RING_PHASECURV_140 | | Working Group 2 |
RING_PHASECURV_130 | | Working Group 2 |
RING_PHASECURV_120 | | Working Group 2 |
RING_PHASECURV_110 | | Working Group 2 |
RING_PHASECURV_100 | | Working Group 2 |
RING_PHASECURV_90 | | Working Group 2 |
RING_PHASECURV_80 | | Working Group 2 |
RING_PHASECURV_70 | | Working Group 2 |
RING_PHASECURV_60 | | Working Group 2 |
RING_PHASECURV_50 | | Working Group 2 |
RING_PHASECURV_40 | | Working Group 2 |
RING_PHASECURV_30 | | Working Group 2 |
RING_PHASECURV_20 | | Working Group 2 |
EUROPA_DISTANT | | Working Group 2 |
J_SAT_INN_AST_A | | Working Group 2 |
J_SAT_IRR_AST_E | | Working Group 2 |
J_SAT_INN_CHAR_A | | Working Group 2 |
J_SAT_INN_AST_T | | Working Group 2 |
J_SAT_IRR_CHAR_E | | Working Group 2 |
G_RS_26G11 | | Working Group 2 |
G_RS_25G10 | | Working Group 2 |
G_RS_24G9 | | Working Group 2 |
G_RS_23G8 | | Working Group 2 |
G_RS_22G7 | | Working Group 2 |
C_RS_21C13 | | Working Group 2 |
C_RS_20C12 | | Working Group 2 |
C_RS_19C11 | | Working Group 2 |
G_RS_18G6 | | Working Group 2 |
G_RS_17G5 | | Working Group 2 |
C_RS_16C10 | | Working Group 2 |
C_RS_15C9 | | Working Group 2 |
C_RS_14C8 | | Working Group 2 |
C_RS_13C7 | | Working Group 2 |
C_RS_12C6 | | Working Group 2 |
C_RS_11C5 | | Working Group 2 |
C_RS_10C4 | | Working Group 2 |
C_RS_9C3 | | Working Group 2 |
C_RS_8C2 | | Working Group 2 |
E_RS_7E2 | | Working Group 2 |
E_RS_6E1 | | Working Group 2 |
C_RS_5C1 | | Working Group 2 |
G_RS_4G4 | | Working Group 2 |
G_RS_2G2 | | Working Group 2 |
IO_RS | | Working Group 2 |
J_RING | | Working Group 2 |
FB_RS | | Working Group 2 |
G_distant | | Working Group 2 |
E_RS | | Working Group 2 |
E_distant | | Working Group 2 |
C_RS | | Working Group 2 |
C_distant | | Working Group 2 |
ASTRO_IRR2_SINOPE | | Working Group 2 |
ASTRO_IRR_ELARA | | Working Group 2 |
CALLISTO_DISTANT | | Working Group 2 |
CALLISTO_FLYBY_WG2 | | Working Group 2 |
CHARACTERIZATION_IRR2_CARME | | Working Group 2 |
EUROPA_FLYBY_WG2 | | Working Group 2 |
GANYMEDE_DISTANT | | Working Group 2 |
GANYMEDE_FLYBY_WG2 | | Working Group 2 |
GANYMEDE_FLYBY_UVS | | Working Group 1 |
C_GPH_21C13 | | Working Group 1 |
C_GPH_19C11 | | Working Group 1 |
G_GPH_17G5 | | Working Group 1 |
C_GPH_16C10 | | Working Group 1 |
C_GPH_15C9 | | Working Group 1 |
C_GPH_14C8 | | Working Group 1 |
C_GPH_13C7 | | Working Group 1 |
C_GPH_11C5 | | Working Group 1 |
C_GPH_10C4 | | Working Group 1 |
C_GPH_9C3 | | Working Group 1 |
C_GPH_8C2 | | Working Group 1 |
E_GPH_7E2 | | Working Group 1 |
E_GPH_6E1 | | Working Group 1 |
C_GPH_5C1 | | Working Group 1 |
G_GPH_4G4 | | Working Group 1 |
G_GPH_2G2 | | Working Group 1 |
G_GPH | | Working Group 1 |
E_GPH | | Working Group 1 |
C_GPH | | 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 |
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 |
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 |
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 |
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 |
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 |
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) | GENERIC |
ASTRO_INNER | Astrometry inner moons | Working Group 2 |