO UPDATE; EQTRX FROM GROUND FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm152 16 degree offpoint mapping; roto times preliminary from Elsa 4) ROTO orbits and slew start icks - ock 12802 slew starts at 718 - ock 12803 slew starts at 714 - ock 12804 slew starts at 710 - ock 12814 slew starts at 427 - ock 12816 slew starts at 728 - ock 12827 slew starts at 664 - ock 12839 slew starts at 662 - ock 12841 slew starts at 420 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set 12) mosaics - NONE UNTIL DUST DISSIPATES 13) no additional schedules from p12752.img upload 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur 15) fixed wavenumber offset, back to mapping shift (had not been updated with coldstart return to default value) NOTE: MGS entered C-Mode at start of 2002-249; all instruments powered off p12959.img notes: NIPCE1- TES INITIATION SEQUENCE 1) equator crossing command and orbit period sent from ground 2) stare nadir (-16 degree) with space/reference sets 3) new space/albedo lamp sequence included 4) ALGOR flight software patch loaded 5) wavenumber shift command NOTE: Power on command built by LMA p12960.img notes: NIPCE2- TES INITIATION SEQUENCE SET_ORB COMMAND; FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm153 16 degree offpoint mapping 4) ROTO orbits and slew start icks: NO ROTO's 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 1 and 2 collection 12) mosaics - NONE UNTIL END OF STORM 13) 12 days loaded 14) set_orbit command being set to fix orbit/ock number from TES power on p13048.img notes: EQTRX FROM GROUND FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm153 16 degree offpoint mapping, 4) ROTO orbits and slew start icks: NO ROTO's 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on orbit 12, added additional s/r set to orb 12) mosaics - NONE UNTIL DUST DISSIPATES 13) 12 days loaded 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur p13094.img notes: EQTRX FROM GROUND; SINGLE ROTO TEST ON COMM ORBIT; FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm153 16 degree offpoint mapping, 4) ROTO orbits and slew start icks - ock 13105 slew starts at 700 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set 12) mosaics - NONE UNTIL DUST DISSIPATES 13) 12 days loaded 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur p13131.img notes: EQTRX FROM GROUND; ROTOS TEST ON COMM ORBIT; FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm153 16 degree offpoint mapping, 4) ROTO orbits and slew start icks - ock 13166 slew starts at 420 - ock 13178 slew starts at 435 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set 12) mosaics - NONE UNTIL DUST DISSIPATES 13) no additional schedules 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur p13180.img notes: EQTRX FROM GROUND; ROTOS TEST ON COMM ORBIT; FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm153 16 degree offpoint mapping, 4) ROTO orbits and slew start icks - ock 13190 slew starts at 1991 - ock 13202 slew starts at 646 - ock 13216 slew starts at 416 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - NONE - dust dissipating, but timing drift unacceptable for targeting 13) 12 days loaded 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur p13219.img notes: EQTRX FROM GROUND; ROTOS AND MOC FOCUS CALIBRATION TEST; FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm153 16 degree offpoint mapping 4) ROTO orbits and slew start icks - ock 13227 slew starts at 702 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: removed until latitude offset fixed 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - NONE - dust dissipating but timing drift unacceptable for targeting 13) 12 days loaded 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur 15) MOC focus cals; TES soft idle -ocks 13238/39, 13251/52 (ick 2715-331) p13270.img notes: EQTRX FROM GROUND; MOC FOCUS CALIBRATION TEST; FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm153 16 degree offpoint mapping 4) no roots 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: removed until latitude offset fixed 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - NONE - dust dissipating but timing drift unacceptable for targeting 13) 12 days loaded 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur 15) MOC focus cals; TES soft idle -ocks 13282/83, 13316/17, 13342/43 (ick ~2700-330) p13351.img notes: EQTRX FROM GROUND; ROTOS; FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm153 16 degree offpoint mapping 4) ROTO orbits and slew start icks - ock 13367 slew starts at 1439 - ock 13368 slew starts at 1401 - ock 13382 slew starts at 1296 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 - sequence timing altered; added to upload for testing 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - NONE - dust dissipating but timing drift unacceptable for targeting 13) 12 days loaded 14) sending equator crossing times from ground, 16 degree offpoint does not contain eqtrx broadcasts yet - timing drifts will occur p13403.img notes: NIPCE1- TES INITIATION SEQUENCE 1) PDS giving eqtrx broadcasts - spacecraft in nadir mapping configuration 2) stare nadir (-16 degree offset) with space/reference sets 3) ALGOR flight software patch loaded 4) wavenumber shift command in mplan NOTE: Power on command built by LMA p13406.img notes: NIPCE2- TES INITIATION SEQUENCE SET_ORB COMMAND; FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit, - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm154 16 degree offpoint mapping 4) no rotos 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) space_ref_long: on 12th orbit; 10 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 1 and 2 collection 12) mosaics - NONE 13) 12 days loaded 14) set_orbit command being set to fix orbit/ock number from power on p13512.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm154 16 degree offpoint mapping, 4) No ROTOs - stopped for start of ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 - sequence timing altered, added to upload for testing 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - NONE 13) 12 days loaded p13599.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm154 16 degree offpoint mapping, 4) No ROTOs - stopped for ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 - sequence timing altered, added to upload for testing 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - NONE 13) 12 days loaded p13699.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm155 16 degree offpoint mapping, 4) No ROTOs - stopped for ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 - sequence timing altered, added to upload for testing 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - - targeted 5 x 13, single scan, dayside: JJ8, ock 13728; JJ1, ock 13777; - targeted 5 x 7, double scan, dayside: Eos Chasma, ock 13734; - targeted 5 x 7, double scan, nightside: Isidis Land1, ock 13711; Coprates A, ock 13716; Nilosyrtus, ock 13736; Gale Cr., ock 13747; NW Tyrrhena, ock 13748; Arda Vallis, ock 13778; Coprates B, ock 13779; SE Arsia A, ock 13781; - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 13) 12 days loaded p13770.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm155 16 degree offpoint mapping, 4) No ROTOs - stopped for ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 - sequence timing altered, added to upload for testing 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - - targeted 5 x 13, single scan, dayside: none - targeted 5 x 7, double scan, dayside: JJ1, ock 13777; W. Hematite Landing site 2, ock 13808; - targeted 5 x 7, double scan, nightside: Arda Vallis, ock 13778; Coprates B, ock 13779; SE Arsia A, ock 13781, Gusev Landing site, ock 13821; W. Hematite Landing site 1, ock 13839/13840; - targeted 3 x 23, double scan, dayside, cloud/volc: none - targeted 3 x 23, double scan, nightside, cloud/volc: none 13) 12 days loaded p13864.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm155 16 degree offpoint mapping, 4) No ROTOs - stopped for ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 - sequence timing altered, added to upload for testing 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - - targeted 5 x 7, double scan, nightside: Coprates Chasma B, ock 13892; 13) 12 days loaded p13949.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm155 16 degree offpoint mapping, 4) No ROTOs - stopped for ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 - sequence timing altered, added to upload for testing 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - - targeted 5 x 7, double scan, dayside: JJ3, ock 13967; JJ7, ock 13988; JJ4, ock 14006; - targeted 5 x 7, double scan, nightside: SE Arsia Mons B, ock 13957; Phlegra Montes, ock 13959; E Isidis A, ock 13993; 13) 12 days loaded p14039.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm156 16 degree offpoint mapping, 4) No ROTOs - stopped for ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 - sequence timing altered, added to upload for testing 10) space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) albedo lamp 2 test on 12th orbit - added additional space/reference set to orbit 12) mosaics - - targeted 5 x 7, double scan, dayside: Vicky1, ock 14120; - targeted 5 x 7, double scan, nightside: Arda Valles, ock 14067; Coprates Chasma A, ock 14093; SE Arsia Mons A, ock 14070; Nilosyrtus, ock 14113; DeuteronilusB, ock 14052; 13) 14 days loaded p14108.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm156 16 degree offpoint mapping, 4) No ROTOs - stopped for ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) mosaics - - targeted 5 x 7, double scan, dayside: Vicky1, ock 14120; - targeted 5 x 7, double scan, nightside: Nilosyrtus, ock 14113; W. Hematite 3, ock 14129/14130; Arda Valles, ock 14155; Coprates Chasma B, ock 14156; SE Arssia Mons A, ock 14158; 12) 14 days loaded p14204.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm156 16 degree offpoint mapping, 4) No ROTOs - stopped for ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) mosaics - - targeted 5 x 7, double scan, dayside: JJ5, ock 14208; - targeted 5 x 7, double scan, nightside: W. Hematite 1, ock 14247/14248; NW Tyrrhena, ock 14213; Coprates Chasma A, ock 14269; SE Arssia Mons A, ock 14246; 12) 12 days loaded p14297.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm156 16 degree offpoint mapping 4) No ROTOs - stopped for ODYSSEY aerobraking 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 12) 14 days loaded p14383.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequence: partial mm156 16 degree offpoint mapping 4) ROTO orbits and slew start icks - ock 14399 slew starts at ick 413 - ock 14406 slew starts at ick 669 - ock 14456 slew starts at ick 1501 - ock 14468 slew starts at ick 1271 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) mosaics - - targeted 5 x 7, double scan, dayside: Malin playa, ock 14423; JJ4, ock 14471 - targeted 5 x 7, double scan, nightside: Nilosytus, ock 14402; Phlegra, ock 14424; Deuteronilus[b], ock 14429; Arda Valles, ock 14444 12) 14 days loaded p14456.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: mm156 and mm157 16 degree offpoint mapping 4) ROTO orbits and slew start icks - ock 14456 slew starts at ick 1501 - ock 14468 slew starts at ick 1271 - ock 14496 slew starts at ick 1426 - ock 14552 slew starts at ick 1329 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) mosaics - - targeted 5 x 7, double scan, dayside: JJ4, ock 14471; Hematite[5], ock 14489; Vicky[1], ock 14497 - targeted 5 x 7, double scan, nightside: Gale Crater, ock 14501/14502 12) 14 days loaded p14551.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 3) upload covers spacecraft command sequences: mm156 and mm157 16 degree offpoint mapping 4) ROTO orbits and slew start icks - ock 14552 slew starts at ick 1329 - ock 14553 slew starts at ick 1267 - ock 14594 slew starts at ick 1502 - ock 14600 slew starts at ick 412 - ock 14612 slew starts at ick 885 - ock 14615 slew starts at ick 1324 - ock 14625 slew starts at ick 1392 5) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 6) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 7) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 9) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 10) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 11) mosaics - - targeted 5 x 7, double scan, dayside: JJ8, ock 14570; Vicky[3], ock 14601 - targeted 5 x 7, double scan, nightside: Nilosyrtus, ock 14578 12) 14 days loaded p14640.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; IMC ON; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) IMC flight software patch loaded: +65 to -65 singles on nightside 3) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 4) upload covers spacecraft command sequences: mm157 and mm158 16 degree offpoint mapping 5) ROTO orbits and slew start icks - ock 14650 slew starts at ick 1394 - ock 14672 slew starts at ick 1455 - ock 14713 slew starts at ick 1394 6) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 7) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 8) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 10) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 11) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) mosaics - - targeted 5 x 7, double scan, dayside: none due to loading IMC - targeted 5 x 7, double scan, nightside: none due to loading IMC 13) 14 days loaded ERROR: loading of IMC software patch caused synchronization and pointing mirror angle errors; all reference looks are unreliable, so no data is processed NOTE: two other uploads were attempted without success to correct and diagnose IMC problem initiated with this upload (p14726.img and p14784.img) p14797.img notes: NIPCE1- TES INITIATION SEQUENCE 1) coldstart command to power cycle TES and remove IMC NIPCE2- TES INITIATION SEQUENCE FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) ALGOR flight software patch loaded 2) IMC flight software patch off 3) optical switch 00 4) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 5) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 6) upload covers spacecraft command sequence: mm158 16 degree offpoint mapping 7) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none, checking instrument health - targeted 5 x 7, double scan, nightside: none, checking instrument health 14) NO new days loaded p14798.img notes: 1) set_orb equator crossing command p14834.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 4) upload covers spacecraft command sequence: mm158 16 degree offpoint mapping 5) ROTO orbits and slew start icks - ock 14848 slew starts at ick 1457 - ock 14858 slew starts at ick 1505 - ock 14870 slew starts at ick 1275 - ock 14871 slew starts at ick 671 - ock 14873 slew starts at ick 1460 6) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 7) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 8) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 10) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 11) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) mosaics - - targeted 5 x 7, double scan, dayside: none, checking instrument health - targeted 5 x 7, double scan, nightside: none, checking instrument health 13) 12 days loaded p14895.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 4) upload covers spacecraft command sequence: mm158 16 degree offpoint mapping 5) ROTO orbits and slew start icks - ock 14929 slew starts at ick 1328 - ock 14933 slew starts at ick 1267 - ock 14954 slew starts at ick 1617 6) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 7) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 8) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 10) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 11) new_space_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 13) 12 days loaded p14968.img notes: FULL TIME 10cm-1 (SINGLES SCAN) MODE; IMC ON; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) IMC flight software patch loaded: +65 to -65 singles on nightside 3) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 4) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 5) upload covers spacecraft command sequence: mm159 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 14992 slew starts at ick 1326 - ock 14994 slew starts at ick 1265 - ock 15001 slew starts at ick 948 - ock 15012 slew starts at ick 1476 - ock 15022 slew starts at ick 1367 - ock 15049 slew starts at ick 1455 7) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_refimc_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mirror scan test on ock 14968: - 0 to 180 to 0 (full 360 degree circle) in 10 degree steps with 5 icks at each angle - 2.25 to 172.25 to 2.25 (full 360 degree circle) in 20 degree steps with 5 icks at each angle - all new pmt entries 14) mosaics - - targeted 5 x 7, single scan, dayside: none due to loading IMC - targeted 5 x 7, single scan, nightside: none due to loading IMC 15) 12 days loaded ERROR: loading of IMC software patch caused synchronization and pointing mirror angle errors; all reference looks are unreliable, so no data is processed NOTE: upload p14982.img was planned to remove patch but spacecraft entered C-mode at ock 14981 before upload was radiated p15092.img notes: POWER ON - TES INITIATION SEQUENCE 1) power-on/power-off after C-mode, reload tables NOTE: Power on command built by LMA (mi043901) ERROR: TES did not come out of prom, bad mission plan checksum occurred in NIPCE1 affecting table load: - coldstart after power-on as expected - warmstart due to bad mission plan checksum - attempted to load Algor patch but could not due to tables not being properly loaded - automated coldstart (second time) - TES in PROM mode until ock 15128 p15129.img notes: NIPCE1- TES INITIATION SEQUENCE FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) ALGOR flight software patch loaded 2) IMC flight software patch off 3) optical switch 00 4) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 5) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 6) upload covers spacecraft command sequences: partial mm159 and mm160 16 degree offpoint mapping - mm160 initiates beta supplement with 3 periods of solar panel motion 7) No ROTOs 8) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 9) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 10) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 11) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 12) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 13) new_space_dbl_ref_long: on 12th orbit; 12 icks at ick 280, 830, and 3430 - during HGA and Solar Array motion and fixed period [for instrument response studies] 14) mosaics - - targeted 5 x 7, double scan, dayside: none, checking instrument health - targeted 5 x 7, double scan, nightside: none, checking instrument health 15) 12 days loaded NOTE: Power on command built by LMA (mi044691) p15130.img notes: 1) set_orb equator crossing command p15237.img notes: FULL TIME 5cm-1 (DOUBLE SCAN) MODE; 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) for all orbits: - spatial mask, full spectral for entire orbit - long packets for entire orbit 4) upload covers spacecraft command sequences: mm161 and mm162 beta supplement with 16 degree offpoint mapping 5) No ROTOs 6) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 7) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 8) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 9) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 10) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 11) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 13) 12 days loaded NOTE: MGS went to low data rate during this upload: detector masks and packet lengths not adjusted causing buffer overflow and data loss p15323.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -46 to +45 deg lat, full spectral, spatial mask night = +46(asc) to +75(dec) deg lat, spectral mask, spatial mask south pole = -76(dec) to -45(asc) deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm163 and mm164 beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 15242 slew starts at ick 562 7) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none, testing buffer management - targeted 5 x 7, double scan, nightside: none, testing buffer management 14) 12 days loaded NOTE: MGS in low data rate during this upload: detector masks and packet lengths not fully adjusted causing buffer overflow and data loss ERROR: MGS entered C-MODE at ock 15385 due to Star-X problem - misidentification of 20 stars p15505.img notes: NIPCE1- TES INITIATION SEQUENCE 15 ORBIT OBSERVATION CYCLE 1) ALGOR flight software patch loaded 2) limited tables loaded NOTE1: Power on command built by LMA (mi051001) p15506.img notes: NIPCE2- TES INITIATION SEQUENCE 15 ORBIT OBSERVATION CYCLE 1) set_orb equator crossing command 2) optical switch 00 3) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 4) data in doubles mode (5 cm-1) day surface = -36 to +35 deg lat, full spectral, spatial mask day and pole = +36(asc) to +75(dec) deg lat, polar spectral mask, spatial mask south pole = -76(dec) to -35(asc) deg lat, polar spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial (see ERROR) - short packets except for space/reference sets 6) upload covers spacecraft command sequences: mm167 and mm168 beta supplement with 16 degree offpoint mapping 7) No ROTOs 8) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 9) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 10) EPF mirror angles= -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5; 3 icks at each angle, all detectors returned 11) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 12) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 13) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 14) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 15) 12 days loaded ERROR: Loss of all single scan data due to incorrect spectral mask applied to reference observations; can not calibrate data ERROR: MGS in low data rate during this upload: detector masks and packet lengths not fully adjusted causing buffer overflow and data loss p15579.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -26 to +25 deg lat, full spectral, spatial mask day and pole = +26(asc) to +75(dec) deg lat, polar spectral mask, spatial mask south pole = -76(dec) to -45(asc) deg lat, polar spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, polar spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm170 through mm172 beta supplement with 16 degree offpoint mapping 6) No ROTOs 7) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded ERROR: MGS in low data rate; detector masks and packet lengths not fully adjusted causing buffer overflow and data loss p15666.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -16 to +15 deg lat, full spectral, spatial mask day and pole = +16(asc) to +75(dec) deg lat, polar spectral mask, spatial mask south pole = -76(dec) to -15(asc) deg lat, polar spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm171 through mm174 beta supplement with 16 degree offpoint mapping 6) No ROTOs 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded ERROR: MGS in low data rate; detector masks and packet lengths not fully adjusted causing buffer overflow and data loss p15750.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -11 to +10 deg lat, full spectral, spatial mask day and pole = +11(asc) to +75(dec) deg lat, polar spectral mask, spatial mask south pole = -76(dec) to -10(asc) deg lat, polar spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm174 through mm176 beta supplement with 16 degree offpoint mapping 6) No ROTOs 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: JJ2, ock 15839 - targeted 5 x 7, double scan, nightside: W. Hematite2, ock 15813; Melas Chasma, ock 15803 14) 12 days loaded ERROR: MGS in low data rate; detector masks and packet lengths not fully adjusted causing buffer overflow and data loss p15835.img notes: 15 ORBIT OBSERVATION CYCLE; CONCURRENT THEMIS OBSERVATIONS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -9 to +8 deg lat, full spectral, spatial mask day and pole = +9(asc) to +75(dec) deg lat, polar spectral mask, spatial mask south pole = -76(dec) to -8(asc) deg lat, polar spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm175 through mm177 beta supplement with 16 degree offpoint mapping 6) No ROTOs 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: JJ2, ock 15839 - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded 15) Concurrent THEMIS observations; TES stares nadir for 4 degrees lat - ock 15836 nadir icks 930-972 - ock 15840 nadir icks 2718-2759 - ock 15843 nadir icks 2708-2749 - ock 15845 nadir icks 955-996 - ock 15846 nadir icks 953-993 - ock 15849 nadir icks 2701-2742 - ock 15853 nadir icks 2718-2759 - ock 15855 nadir icks 948-988 - ock 15857 nadir icks 2692-2732 - ock 15859 nadir icks 954-994 - ock 15860 nadir icks 2722-2762 ERROR: MGS in low data rate; detector masks and packet lengths not fully adjusted causing buffer overflow and data loss p15873.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -9 to +8 deg lat, full spectral, spatial mask day to pole = +9(asc) to +75(dec) deg lat, polar spectral mask, spatial mask south pole = -76(dec) to -8(asc) deg lat, polar spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm177-mm178 and mz171a; beta supplement with 16 degree offpoint mapping 6) No ROTOs; MOC focus cals TES stares nadir (-16 degree) for duration - ock 15876 slew starts at 3165 - ock 15890 slew starts at 2986 - ock 15904 slew starts at 2990 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded ERROR: MGS in low data rate; detector masks and packet lengths not fully adjusted causing buffer overflow and data loss p15947.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -11 to +10 deg lat, full spectral, spatial mask day to pole = +11(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together) south pole = -76(dec) to -10(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm178-mm179 and mz172-mz173; beta supplement with 16 degree offpoint mapping 6) No ROTOs; MOC focus cals; TES stares nadir (-16 degree) for duration - ock 15949 slew starts at 3010 - ock 15998 slew starts at 3019 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded ERROR: MGS in low data rate; detector masks and packet lengths not fully adjusted causing buffer overflow and data loss p16007.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -11 to +10 deg lat, full spectral, spatial mask day to pole = +11(asc) to +65(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together) south pole = -66(dec) to -10(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +66 to -65 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm179 through mm181; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 16012 slew starts at 1266 - ock 16013 slew starts at 1074 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3000 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 10 days loaded ERROR: MGS in low data rate; detector masks and packet lengths almost fully adjusted causing some buffer overflow and data loss p16105.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -11 to +10 deg lat, full spectral, spatial mask day to pole = +11(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together) south pole = -76(dec) to -10(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm181-mm182 and mz175; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 16122 slew starts at 1332 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded p16119.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -11 to +10 deg lat, full spectral, spatial mask day to pole = +11(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together) south pole = -76(dec) to -10(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm181-mm182 and mz175; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 16122 slew starts at 1332 - ock 16135 slew starts at 869 - ock 16172 slew starts at 1125 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded p16178.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = -2 to +19 deg lat, full spectral, spatial mask day to pole = +20(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together) south pole = -76(dec) to -1(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm183 through mm185 and mz177-mz178; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 16195 slew starts at 950 - ock 16196 slew starts at 1396 - ock 16208 slew starts at 1441 - ock 16232 slew starts at 1245 - ock 16233 slew starts at 1358 - ock 16246 slew starts at 1433 - ock 16263 slew starts at 1590 - ock 16265 slew starts at 1269 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded p16253.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = +0 to +20 deg lat, full spectral, spatial mask day to pole = +21(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together) south pole = -76(dec) to -1(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm185 through mm187 and mz178 through mz180; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 16263 slew starts at 1590 - ock 16265 slew starts at 1269 - ock 16277 slew starts at 1340 - ock 16284 slew starts at 1394 - ock 16303 slew starts at 1527 - ock 16304 slew starts at 1365 - ock 16319 slew starts at 1479 - ock 16333 slew starts at 1523 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded p16350.img notes: 15 ORBIT OBSERVATION CYCLE 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = +1 to +21 deg lat, full spectral, spatial mask day to pole = +22(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together) south pole = -76(dec) to +0(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm187 through mm189 and mz181-mz182; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 16355 slew starts at 1556 - ock 16363 slew starts at 1422 - ock 16370 slew starts at 1030 - ock 16403 slew starts at 1451 - ock 16416 slew starts at 1269 - ock 16418 slew starts at 1555 - ock 16428 slew starts at 1336 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: vicky2, ock 16436 - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded p16433.img notes: 15 ORBIT OBSERVATION CYCLE; CONCURRENT THEMIS OBSERVATION; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = +2.5 to +22.5 deg lat, full spectral, spatial mask day to pole = +23(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together) south pole = -76(dec) to +2(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm189 through mm191 and mz183-mz184; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 16440 slew starts at 812 - ock 16450 slew starts at 1408 - ock 16465 slew starts at 1256 - ock 16488 slew starts at 972 - ock 16491 slew starts at 1506 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: vicky2, ock 16436 - targeted 5 x 7, double scan, nightside: none 14) Concurrent THEMIS observations; TES stares nadir for 4 degrees lat - ock 16440 nadir icks 2442-2622 - THEMIS attempting to image MGS spacecraft 15) 12 days loaded 16) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency; - no change of TES observation cycle to accommodate spacecraft slew - nadir slew from ockA, ick 3330 to ockB, ick 600 for ockA/ockB: 16438/16439; 16442/16443; 16446/16447; 16450/16451; 16454/16455; 16458/16459; 16462/16463; 16466/16467; 16470/16471; 16473/16474; 16478/16479; 16481/16482; 16484/16485; 16487/16488; 16490/16491; 16493/16494; 16496/16497; 16499/16500; 16502/16503; 16505/16506; 16508/16409; 16511/16512; 16514/16515 p16521.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = +3 to +24 deg lat, full spectral, spatial mask day to pole = +25(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together) south pole = -76(dec) to +2(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm191 through mm193 and mz185-mz186; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 16525 slew starts at 1621 - ock 16529 slew starts at 1271 - ock 16562 slew starts at 874 - ock 16574 slew starts at 1182 - ock 16589 slew starts at 1201 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) Concurrent THEMIS observations; TES stares nadir for 4 degrees lat - ock 16440 nadir icks 2442-2622 - THEMIS attempting to image MGS spacecraft 15) 12 days loaded 16) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency - no change of TES observation cycle to accommodate spacecraft slew - nadir slew from ockA, ick 3330 to ockB, ick 600 for ockA/ockB: 16523/16524; 16530/16531; 16531/16532; 16532/16533; 16535/16536; 16538/16539; 16541/16542; 16544/16545; 16547/16548; 16550/16551; 16555/16556; 16556/16557; 16559/16560; 16560/16561; 16563/16564; 16569/16570; 16576/16577; 16577/16578; 16578/16579; 16582/16583; 16584/16585; 16587/16588; 16590/16591; 16593/16594; 16596/16597; 16599/16600; 16602/16603; 16605/16606 p16606.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = +4 to +25 deg lat, full spectral, spatial mask day to pole = +26(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +3(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm193, mm194, mm195, mz 187, and mz 188; beta supplement with 16 degree off point mapping 6) ROTO orbits and slew start icks - ock 16613 slew starts at 1621 - ock 16638 slew starts at 1625 - ock 16649 slew starts at 901 - ock 16677 slew starts at 1391 - ock 16680 slew starts at 1269 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 10) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 11) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 12) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 13) 12 days loaded 14) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency - no change of TES observation cycle to accommodate spacecraft slew - nadir slew from ockA, ick 3330 to ockB, ick 600 for ockA/ockB: 16608/16609; 16609/16610; 16613/16614; 16615/16616; 16618/16619; 16621/16622; 16624/16625; 16627/16628; 16630/16631; 16633/16634; 16636/16637; 16639/16640; 16642/16643; 16644/16645; 16646/16647; 16649/16650; 16652/16653; 16655/16656; 16658/16659; 16661/16662; 16664/16665; 16667/16668; 16670/16671; 16673/16674; 16681/16682; 16682/16683; 16683/16684; 16685/16686; 16688/16689; 16691/16692 p16692.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = +6 to +26 deg lat, full spectral, spatial mask day to pole = +27(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +5(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm195, mm196, mm197, and mz 190; beta supplement with 16 degree off point mapping 6) ROTO orbits and slew start icks - ock 16742 slew starts at 1282 - ock 16761 slew starts at 1409 7) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded 16) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency - no change of TES observation cycle to accommodate spacecraft slew - nadir slew from ockA, ick 3330 to ockB, ick 600 for ockA/ockB: 16693/16694; 16695/16696; 16698/16699; 16701/16702; 16706/16707; 16707/16708; 16710/16711; 16713/16714; 16716/16717; 16718/16719; 16722/16723; 16726/16727; 16728/16729; 16730/16731; 16732/16733; 16734/16735; 16737/16738; 16740/16741; 16746/16747; 16747/16748; 16749/16750; 16752/16753; 16755/16756; 16758/16759; 16761/16762; 16764/16765; 16767/16768; 16770/16771; 16773/16774; 16776/16777 NOTE: Fewer realtime passes than expected available for emptying the buffer; caused overflow and data loss starting ock 16715 to 16750 p16778.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 2nd, 4th, 6th, 8th, 10th, 12th, and 14th orbits 3) data in doubles mode (5 cm-1) day surface = +7 to +27 deg lat, full spectral, spatial mask day to pole = +28(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +6(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm197, mm198, mm199, mz 191a, and mz 192; beta supplement with 16 degree off point mapping 6) ROTO orbits and slew start icks; changed to detector_mask=1 - ock 16780 slew starts at 1054 - ock 16782 slew starts at 1532 - ock 16790 slew starts at 1204 - ock 16796 slew starts at 1455 - ock 16812 slew starts at 1363 - ock 16826 slew starts at 1681 - ock 16847 slew starts at 1497 - ock 16856 slew starts at 1268 7) limb: all aft looking, space, limb set (100 km height, 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none, due to buffer management problem - targeted 5 x 7, double scan, nightside: none, due to buffer management problem 14) 12 days loaded 15) Last data collecting upload before solar conduction 16) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency - no change of TES observation cycle to accommodate spacecraft slew - nadir slew from ockA, ick 3330 to ockB, ick 600 for ockA/ockB: 16783/16784; 16784/16785; 16786/16787; 16789/16790; 16792/16793; 16798/16799; 16799/16800; 16801/16802; 16804/16805; 16807/16808; 16810/16811; 16812/16813; 16814/16815; 16818/16819; 16820/16821; 16823/16824; 16827/16828; 16829/16830; 16832/16833; 16835/16836; 16838/16839; 16841/16842; 16844/16845; 16847/16848; 16850/16851; 16852/16853; 16856/16857; 16859/16860; 16862/16863; 16869/16870; 16870/16871; 16871/16872; 16874/16875; 16877/16878; 16878/16879; 16881/16880; 16884/16885 p16887.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS SOLAR CONJUNCTION UPLOAD 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 10th orbit 3) data in doubles mode (5 cm-1) day surface = +8 to +28 deg lat, full spectral, spatial mask day to pole = +29(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +7(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm199, mm200, mm201, and mm202; beta supplement with 16 degree off point mapping and solar conjunction - NO data downlink for mm199, mm200, and mm201; recording and downlink resumes with mm202 6) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 7) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 8) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 9) 22 days loaded 10) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency and to reduce need for Angular Momentum Desaturation (CMD) events - no change of TES observation cycle to accommodate spacecraft slew - nadir slew of spacecraft three times per every twelve orbits - nadir slew from ockA, ick 3330 to ockB, ick 600 for ockA/ockB: (individual ock not listed as data were not downlinked during solar conjunction) NOTE: Data downlinked only for ock 17111 to 17130 (post solar conjunction) p17131.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS POST-SOLAR CONJUNCTION UPLOAD 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 10th orbit - full spectral, spatial mask (detector_mask=1) 3) data in doubles mode (5 cm-1) day surface = +8 to +28 deg lat, full spectral, spatial mask day to pole = +29(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +7(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm203, mm204, and mm205; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 17132 slew starts at 1301 - ock 17134 slew starts at 1532 - ock 17145 slew starts at 1565 - ock 17156 slew starts at 1772 - ock 17169 slew starts at 1245 - ock 17186 slew starts at 1746 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded 15) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency and to reduce need for Angular Momentum Desaturation (AMD) events - changes of TES observation cycle to accommodate spacecraft slew: limb and EPF angles adjusted during nadir dwell periods - nadir slew of spacecraft three times per every twelve orbits - nadir slew from ockA, ick 3330 to ockB, ick 600 for ockA/ockB: 17135/17136; 17136/17137; 17138/17139; 17141/17142; 17146/17147; 17147/17148; 17150/17151; 17153/17154; 17157/17158; 17160/17161; 17163/17164; 17166/17167; 17169/17170; 17172/17173; 17175/17176; 17178/17179; 17181/17182; 17184/17185; 17187/17188; 17190/17191; 17193/17194; 17196/17197; 17199/17200; 17202/17203; 17205/17206 p17206.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 10th orbit - full spectral, spatial mask (detector_mask=1) 3) data in doubles mode (5 cm-1) day surface = +11 to +31 deg lat, full spectral, spatial mask day to pole = +32(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +10(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm204, mm205, mm206, mm207 and mz196-197; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 17220 slew starts at 1055 - ock 17228 slew starts at 1145 - ock 17267 slew starts at 2009 - ock 17272 slew starts at 1364 - ock 17291 slew starts at 1308 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded 15) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency and to reduce need for Angular Momentum Desaturation (AMD) events - changes of TES observation cycle to accommodate spacecraft slew: limb and EPF angles adjusted during nadir dwell periods - nadir slew of spacecraft three times per every twelve orbits - nadir slew from ockA, ick 3330 to ockB, ick 600 for ockA/ockB: 17209/17210; 17211/17212; 17212/17213; 17213/17214; 17214/17215; 17217/17218; 17218/17219; 17219/17220; 17221/17222; 17223/17224; 17225/17226; 17227/17228; 17229/17230; 17230/17231; 17231/17232; 17232/17233; 17234/17235; 17235/17236; 17245/17246; 17246/17247; 17247/17248; 17248/17249; 17250/17251; 17252/17253; 17254/17255; 17256/17257; 17257/17258; 17258/17259; 17259/17260; 17260/17261; 17262/17263; 17264/17265; 17266/17267; 17268/17269; 17270/17271; 17271/17272; 17272/17273; 17273/17274; 17275/17276; 17277/17278; 17279/17280; 17281/17282; 17282/17283; 17283/17284; 17284/17285; 17286/17287; 17288/17289; 17290/17291; 17291/17292; 17294/17295 p17233.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 10th orbit - full spectral, spatial mask (detector_mask=1) 3) data in doubles mode (5 cm-1) day surface = +11 to +31 deg lat, full spectral, spatial mask day to pole = +32(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +10(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm205, mm206, mm207, mm208, and mz197; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 17272 slew starts at 1364 - ock 17291 slew starts at 1308 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded 15) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency and to reduce need for Angular Momentum Desaturation (AMD) events - changes of TES observation cycle to accommodate spacecraft slew: limb and EPF angles adjusted during nadir dwell periods - nadir slew of spacecraft six to seven times per every twelve orbits - nadir slew from ockA, ick 3330 to ockB, ick 600 for ockA/ockB: 17233/17234; 17234/17235; 17235/17236; 17236/17237; 17245/17246; 17246/17247; 17247/17248; 17248/17249; 17249/17250; 17250/17251; 17251/17252; 17252/17253; 17253/17254; 17254/17255; 17255/17256; 17256/17257; 17257/17258; 17258/17259; 17259/17260; 17260/17261; 17261/17262; 17262/17263; 17263/17264; 17264/17265; 17265/17266; 17266/17267; 17267/17268; 17268/17269; 17269/17270; 17270/17271; 17271/17272; 17272/17273; 17273/17274; 17274/17275; 17275/17276; 17276/17277; 17277/17278; 17278/17279; 17279/17280 ERROR: multiple warmstarts due to incorrect timing of idle ick within space/ref observations sequence at beginning and end of nadir dwell periods; all space/ref observations are lost and data quality during nadir dwell is compromised p17319.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 10th orbit - full spectral, spatial mask (detector_mask=1) 3) data in doubles mode (5 cm-1) day surface = +11.8 to +31.8 deg lat, full spectral, spatial mask day to pole = +32(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +10(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm207, mm208, mm209, mm210, and mz199; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 17341 slew starts at 1179 - ock 17343 slew starts at 1401 - ock 17359 slew starts at 1520 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded 15) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency and to reduce need for Angular Momentum Desaturation (AMD) events - changes of TES observation cycle to accommodate spacecraft slew: limb and EPF angles adjusted during nadir dwell periods - nadir slew of spacecraft six to seven times per every twelve orbits - nadir slew from ockA, ick 3330 to ockB, ick 600 for each of the following ockA: ock 17319 through ock 17378; ock 17380 through ock 17415; ock 17417 through ock 17464 NOTE: timing of idle ick within space/ref observations sequence at beginning and end of naidir dwell periods fixed with this upload p17378.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 10th orbit - full spectral, spatial mask (detector_mask=1) 3) data in doubles mode (5 cm-1) day surface = +12.5 to +32.5 deg lat, full spectral, spatial mask day to pole = +33(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +12(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm208, mm209, mm210, mz200, and mz201; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 17381 slew starts at 1200 - ock 17382 slew starts at 1774 - ock 17412 slew starts at 1455 - ock 17413 slew starts at 1066 - ock 17414 slew starts at 1497 - ock 17415 slew starts at 1432 - ock 17417 slew starts at 1404 - ock 17418 slew starts at 977 - ock 17430 slew starts at 1621 - ock 17431 slew starts at 1402 - ock 17441 slew starts at 18807 - ock 17445 slew starts at 1219 - ock 17455 slew starts at 1362 - ock 17465 slew starts at 1439 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded 15) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency and to reduce need for Angular Momentum Desaturation (AMD) events - changes of TES observation cycle to accommodate spacecraft slew: limb and EPF angles adjusted during nadir dwell periods - nadir slew of spacecraft eight times per every twelve orbits - nadir slew from ockA, ick 3330 to ockB, ick 600 for each of the following ockA: ock 17378; ock 17380 through ock 17415; ock 17417 through ock 17464 p17462.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 10th orbit - full spectral, spatial mask (detector_mask=1) 3) data in doubles mode (5 cm-1) day surface = +13 to +33 deg lat, full spectral, spatial mask day to pole = +34(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +12(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm210, mm211, mm212, mz202, and mz203; beta supplement with 16 degree offpoint mapping 6) ROTO orbits and slew start icks - ock 17465 slew starts at 1439 - ock 17469 slew starts at 1201 - ock 17515 slew starts at 1397 - ock 17516 slew starts at 1423 - ock 17527 slew starts at 991 - ock 17528 slew starts at 1436 - ock 17548 slew starts at 1489 - ock 17549 slew starts at 1528 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded 15) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency and to reduce need for Angular Momentum Desaturation (AMD) events - changes of TES observation cycle to accommodate spacecraft slew: limb and EPF angles adjusted during nadir dwell periods - nadir slew of spacecraft eight times per every twelve orbits - nadir slew from ockA, ick 3330 to ockB, ick 600 for each of the following ockA: ock 17462 through ock 17550 p17546.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 10th orbit - full spectral, spatial mask (detector_mask=1) 3) data in doubles mode (5 cm-1) day surface = +14 to +34 deg lat, full spectral, spatial mask day to pole = +35(asc) to +75(dec) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) south pole = -76(dec) to +13(asc) deg lat, polar spectral mask, spatial mask (all detectors averaged together, detector_mask=1) reference = full spectral, full spatial - short packets except for space/reference sets 4) data in singles mode (10 cm-1) night = +76 to -75 deg lat, spectral mask, spatial mask reference = full spectral, full spatial - short packets except for space/reference sets 5) upload covers spacecraft command sequences: mm212, mm213, mm214, and mz204; beta supplement with 16 degree offpoint mapping mz204 6) ROTO orbits and slew start icks - ock 17560 slew starts at 987 - ock 17561 slew starts at 1367 - ock 17567 slew starts at 911 - ock 17588 slew starts at 1454 - ock 17590 slew starts at 1527 - ock 17614 slew starts at 1121 - ock 17625 slew starts at 1980 - ock 17626 slew starts at 1005 7) limb: all aft looking, space, limb set (100 km height 1/2 degree steps, padded by one look at surface angle) - all short packets, full spatial 8) limbs every 20 degrees, alternating 1st and 2nd orbits with 10 degree offset between orbits 9) EPF = -75.5,-70.5,-63,-42.5,-16,10.5,31,38.5,43.5 angles, 3 icks at each angle, all detectors returned 10) 1 S-polar, and 1 nightside epf per cycle; 15 orbits in full cycle; 2 or 3 dayside epf per 3rd orbit (epf-only orbit), using only -75 to +75 cycle, with -90 (S-polar), and +20 (nightside) 11) dense epf: one per day (on epf-only orbit), cycling in 15 degree latitude steps -75, -60, -45, -30, -15, 0, 15 12) new_space_ref_long: on 12th orbit; 12 icks at ick 180, 830, and 3170 - during HGA and Solar Array motion and fixed period [for instrument response studies] 13) mosaics - - targeted 5 x 7, double scan, dayside: none - targeted 5 x 7, double scan, nightside: none 14) 12 days loaded 15) MGS spacecraft slewing to true nadir at descending equator crossing for improved fuel efficiency and to reduce need for Angular Momentum Desaturation (AMD) events - changes of TES observation cycle to accommodate spacecraft slew: limb and EPF angles adjusted during nadir dwell periods - nadir slew of spacecraft eight times per every twelve orbits - nadir slew from ockA, ick 3330 to ockB, ick 600 for each of the following ockA: ock 17546 through ock 17606; ock 17618 through ock 17636 p17583.img notes: 15 ORBIT OBSERVATION CYCLE; MGS NADIR SLEWS; RADIO SCIENCE SLEWS 1) optical switch 00 2) stare nadir (-16 degree) to force internal check of mirror position - for 20 icks starting at ick 700 per 10th orbit - full spectral, spatial mask (detector_mask=1) 3) data in doubles mode (5 cm-1) day surface = +14 to +34 deg lat, full spectral, spatial mask day to pole = +35(asc) to +75(dec) deg lat, pol