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,