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UVS_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.UVS
UVS_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.UVS
TRANSIT_ETEvent tool support segment definitionGENERIC
TRAJECTORY_SEGMENTdefined segment for moon coverage tool export functionnalityGENERIC
TOR_RS Working Group 3
SWI_PRIME_OBSERVATION SWI
SWI_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.SWI
SUN_OCC_ETEvent tool support segment definitionGENERIC
SUN_OCCSolar occultation by Jupiter, as seen from the SC.Working Group 4
STELLAR_OCC_ETEvent tool support segment definitionGENERIC
STAR_OCC_OBSSTAR_OCC_OBSWorking Group 4
STAR_OCC Working Group 4
SPICE_ATT_TRANSFER_HOTDefault attitude during cruise phase applicable during the hot phasesGENERIC
SPICE_ATT_TRANSFER_COLDDefault attitude during cruise phaseGENERIC
SPICE_ATT_JUPITER_TOURDefault attitude during the Tour phaseGENERIC
SPICE_ATT_GOTOTRANSFER_COLD_SUP_SOL_CONJDefault attitude during cruise phase superior solar conjunctions 'cold'GENERIC
SPICE_ATT_GOTOMARS_NPO GENERIC
SPICE_ATT_GOTOMARS_NOA_HOT GENERIC
SPICE_ATT_GOTOJUPITER_TOUR_SUP_SOL_CONJDefault attitude during superior solar conjunctionGENERIC
SPICE_ATT_GOTOGANYMEDE_PHASE_SUP_SOL_CONJ GENERIC
SPICE_ATT_GOTOGANYMEDE_NPO GENERIC
SPICE_ATT_GOTOGANYMEDE_NOA_HOT GENERIC
SPICE_ATT_GOTOGANYMEDE_NOA GENERIC
SPICE_ATT_GOTOEUROPA_NPO GENERIC
SPICE_ATT_GOTOEUROPA_NOA_HOT GENERIC
SPICE_ATT_GOTOEUROPA_NOA GENERIC
SPICE_ATT_GOTOEARTH_NPO GENERIC
SPICE_ATT_GOTOEARTH_NOA_HOT GENERIC
SPICE_ATT_GOTOEARTH_NOA GENERIC
SPICE_ATT_GOTOEARTH_COMMSEarth communication segmentGENERIC
SPICE_ATT_GOTOCALLISTO_NPO GENERIC
SPICE_ATT_GOTOCALLISTO_NOA_HOT GENERIC
SPICE_ATT_GOTOCALLISTO_NOA GENERIC
SPICE_ATT_GANYMEDE_PHASEDefault attitude during the Ganymede phaseGENERIC
SOC_PRIME_OBSERVATIONPlaceholder for SOC Prime ObservationSOC
SOC_OBSERVATION SOC
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
RPWI_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RPWI
RPWI_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RPWI
RINGSPIRAL_MPRINGSPIRAL_MP (medium phase: JANUS Def)Working Group 2
RINGSPIRAL_HPRINGSPIRAL_HP (high phase, Janus def)Working Group 2
RINGPHASE Working Group 2
RINGMOSAICRINGMOSAIC (Janus definition). impression of the extent of the whole ring systemWorking 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
RIME_PRIME_OBSERVATION RIME
RECOVERY_FLYBY20.5 hour recovery segments to be scheduled flybys Duration is derived from https://issues.cosmos.esa.int/juicewiki/display/SOCDEV/Downlink%2C+Recovery%2C+and+Eclipse+Scenario+AnalysisGENERIC
RECOVERY GENERIC
RADEM_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RADEM
PR WGX
PERIJOVE_TERMINATOR Working Group 4
PERIJOVE_NIGHTSIDE Working Group 4
PERIJOVE_DAYSIDE Working Group 4
PEP_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.PEP
PEP_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.PEP
OPNAV_GANOPNAV_GANGENERIC
OPNAV_EUROPNAV_EURGENERIC
OPNAV_CALOPNAV_CALGENERIC
NAVCAM_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.NAVCAM
NAVCAM_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.NAVCAM
MAJIS_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.MAJIS
MAJIS_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.MAJIS
JUPITER_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking Group 3
JUPITER_PHASE_MIN Working Group 4
JUPITER_PHASE_MAX Working Group 4
JUPITER_PHASE_165_INC Working Group 4
JUPITER_PHASE_165_DEC Working Group 4
JUPITER_PHASE_150_INC Working Group 4
JUPITER_PHASE_150_DEC Working Group 4
JUPITER_PHASE_135_INC Working Group 4
JUPITER_PHASE_135_DEC Working Group 4
JUPITER_PHASE_120_INC Working Group 4
JUPITER_PHASE_120_DEC Working Group 4
JUPITER_PHASE_090 Working Group 4
JUPITER_PERIJOVEJupiter observationsWorking Group 4
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_NULLIn situ Jupiter magnetic null searchWorking Group 3
JUPITER_MONITORING Working Group 4
JUPITER_INCLINED_AURORA Working Group 4
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_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

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