J_SAT_HERSE | | Working Group 2 |
J_SAT_HIMALIA | | Working Group 2 |
J_SAT_INN_AST_A | | Working Group 2 |
J_SAT_INN_AST_T | | Working Group 2 |
J_SAT_INN_CHAR_A | | Working Group 2 |
J_SAT_IOCASTE | | Working Group 2 |
J_SAT_IRR_AST_E | | Working Group 2 |
J_SAT_IRR_CHAR_E | | Working Group 2 |
J_SAT_ISONOE | | Working Group 2 |
J_SAT_KALE | | Working Group 2 |
J_SAT_KALLICHORE | | Working Group 2 |
J_SAT_KALYKE | | Working Group 2 |
J_SAT_LEDA | | Working Group 2 |
J_SAT_LYSITHEA | | Working Group 2 |
J_SAT_MEGACLITE | | Working Group 2 |
J_SAT_MNEME | | Working Group 2 |
J_SAT_ORTHOSIE | | Working Group 2 |
J_SAT_PANDIA | | Working Group 2 |
J_SAT_PASIPHAE | | Working Group 2 |
J_SAT_PASITHEE | | Working Group 2 |
J_SAT_PHILOPHROSYNE | | Working Group 2 |
J_SAT_PRAXIDIKE | | Working Group 2 |
J_SAT_S2003_J10 | | Working Group 2 |
J_SAT_S2003_J12 | | Working Group 2 |
J_SAT_S2003_J16 | | Working Group 2 |
J_SAT_S2003_J19 | | Working Group 2 |
J_SAT_S2003_J4 | | Working Group 2 |
J_SAT_S2003_J9 | | Working Group 2 |
J_SAT_S2010_J1 | | Working Group 2 |
J_SAT_S2010_J2 | | Working Group 2 |
J_SAT_S2011_J2 | | Working Group 2 |
J_SAT_S2016_J1 | | Working Group 2 |
J_SAT_S2017_J2 | | Working Group 2 |
J_SAT_S2017_J3 | | Working Group 2 |
J_SAT_S2017_J5 | | Working Group 2 |
J_SAT_S2017_J6 | | Working Group 2 |
J_SAT_S2017_J7 | | Working Group 2 |
J_SAT_S2017_J9 | | Working Group 2 |
J_SAT_SINOPE | | Working Group 2 |
J_SAT_TAYGETE | | Working Group 2 |
J_SAT_THEMISTO | | Working Group 2 |
J_SAT_THYONE | | Working Group 2 |
J_SAT_VALETUDO | | Working Group 2 |
RING_PHASECURV_100 | | Working Group 2 |
RING_PHASECURV_110 | | Working Group 2 |
RING_PHASECURV_120 | | Working Group 2 |
RING_PHASECURV_130 | | Working Group 2 |
RING_PHASECURV_140 | | Working Group 2 |
RING_PHASECURV_150 | | Working Group 2 |
RING_PHASECURV_160 | | Working Group 2 |
RING_PHASECURV_170 | | Working Group 2 |
RING_PHASECURV_20 | | Working Group 2 |
RING_PHASECURV_30 | | Working Group 2 |
RING_PHASECURV_40 | | Working Group 2 |
RING_PHASECURV_50 | | Working Group 2 |
RING_PHASECURV_60 | | Working Group 2 |
RING_PHASECURV_70 | | Working Group 2 |
RING_PHASECURV_80 | | Working Group 2 |
RING_PHASECURV_90 | | Working Group 2 |
RINGPHASE | | Working Group 2 |
C_GPH | | Working Group 1 |
C_GPH_10C4 | | Working Group 1 |
C_GPH_11C5 | | Working Group 1 |
C_GPH_13C7 | | Working Group 1 |
C_GPH_14C8 | | Working Group 1 |
C_GPH_15C9 | | Working Group 1 |
C_GPH_16C10 | | Working Group 1 |
C_GPH_17C10 | | Working Group 1 |
C_GPH_19C11 | | Working Group 1 |
C_GPH_21C13 | | Working Group 1 |
C_GPH_5C1 | | Working Group 1 |
C_GPH_8C2 | | Working Group 1 |
C_GPH_9C3 | | Working Group 1 |
CALLISTO_FLYBY | | Working Group 1 |
CALLISTO_FLYBY_3GM | | Working Group 1 |
CALLISTO_FLYBY_GALA | | Working Group 1 |
CALLISTO_FLYBY_JANUS | | Working Group 1 |
CALLISTO_FLYBY_MAJIS | | Working Group 1 |
E_GPH | | Working Group 1 |
E_GPH_6E1 | | Working Group 1 |
E_GPH_7E2 | | Working Group 1 |
EUROPA_FLYBY | | Working Group 1 |
EUROPA_FLYBY_3GM | | Working Group 1 |
EUROPA_FLYBY_GALA | | Working Group 1 |
EUROPA_FLYBY_JANUS | | Working Group 1 |
EUROPA_FLYBY_MAJIS | | Working Group 1 |
G_GPH | | Working Group 1 |
G_GPH_17G5 | | Working Group 1 |
G_GPH_2G2 | | Working Group 1 |
G_GPH_4G4 | | Working Group 1 |
GANYMEDE_FLYBY | | Working Group 1 |
GANYMEDE_FLYBY_3GM | | Working Group 1 |
GANYMEDE_FLYBY_GALA | | Working Group 1 |
GANYMEDE_FLYBY_JANUS | | Working Group 1 |
GANYMEDE_FLYBY_MAJIS | | Working Group 1 |
GANYMEDE_FLYBY_UVS | | Working Group 1 |
IO_MONITORING | - JANUS minimum distance = 7.00e+05 km
- MAJIS minimum distance = 8.00e+05 km
- SWI minimum distance = 6.00e+05 km (able to resolve target when angular size is > 1 mrad)
| Working Group 2 |
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 |
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 |
JMAG_CALROLL | 5 calibration roll needed by JMAG. 2 as soon as possible after JOI. 3 during phase 5: one at the start of phase 5, the last 2 as late as possible before GOI | WGX |