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TRAJECTORY_SEGMENTdefined segment for moon coverage tool export functionnalityGENERIC
EUR_CAL_TRANSIT_PRDouble transit in front of Jupiter (Europa, Callisto)WGX
GAN_EUR_TRANSIT_PRDouble transit in front of Jupiter (Europa, Ganymede)WGX
GAN_CAL_TRANSIT_PRDouble transit in front of Jupiter (Ganymede, Callisto)WGX
E_GPH_7E1E_GPH_7E1Working Group 1
E_GPH_8E2E_GPH_8E2Working Group 1
E_IS_OBSE_IS_OBSWorking Group 3
E_RS_7E1E_RS_7E1Working Group 2
E_RS_8E2E_RS_8E2Working Group 2
SPICE_ATT_GOTOEARTH_COMMSEarth communication segmentGENERIC
EARTH_OCCEarth occultation by JupiterWorking Group 4
EARTH_OCC_EGRESSEarth occultation by Jupiter. EgressWorking Group 4
EARTH_OCC_INGRESSEarth occultation by Jupiter. IngressWorking Group 4
ECLIPSE_JUPITER_THERMALECLIPSE_JUPITER_THERMALGENERIC
EUROPA_FLYBY_RIME_AJSEuropa active radar opportunity, anti-jovian sideWorking Group 1
EUROPA_FLYBY_RIME_JSEuropa active radar opportunity, jovian sideWorking Group 1
EUROPA_FB_RSEuropa Flyby remote sensingWorking Group 2
E_GPH_OBSEuropa geophysics generic containing obs database linkWorking Group 1
EUROPA_RPWI_PASSIVRADEuropa passive radar opportunity for RPWIWorking Group 1
E_RS_OBSEuropa remote sensing generic segment containing obs database linkWorking Group 2
EUROPA_IONO_ISEUROPA_IONO_IS In situ Europa ionosphere observationWorking Group 3
EARTH_OCC_ETEvent tool support segment definitionGENERIC
FLYBY_ETEvent tool support segment definitionGENERIC
STELLAR_OCC_ETEvent tool support segment definitionGENERIC
SUN_OCC_ETEvent tool support segment definitionGENERIC
TRANSIT_ETEvent tool support segment definitionGENERIC
CALLISTO_ENAFar approach energetic neutral atom imaging of CallistoWorking Group 3
EUROPA_ENAFar approach energetic neutral atom imaging of EuropaWorking Group 3
GANYMEDE_ENAFar approach energetic neutral atom imaging of GanymedeWorking Group 3
FB_THERMALFB_THERMALGENERIC
JUPITER_FD_WOLFlight dynamics wheel off-loading slot, outside of Flyby preparation and recuperationGENERIC
G_GPH_26G6G_GPH_26G6Working Group 1
G_GPH_3G3G_GPH_3G3Working Group 1
G_GPH_5G5G_GPH_5G5Working Group 1
G_IS_OBSG_IS_OBSWorking Group 3
G_RS_OBSG_RS GENERICWorking Group 2
G_RS_26G6G_RS_26G6Working Group 2
G_RS_27G7G_RS_27G7Working Group 2
G_RS_30G8G_RS_30G8Working Group 2
G_RS_32G9G_RS_32G9Working Group 2
G_RS_33G10G_RS_33G10Working Group 2
G_RS_34G11G_RS_34G11Working Group 2
G_RS_35G12G_RS_35G12Working Group 2
GANYMEDE_FLYBY_RIME_AJSGanymede active radar opportunity, anti-jovian sideWorking Group 1
GANYMEDE_FLYBY_RIME_JSGanymede active radar opportunity, jovian sideWorking Group 1
GANYMEDE_FB_RSGanymede flyby remote sensingWorking Group 2
G_IS_3G3Ganymede in-situ observations around closest approachWorking Group 3
GANYMEDE_RPWI_PASSIVRADGanymede passive radar opportunity for RPWIWorking Group 1
GANYMEDE_IONOGANYMEDE_IONO In situ Ganymede ionosphere observationWorking Group 3
G_GPH_OBSGeneric G_GPH containing link to obs defWorking Group 1
G_RS_3G3HAA as per 3GM UM IS considering NIMWorking Group 2
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
CALLISTO_WAKEIn situ Callisto wake observationWorking Group 3
EUROPA_TOR_ISIn situ Europa torus observationWorking Group 3
EUROPA_WAKEIn situ Europa wake observationWorking Group 3
GANYMEDE_WAKEIn situ Ganymede wake observationWorking Group 3
JUPITER_CBIn situ Jupiter corotation breakdown region and plasma transport observation. Maximize the intervals for which co-rotation is measured to build spatial and temporal coverage of corotation profiles across the magnetosphere and also in the local moon environments.Working Group 3
JUPITER_CPSIn situ Jupiter current/plasma sheet observationWorking 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
GANYMEDE_GMIn situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environmentWorking 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_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking Group 3
JUPITER_FD_WOL_FBIn the last week before the fly-by a WOL slot shall be combined with the TCM slot at To– 3 days (i.e. a single 3-hr slot). Another 2-hour WOL slot shall be reserved at To + 12 hours.GENERIC
IO_ECLIPSEIo observation while Io is in eclipse.Working Group 2
IO_TOR_DUSTIo torus dustWorking Group 2
IO_MAJ_COMPOSITIONIO_MAJ_COMPOSITIONWorking Group 2
IO_MAJ_HOTSPOTSIO_MAJ_HOTSPOTSWorking Group 2
J_SAT_505_AmaJ_SAT_505_AmaWorking Group 2
J_SAT_514_TheJ_SAT_514_TheWorking Group 2
J_SAT_515_AdrJ_SAT_515_AdrWorking Group 2
J_SAT_516_MetJ_SAT_516_MetWorking Group 2
J_SAT_55507_3J23J_SAT_55507_3J23Working Group 2
J_SAT_OBSJ_SAT_OBSWorking Group 2
JA_PE_OBSJA_PE generic for link obs<-> segmentsWorking Group 4
JA_PE21JA_PE21Working Group 4
JA_PE25JA_PE25Working Group 4
JA_PE60JA_PE60Working Group 4
JA_PE61JA_PE61Working Group 4
JA_PE62JA_PE62Working Group 4
JA_PE63JA_PE63Working Group 4
JA_PE64JA_PE64Working Group 4
JA_PE65JA_PE65Working Group 4
JA_PE66JA_PE66Working Group 4
JA_PE67JA_PE67Working Group 4
JA_PE68JA_PE68Working Group 4
JA_PE69JA_PE69Working Group 4
JM_PE_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
JUPITER_PERIJOVEJupiter observationsWorking Group 4
J_SATjupiter satellite GENERICWorking Group 2
OPNAV_CALOPNAV_CALGENERIC
OPNAV_EUROPNAV_EURGENERIC
OPNAV_GANOPNAV_GANGENERIC
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_HPRing high phaseWorking Group 2
RING_LPRing low phaseWorking 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
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

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