View segment definition

DL_
DL_
assuming:
JMAG: 2.31 kbps
RPWI: 1.7*2.167 kbps (Ballparks numbers from the team)
PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018)
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

PEP_JUPITER_IN_SITU_NOMINAL_1, PEP_JUPITER_IN_SITU_IMAGING_NOMINAL_1, PEP_JUPITER_IN_SITU_IMAGING_BURST_1, PEP_JUPITER_IN_SITU_IMAGING_LOW_1, RPWI Instrument Downlink, 3GM_HAA_CALIBRATION, 3GM GRAVITY FOR EPHEMERIDES, HAA_STDBY, 3GM USO SWON, PEP_GANYMEDE_IN_SITU_LOW_1, PEP_JUPITER_IN_SITU_BURST_1, PEP_JUPITER_IN_SITU_LOW_1, PEP_GANYMEDE_IN_SITU_LOW_5, PEP_GANYMEDE_IN_SITU_NOMINAL_3, PEP_GANYMEDE_IN_SITU_LOW_6, PEP_GANYMEDE_IN_SITU_LOW_7, PEP_GANYMEDE_IN_SITU_LOW_8, DRAFT_3GM_GRAVITY_TOUR

Advanced

Current implementation in geopipeline:
- computed for Canberra (DSN), Cebreros (ESTRACK), Goldstone (DSN), Madrid (DSN), Malargue (ESTRACK)
- visibility events start when ground-station to SC reaches 10 deg elevation above local ground station horizon
- 8 hours segment defined from the visibility start
- 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
- 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: 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)
- Both filtered and unfiltered passes files are produced, for each station
during first 8 hours of visibility of MLG station. Extended during phase 3.
SWI monitoring of the moons not considered for now