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2
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3
Description
1
Group
508_PasTest opportunity segment PasiphaeWorking Group 2
ASTRO_INNERAstrometry inner moonsWorking Group 2
ASTRO_IRR_ELARA Working Group 2
ASTRO_IRR1_CARPOAstrometry irregular moon CARPOWorking Group 2
ASTRO_IRR1_CHALDENEAstrometry irregular moon CHALDENEWorking Group 2
ASTRO_IRR1_HIMALIAAstrometry irregular moon HIMALIAWorking Group 2
ASTRO_IRR1_KALLICHOREAstrometry irregular moon KALLICHOREWorking Group 2
ASTRO_IRR1_LEDAAstrometry irregular moon LEDAWorking Group 2
ASTRO_IRR1_LYSITHEAAstrometry irregular moon LYSITHEAWorking Group 2
ASTRO_IRR1_MEGACLITEASTRO_IRR1_MEGACLITEWorking Group 2
ASTRO_IRR1_TAYGETEAstrometry irregular moon TAYGETEWorking Group 2
ASTRO_IRR1_THEMISTOAstrometry irregular moon THEMISTOWorking Group 2
ASTRO_IRR2_ANANKEAstrometry irregular moon AnankeWorking Group 2
ASTRO_IRR2_CARMEAstrometry irregular moon CarmeWorking Group 2
ASTRO_IRR2_PASIPHAEastrometry measurement with inertial pointing to moon Pasiphae Working Group 2
ASTRO_IRR2_SINOPE Working Group 2
CALLISTO_DISTANT Working Group 2
CALLISTO_FB_RSCallisto Flyby remote sensingWorking Group 2
CALLISTO_FLYBY_WG2 Working Group 2
CHAR_IRR1Characterization irregular moons group 1 (see list below)Working Group 2
CHARACTERIZATION_IRR_ELARACharacterization irregular moon ElaraWorking Group 2
CHARACTERIZATION_IRR2_ANANKECharacterization irregular moon ANANKEWorking Group 2
CHARACTERIZATION_IRR2_CARME Working Group 2
CHARACTERIZATION_IRR2_PASIPHAEcharacterization irregular moon PasiphaeWorking Group 2
CHARACTERIZATION_IRR2_SINOPECharacterization irregular moon SinopeWorking Group 2
EUROPA_DISTANT Working Group 2
EUROPA_FB_RSEuropa Flyby remote sensingWorking Group 2
EUROPA_FLYBY_WG2 Working Group 2
GANYMEDE_DISTANT Working Group 2
GANYMEDE_FB_RSGanymede flyby remote sensingWorking Group 2
GANYMEDE_FLYBY_WG2 Working Group 2
HIGHPHPROFILErings high phase profile (JANUS DEF)Working Group 2
IO_ECLIPSEIo observation while Io is in eclipse.Working Group 2
IO_MAJ_COMPOSITIONIO_MAJ_COMPOSITIONWorking Group 2
IO_MAJ_HOTSPOTSIO_MAJ_HOTSPOTSWorking 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
IO_TOR_DUSTIo torus dustWorking Group 2
RING_HPRing high phaseWorking Group 2
RING_LPRing low phaseWorking 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_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_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_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
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
RINGMOSAICRINGMOSAIC (Janus definition). impression of the extent of the whole ring systemWorking Group 2
RINGPHASE Working Group 2
RINGSPIRAL_HPRINGSPIRAL_HP (high phase, Janus def)Working Group 2
RINGSPIRAL_MPRINGSPIRAL_MP (medium phase: JANUS Def)Working Group 2
ROI_INTERSECTIONROI_INTERSECTIONWorking Group 2
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

64 segment definitions