| J_SAT_CARME | | Working Group 2 |
|---|
| J_SAT_CARPO | | Working Group 2 |
|---|
| J_SAT_CHALDENE | | Working Group 2 |
|---|
| J_SAT_DIA | | Working Group 2 |
|---|
| J_SAT_EIRENE | | Working Group 2 |
|---|
| J_SAT_ELARA | | Working Group 2 |
|---|
| J_SAT_ERINOME | | Working Group 2 |
|---|
| J_SAT_ERSA | | Working Group 2 |
|---|
| J_SAT_EUANTHE | | Working Group 2 |
|---|
| J_SAT_EUKELADE | | Working Group 2 |
|---|
| J_SAT_EUPHEME | | Working Group 2 |
|---|
| J_SAT_EUPORIE | | Working Group 2 |
|---|
| J_SAT_HARPALYKE | | Working Group 2 |
|---|
| J_SAT_HEGEMONE | | Working Group 2 |
|---|
| J_SAT_HELIKE | | Working Group 2 |
|---|
| J_SAT_HERMIPPE | | Working Group 2 |
|---|
| 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_OBS | J_SAT_OBS | 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_HP | Ring high phase | Working Group 2 |
|---|
| RING_LP | Ring low phase | Working Group 2 |
|---|
| RING_PHASECURV_10 | Opportunity implementation in geopipeline
SC distance to Jupiter larger than 8e5 km
SC elevation above the rings lower than 0.5 deg
Only one Ansae tested for phase conditions - value must be between 10 deg and 20 deg | 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_5 | Opportunity implementation in geopipeline
SC distance to Jupiter larger than 8e5 km
SC elevation above the rings lower than 0.5 deg
Only one Ansae tested for phase conditions - value must be between 5 deg and 10 deg | 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 |
|---|
| RINGMATTER | RINGMATTER. Observations of the main rings and the gossamer rings, imaging the ring ansae from moderately large elevation.
The moderatly large elevation will reveal azimuthal structure in the rings and the presence of clumps at the resolution limit of the imaging. | Working Group 2 |
|---|
| RINGSPIRAL_HP | RINGSPIRAL_HP (high phase, Janus def) | Working Group 2 |
|---|
| RINGSPIRAL_MP | RINGSPIRAL_MP (medium phase: JANUS Def) | Working Group 2 |
|---|
| ROI_INTERSECTION | ROI_INTERSECTION | Working Group 2 |
|---|
| SHADOWEDGE | rings SHADOWEDGE. Imaging of the ring region intersected by the planetary shadow at moderate
elevation and very high phase. Especially for the very faint gossamer rings and the Thebe
extension | Working Group 2 |
|---|
| C_GPH_10C3 | C_GPH_10C3 | Working Group 1 |
|---|
| C_GPH_11C4 | C_GPH_11C4 | Working Group 1 |
|---|
| C_GPH_12C5 | C_GPH_12C5 | Working Group 1 |
|---|
| C_GPH_13C6 | C_GPH_13C6 | Working Group 1 |
|---|
| C_GPH_14C7 | C_GPH_14C7 | Working Group 1 |
|---|
| C_GPH_15C8 | C_GPH_15C8 | 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_18C11 | C_GPH_18C11 | Working Group 1 |
|---|
| C_GPH_19C12 | C_GPH_19C12 | Working Group 1 |
|---|
| C_GPH_20C13 | C_GPH_20C13 | Working Group 1 |
|---|
| C_GPH_21C14 | C_GPH_21C14 | Working Group 1 |
|---|
| C_GPH_22C15 | C_GPH_22C15 | Working Group 1 |
|---|
| C_GPH_23C16 | C_GPH_23C13 | Working Group 1 |
|---|
| C_GPH_24C17 | C_GPH_24C17 | Working Group 1 |
|---|
| C_GPH_25C18 | C_GPH_25C18 | Working Group 1 |
|---|