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SHADOWEDGErings 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 extensionWorking Group 2
ROI_INTERSECTIONROI_INTERSECTIONWorking Group 2
RINGSPIRAL_MPRINGSPIRAL_MP (medium phase: JANUS Def)Working Group 2
RINGSPIRAL_HPRINGSPIRAL_HP (high phase, Janus def)Working Group 2
RINGMATTERRINGMATTER. 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
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_5Opportunity 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 degWorking Group 2
RING_PHASECURV_40 Working Group 2
RING_PHASECURV_30 Working Group 2
RING_PHASECURV_20 Working Group 2
RING_PHASECURV_170 Working Group 2
RING_PHASECURV_160 Working Group 2
RING_PHASECURV_150 Working Group 2
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_10Opportunity 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 degWorking Group 2
RING_LPRing low phaseWorking Group 2
RING_HPRing high phaseWorking Group 2
J_SAT_VALETUDO Working Group 2
J_SAT_THYONE-Working Group 2
J_SAT_THEMISTO Working Group 2
J_SAT_TAYGETE Working Group 2
J_SAT_SINOPE 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_PRAXIDIKE Working Group 2
J_SAT_PHILOPHROSYNE-Working Group 2
J_SAT_PASITHEE Working Group 2
J_SAT_PASIPHAE Working Group 2
J_SAT_PANDIA Working Group 2
J_SAT_ORTHOSIE-Working Group 2
J_SAT_OBSJ_SAT_OBSWorking Group 2
J_SAT_MNEME-Working Group 2
J_SAT_MEGACLITE Working Group 2
J_SAT_LYSITHEA Working Group 2
J_SAT_LEDA Working Group 2
J_SAT_KALYKE-Working Group 2
J_SAT_KALLICHORE Working Group 2
J_SAT_KALE-Working Group 2
J_SAT_ISONOE Working Group 2
J_SAT_IRR_CHAR_E Working Group 2
J_SAT_IRR_AST_E Working Group 2
J_SAT_IOCASTE Working Group 2
J_SAT_INN_CHAR_A Working Group 2
J_SAT_INN_AST_T Working Group 2
J_SAT_INN_AST_A Working Group 2
J_SAT_HIMALIA Working Group 2
J_SAT_HERSE Working Group 2
J_SAT_HERMIPPE Working Group 2
J_SAT_HELIKE Working Group 2
J_SAT_HEGEMONE Working Group 2
J_SAT_HARPALYKE Working Group 2
J_SAT_EUPORIE-Working Group 2
J_SAT_EUPHEME-Working Group 2
J_SAT_EUKELADE-Working Group 2
J_SAT_EUANTHE-Working Group 2
J_SAT_ERSA Working Group 2
J_SAT_ERINOME Working Group 2
J_SAT_ELARA Working Group 2
J_SAT_EIRENE-Working Group 2
J_SAT_DIA-Working Group 2
J_SAT_CHALDENE Working Group 2
J_SAT_CARPO-Working Group 2
J_SAT_CARME Working Group 2
J_SAT_CALLIRRHOE Working Group 2
J_SAT_AUTONOE Working Group 2
J_SAT_ARCHE Working Group 2
J_SAT_AOEDE Working Group 2
J_SAT_ANANKE Working Group 2
J_SAT_AITNE-Working Group 2
J_SAT_516_MetJ_SAT_516_MetWorking Group 2
J_SAT_515_AdrJ_SAT_515_AdrWorking Group 2
J_SAT_514_TheJ_SAT_514_TheWorking Group 2
J_SAT_505_AmaJ_SAT_505_AmaWorking Group 2
J_SATjupiter satellite GENERICWorking Group 2
J_RING Working Group 2
IO_TOR_DUSTIo torus dustWorking Group 2
IO_RS Working Group 2
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

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