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Description
Group
JM_ENA Working Group 3
JM_GM Working Group 3
G_IS Working Group 3
E_IS Working Group 3
C_IS Working Group 3
CALLISTO_ENAFar approach energetic neutral atom imaging of CallistoWorking Group 3
CALLISTO_FLYBY_RPWI_IONO_AJS Working Group 3
CALLISTO_WAKEIn situ Callisto wake observationWorking Group 3
EUROPA_ENAFar approach energetic neutral atom imaging of EuropaWorking Group 3
EUROPA_FLYBY_RPWI_IONO_AJS Working Group 3
EUROPA_TOR_ISIn situ Europa torus observationWorking Group 3
EUROPA_WAKEIn situ Europa wake observationWorking Group 3
GANYMEDE_ENAFar approach energetic neutral atom imaging of GanymedeWorking Group 3
GANYMEDE_GMIn situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environmentWorking Group 3
GANYMEDE_FLYBY_RPWI_IONO_AJS Working Group 3
GANYMEDE_WAKEIn situ Ganymede wake observationWorking Group 3
JUPITER_CPSIn situ Jupiter current/plasma sheet observationWorking Group 3
JUPITER_ENAImaging of Jupiter's magnetosphere in energetic neutral atoms (ENAs).Maximize pitch angle coverage with PEP JEI,JDC,JoEE, JENI (ion mode) a) JENI has a broad FoV and captures Jupiter and the Io/Europa torus and magnetosphere at most times. No special pointing design required for JENI besides requiring an approximate nadir pointing (considerable offsets can still be acceptable) b) JNA disk-shaped/slit FoV has a slight offset from the XZ spacecraft plane, meaning that during nadir pointing, it images preferentially the northern or southern extension of the Europa/Io torus, whereas Jupiter may be in the edge or outside of the FoV, especially at large distances. Scans (small rotations around Sc-X) or periods with stable, small offset of the SC-xz plane from Nadir can help to better image stronger emissions from the equatorial torusWorking Group 3
JUPITER_GMIn situ mapping of global configuration and monitoring dynamics of the Jovian magnetospheric environment. corotation should be in the FoV of PEP/JDC or PEP/JEI. Conditions for coverage: ◦ Minimum angle less than about 11.25 deg (half-azimuthal sector size) of a JEI or JDC pixel from corotation ◦ Boresight angle of JDC or JEI less than ˜90 deg Conditions for ideal coverage: ◦ Minimum angle less than about 11.25 deg (half-azimuthal sector size) of a JEI or JDC pixel from corotation ◦ Boresight angle less than ˜75 deg (JEI) or 70 deg (JDC): corotation away from the FoV edge JDC is preferred for monitoring corotation, over JEI, when possible.Working Group 3
JUPITER_NULLIn situ Jupiter magnetic null searchWorking Group 3
JUPITER_PDTIn situ Jupiter particle distribution transition region observation. Maximize pitch angle coverage for PEP/JEI, JDC,JoEE, JENI (ion mode)Working Group 3
JUPITER_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking Group 3
RINGMOSAICRINGMOSAIC (Janus definition). impression of the extent of the whole ring systemWorking Group 2
RINGPHASE Working Group 2
G_RS_36G11G_RS_36G11Working Group 2
G_RS_35G10G_RS_35G10Working Group 2
G_RS_34G9G_RS_34G9Working Group 2
G_RS_32G8G_RS_32G8Working Group 2
G_RS_28G7G_RS_28G7Working Group 2
G_RS_27G6G_RS_27G6Working Group 2
C_RS_33C23C_RS_33C23Working Group 2
C_RS_31C22C_RS_31C22Working Group 2
C_RS_30C21 Working Group 2
C_RS_26C19 Working Group 2
RINGSPIRAL_MPRINGSPIRAL_MP (medium phase: JANUS Def)Working Group 2
RINGSPIRAL_HPRINGSPIRAL_HP (high phase, Janus def)Working 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
IO_MAJ_HOTSPOTSIO_MAJ_HOTSPOTSWorking Group 2
IO_MAJ_COMPOSITIONIO_MAJ_COMPOSITIONWorking 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
HIGHPHPROFILErings high phase profile (JANUS DEF)Working Group 2
IO_ECLIPSEIo observation while Io is in eclipse.Working Group 2
E_RS_OBSEuropa remote sensing generic segment containing obs database linkWorking Group 2
C_RS_OBSCallisto Remote sensing GENERIC containing obs database linkWorking Group 2
G_RS_OBSG_RS GENERICWorking Group 2
C_RS_29C20C_RS_29C20Working Group 2
C_RS_25C18C_RS_25C18Working Group 2
C_RS_24C17C_RS_24C17Working Group 2
C_RS_23C16C_RS_23C16Working Group 2
C_RS_22C15C_RS_22C15Working Group 2
C_RS_21C14C_RS_21C14Working Group 2
C_RS_20C13C_RS_20C13Working Group 2
C_RS_19C12C_RS_19C12Working Group 2
C_RS_18C11C_RS_18C11Working Group 2
C_RS_17C10C_RS_17C10Working Group 2
C_RS_16C9C_RS_16C9Working Group 2
C_RS_15C8C_RS_15C8Working Group 2
C_RS_14C7C_RS_14C7Working Group 2
C_RS_13C6C_RS_13C6Working Group 2
C_RS_12C5C_RS_12C5Working Group 2
C_RS_11C4C_RS_11C4Working Group 2
C_RS_10C3C_RS_10C3Working Group 2
C_RS_9C2C_RS_9C2Working Group 2
C_RS_6C1C_RS_6C1Working Group 2
E_RS_8E2E_RS_8E2Working Group 2
E_RS_7E1E_RS_7E1Working Group 2
G_RS_1G1 Working Group 2
G_RS_5G5 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_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
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_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_LPRing low phaseWorking Group 2
RING_HPRing high phaseWorking Group 2
EUROPA_DISTANT Working Group 2
J_SATjupiter satellite GENERICWorking Group 2
G_RS_4G4 Working Group 2
G_RS_3G3HAA as per 3GM UM IS considering NIMWorking Group 2
G_RS_2G2 Working Group 2
IO_RS Working Group 2
J_RING Working Group 2
EUROPA_FB_RSEuropa Flyby remote sensingWorking Group 2
CALLISTO_FB_RSCallisto Flyby remote sensingWorking Group 2
GANYMEDE_FB_RSGanymede flyby remote sensingWorking Group 2
G_distant Working Group 2
E_RS Working Group 2

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