View segment definition

DL_
DL_
Downlink communication prime segments.
pointing: HGA pointing to Earth, power optimized
CReMA 3.0, CReMA 3.1, CReMA 3.2, CREMA_5_0, CREMA_5_0b23_1, CREMA_5_1_150lb_23_1, CREMA_5_1_150lb_23_1_a3, CREMA_5_1_150lb_23_1_b2
True
GENERIC

Pointing

-

Scheduler

None
-

Observation Definitions

PEL_JUPITER_IN_SITU_NOMINAL_1, PEL_JUPITER_IN_SITU_IMAGING_NOMINAL_1, PEL_JUPITER_IN_SITU_IMAGING_BURST_1, PEL_JUPITER_IN_SITU_IMAGING_LOW_1, RPWI Instrument Downlink, MAG_DL, MAG_DL_FOB, PEL_GANYMEDE_IN_SITU_LOW_1, PEL_JUPITER_IN_SITU_BURST_1, PEL_JUPITER_IN_SITU_LOW_1, PEL_GANYMEDE_IN_SITU_LOW_5, MAG_DL_LIGHT_ONLY, MAG_DL_FOB_LIGHT_ONLY, PEL_GANYMEDE_IN_SITU_NOMINAL_3, PEL_GANYMEDE_IN_SITU_LOW_6, PEL_GANYMEDE_IN_SITU_LOW_7, 3GM_GRAVITY_GCO500_200, 3GM_GRAVITY_TOUR, PEH_JUPITER_IN_SITU_IMAGING_NOMINAL_1, PEH_JUPITER_IN_SITU_NOMINAL_1, PEH_JUPITER_IN_SITU_IMAGING_BURST_1

Advanced

Current implementation in geopipeline:
- computed for Malargue (ESTRACK)
- visibility events start when ground-station to SC reaches 10 deg elevation above local ground station horizon
- 9 hours segment duration defined from the visibility start event
- the duration includes slew times of 30mn added TWICE to simulate slew toward the HGA pointing (assumed to start slewing at visibility start event) and back - so the total pass duration is 9h as default, with 8 hours for actual transmission
- Filtering for the TOUR phase: remove those segments where at least one occultation is found by (jupiter, callisto, europa, ganymede or io) AND/OR if part of segment in superior solar conjunction (SES limit 3 deg)
- Filtering for the Ganymede phase (down to 500 km phase): segments redefined around occulting bodies (jupiter, callisto, europa, ganymede or io), keeping only segments with at least 3h10 mn duration to take into account 5 mn margin before and after each occultation AND/OR superior solar conjunction taken into account (SES limit 3 deg)
- For Ganymede 200 km phase: the minimum segment duration is reduced to 1 hour
- Both filtered and unfiltered passes files are produced, for each station
during first 8 hours of visibility of MLG station. Extended during phase 3.