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JA_PE17work-around for segmentation schedulerWorking Group 4
JA_PE15work-aroudn for aegmentation schedulerWorking Group 4
JA_PE13work-aroudn for aegmentation schedulerWorking Group 4
JA_PE35work around for segmentation schedulerWorking Group 4
JA_PE33work around for segmentation schedulerWorking Group 4
JA_PE31work around for segmentation schedulerWorking Group 4
JA_PE29work around for segmentation schedulerWorking Group 4
JA_PE27work around for segmentation schedulerWorking Group 4
JA_PE23work around for segmentation schedulerWorking Group 4
JA_PE19work around for segmentation schedulerWorking Group 4
EUR_CAL_GAN_TRANSIT_PRTriple transit in front of JupiterWGX
G_GPH_1G1test 3_2Working Group 1
JA_PE1test 3_2Working Group 4
STAR_OCC_OBSSTAR_OCC_OBSWorking Group 4
SUN_OCCSolar occultation by Jupiter, as seen from the SC.Working Group 4
SHT_TESTSHT_TESTGENERIC
JM_PE33share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE31share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE29share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE27share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE25share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE23share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE21share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE19share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE17share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE15share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE13share prime high lat PJ between WG3 and WG4Working Group 3
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
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
HIGHPHPROFILErings high phase profile (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_LPRing low phaseWorking Group 2
RING_HPRing high phaseWorking 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_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
OPNAV_GANOPNAV_GANGENERIC
OPNAV_EUROPNAV_EURGENERIC
OPNAV_CALOPNAV_CALGENERIC
J_SATjupiter satellite GENERICWorking Group 2
JUPITER_PERIJOVEJupiter observationsWorking Group 4
JM_PE_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
JA_PE69JA_PE69Working Group 4
JA_PE68JA_PE68Working Group 4
JA_PE67JA_PE67Working Group 4
JA_PE66JA_PE66Working Group 4
JA_PE65JA_PE65Working Group 4
JA_PE64JA_PE64Working Group 4
JA_PE63JA_PE63Working Group 4
JA_PE62JA_PE62Working Group 4
JA_PE61JA_PE61Working Group 4
JA_PE60JA_PE60Working Group 4
JA_PE25JA_PE25Working Group 4
JA_PE21JA_PE21Working Group 4
JA_PE_OBSJA_PE generic for link obs<-> segmentsWorking Group 4
J_SAT_OBSJ_SAT_OBSWorking 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
IO_MAJ_HOTSPOTSIO_MAJ_HOTSPOTSWorking Group 2
IO_MAJ_COMPOSITIONIO_MAJ_COMPOSITIONWorking Group 2
IO_TOR_DUSTIo torus dustWorking Group 2
IO_ECLIPSEIo observation while Io is in eclipse.Working Group 2
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
JUPITER_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking 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
GANYMEDE_GMIn situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environmentWorking 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_NULLIn situ Jupiter magnetic null searchWorking Group 3
JUPITER_CPSIn situ Jupiter current/plasma sheet 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
GANYMEDE_WAKEIn situ Ganymede wake observationWorking Group 3
EUROPA_WAKEIn situ Europa wake observationWorking Group 3
EUROPA_TOR_ISIn situ Europa torus observationWorking Group 3
CALLISTO_WAKEIn situ Callisto wake 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
G_RS_3G3HAA as per 3GM UM IS considering NIMWorking Group 2
G_GPH_OBSGeneric G_GPH containing link to obs defWorking Group 1
GANYMEDE_IONOGANYMEDE_IONO In situ Ganymede ionosphere observationWorking Group 3
GANYMEDE_RPWI_PASSIVRADGanymede passive radar opportunity for RPWIWorking Group 1
G_IS_3G3Ganymede in-situ observations around closest approachWorking Group 3
GANYMEDE_FB_RSGanymede flyby remote sensingWorking Group 2
GANYMEDE_FLYBY_RIME_JSGanymede active radar opportunity, jovian sideWorking Group 1
GANYMEDE_FLYBY_RIME_AJSGanymede active radar opportunity, anti-jovian sideWorking Group 1
G_RS_35G12G_RS_35G12Working Group 2
G_RS_34G11G_RS_34G11Working Group 2
G_RS_33G10G_RS_33G10Working Group 2
G_RS_32G9G_RS_32G9Working Group 2
G_RS_30G8G_RS_30G8Working Group 2
G_RS_27G7G_RS_27G7Working Group 2
G_RS_26G6G_RS_26G6Working Group 2
G_RS_OBSG_RS GENERICWorking Group 2
G_IS_OBSG_IS_OBSWorking Group 3
G_GPH_5G5G_GPH_5G5Working Group 1
G_GPH_3G3G_GPH_3G3Working Group 1
G_GPH_26G6G_GPH_26G6Working Group 1
JUPITER_FD_WOLFlight dynamics wheel off-loading slot, outside of Flyby preparation and recuperationGENERIC
FB_THERMALFB_THERMALGENERIC

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