G_GPH_5G5 | G_GPH_5G5 | Working Group 1 |
G_GPH_3G3 | G_GPH_3G3 | Working Group 1 |
G_GPH_27G6 | G_GPH_27G6 | Working Group 1 |
G_GPH_26G6 | G_GPH_26G6 | Working Group 1 |
E_RS_OBS | Europa remote sensing generic segment containing obs database link | Working Group 2 |
E_GPH_OBS | Europa geophysics generic containing obs database link | Working Group 1 |
EARTH_OCC | Earth occultation by Jupiter | Working Group 4 |
SPICE_ATT_GOTOEARTH_COMMS | Earth communication segment | GENERIC |
E_RS_8E2 | E_RS_8E2 | Working Group 2 |
E_RS_7E1 | E_RS_7E1 | Working Group 2 |
E_IS_OBS | E_IS_OBS | Working Group 3 |
E_GPH_8E2 | E_GPH_8E2 | Working Group 1 |
E_GPH_7E1 | E_GPH_7E1 | Working Group 1 |
DL_ | Downlink communication prime segments.
pointing: HGA pointing to Earth | GENERIC |
SPICE_ATT_JUPITER_TOUR | Default attitude during the Tour phase | GENERIC |
SPICE_ATT_GANYMEDE_PHASE | Default attitude during the Ganymede phase | GENERIC |
SPICE_ATT_GOTOJUPITER_TOUR_SUP_SOL_CONJ | Default attitude during superior solar conjunction | GENERIC |
SPICE_ATT_GOTOTRANSFER_COLD_SUP_SOL_CONJ | Default attitude during cruise phase superior solar conjunctions 'cold' | GENERIC |
SPICE_ATT_TRANSFER_HOT | Default attitude during cruise phase applicable during the hot phases | GENERIC |
SPICE_ATT_TRANSFER_COLD | Default attitude during cruise phase | GENERIC |
C_GPH_15C7 | crema 3_2 | Working Group 1 |
JA_INCL_noDL | created for case 1 | Working Group 4 |
C_RS_OBS | Callisto Remote sensing GENERIC containing obs database link | Working Group 2 |
C_GPH_OBS | Callisto geophysics generic containing obs database link | Working Group 1 |
C_RS_9C2 | C_RS_9C2 | Working Group 2 |
C_RS_6C1 | C_RS_6C1 | Working Group 2 |
C_RS_33C23 | C_RS_33C23 | Working Group 2 |
C_RS_31C22 | C_RS_31C22 | Working Group 2 |
C_RS_31C21 | C_RS_31C21 | Working Group 2 |
C_RS_29C20 | C_RS_29C20 | Working Group 2 |
C_RS_28C19 | C_RS_28C19 | Working Group 2 |
C_RS_25C18 | C_RS_25C18 | Working Group 2 |
C_RS_24C17 | C_RS_24C17 | Working Group 2 |
C_RS_23C16 | C_RS_23C16 | Working Group 2 |
C_RS_22C15 | C_RS_22C15 | Working Group 2 |
C_RS_21C14 | C_RS_21C14 | Working Group 2 |
C_RS_20C13 | C_RS_20C13 | Working Group 2 |
C_RS_19C12 | C_RS_19C12 | Working Group 2 |
C_RS_18C11 | C_RS_18C11 | Working Group 2 |
C_RS_17C10 | C_RS_17C10 | Working Group 2 |
C_RS_16C9 | C_RS_16C9: Prime surface and exosphere segment defined as 24 hours centered at CA.
WG1 (gravity) is rider.
Pointing is mainly surface and/or limb (details TBD) | Working Group 2 |
C_RS_15C8 | C_RS_15C8 | Working Group 2 |
C_RS_14C7 | C_RS_14C7 | Working Group 2 |
C_RS_13C6 | C_RS_13C6 | Working Group 2 |
C_RS_12C5 | C_RS_12C5 | Working Group 2 |
C_RS_11C4 | C_RS_11C4 | Working Group 2 |
C_RS_10C3 | C_RS_10C3 | Working Group 2 |
C_IS_OBS | C_IS_OBS | Working Group 3 |
C_GPH_29C20 | C_GPH_29C20 | Working Group 1 |
C_GPH_28C19 | C_GPH_28C19 | Working Group 1 |
C_GPH_26C19 | C_GPH_26C19 | Working Group 1 |
C_GPH_25C18 | C_GPH_25C18 | Working Group 1 |
C_GPH_24C17 | C_GPH_24C17 | Working Group 1 |
C_GPH_23C16 | C_GPH_23C13 | Working Group 1 |
C_GPH_22C15 | C_GPH_22C15 | Working Group 1 |
C_GPH_21C14 | C_GPH_21C14 | Working Group 1 |
C_GPH_20C13 | C_GPH_20C13 | Working Group 1 |
C_GPH_19C12 | C_GPH_19C12 | Working Group 1 |
C_GPH_18C11 | C_GPH_18C11 | Working Group 1 |
C_GPH_16C9 | C_GPH_16C9
Geophysics prime segment, defined based on GALA (transmitting) operational range of altitude above Callisto < 2000 km.
Assumed Nadir pointing | Working Group 1 |
C_GPH_15C8 | C_GPH_15C8 | Working Group 1 |
C_GPH_14C7 | C_GPH_14C7 | Working Group 1 |
C_GPH_13C6 | C_GPH_13C6 | Working Group 1 |
C_GPH_12C5 | C_GPH_12C5 | Working Group 1 |
C_GPH_11C4 | C_GPH_11C4 | Working Group 1 |
C_GPH_10C3 | C_GPH_10C3 | Working Group 1 |
ECLIPSE_BATTERY_RECOVERY_FAST | Battery recharge after eclipse | GENERIC |
ECLIPSE_BATTERY_RECOVERY_STANDARD | Battery recharge after eclipse
pointing should be default power optimised pointing | GENERIC |
DL_EXT | assuming:
JMAG: 2.31 kbps
RPWI: 1.7*2.167 kbps
PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018) | GENERIC |
JM_PE | assuming:
JMAG: 2.31 kbps
RPWI: 1.7*2.167 kbps
PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018) | Working Group 3 |
CALIB | all calibrations activities to be included as part of the segmentation (e.g. calibration roll etc...) | WGX |
BATTERY_RECHARGE | 20.5 hour recovery segments to be scheduled after very demanding periods. For the moment only after flybys and eclipses.
Duration is derived from https://issues.cosmos.esa.int/juicewiki/display/SOCDEV/Downlink%2C+Recovery%2C+and+Eclipse+Scenario+Analysis | GENERIC |
RECOVERY_FLYBY | 15.15 hours recovery segments to be scheduled after flybys/eclipse, when standard instrument mode is assumed
Duration is derived from https://issues.cosmos.esa.int/juicewiki/display/SOCDEV/Downlink%2C+Recovery%2C+and+Eclipse+Scenario+Analysis
Pointing should be power optimized | GENERIC |
C_RS_30C21 | | Working Group 2 |
C_RS_26C19 | | Working Group 2 |
C_GPH_17C10 | | Working Group 1 |
SOC_OBSERVATION | | SOC |
3GM_OBSERVATION | | 3GM |
SWI_PRIME_OBSERVATION | | SWI |
RIME_PRIME_OBSERVATION | | RIME |
J_SAT_THYONE | | Working Group 2 |
J_SAT_S2017_J9 | | Working Group 2 |
J_SAT_S2017_J7 | | Working Group 2 |
J_SAT_S2017_J6 | | Working Group 2 |
J_SAT_S2017_J5 | | Working Group 2 |
J_SAT_S2017_J3 | | Working Group 2 |
J_SAT_S2017_J2 | | Working Group 2 |
J_SAT_S2016_J1 | | Working Group 2 |
J_SAT_S2011_J2 | | Working Group 2 |
J_SAT_S2010_J2 | | Working Group 2 |
J_SAT_S2010_J1 | | Working Group 2 |
J_SAT_S2003_J9 | | Working Group 2 |
J_SAT_S2003_J4 | | Working Group 2 |
J_SAT_S2003_J19 | | Working Group 2 |
J_SAT_S2003_J16 | | Working Group 2 |
J_SAT_S2003_J12 | | Working Group 2 |
J_SAT_S2003_J10 | | Working Group 2 |
J_SAT_PHILOPHROSYNE | | Working Group 2 |
J_SAT_ORTHOSIE | | Working Group 2 |
J_SAT_MNEME | | Working Group 2 |