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JA_PE17work-around for segmentation schedulerWorking Group 4
JA_PE13work-aroudn for aegmentation schedulerWorking Group 4
JA_PE15work-aroudn for aegmentation schedulerWorking Group 4
JA_PE19work around for segmentation schedulerWorking Group 4
JA_PE23work around for segmentation schedulerWorking Group 4
JA_PE27work around for segmentation schedulerWorking Group 4
JA_PE29work around for segmentation schedulerWorking Group 4
JA_PE31work around for segmentation schedulerWorking Group 4
JA_PE33work around for segmentation schedulerWorking Group 4
JA_PE35work 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
ECLIPSESUN OCCULTATION BY JUPITER CONVERTED INTO ECLIPSE SEGMENTSGENERIC
STAR_OCC_OBSSTAR_OCC_OBSWorking Group 4
SUN_OCCSolar occultation by Jupiter, as seen from the SC.Working Group 4
JM_PE13share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE15share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE17share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE19share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE21share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE23share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE25share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE27share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE29share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE31share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE33share prime high lat PJ between WG3 and WG4Working Group 3
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
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_LPRing low phaseWorking Group 2
RING_HPRing high phaseWorking Group 2
3GM_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.3GM
GALA_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.GALA
GALA_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.GALA
JANUS_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.JANUS
JANUS_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.JANUS
JMAG_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.JMAG
JMAG_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.JMAG
MAJIS_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.MAJIS
MAJIS_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.MAJIS
NAVCAM_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.NAVCAM
NAVCAM_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.NAVCAM
PEP_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.PEP
PEP_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.PEP
RADEM_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RADEM
RPWI_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RPWI
RPWI_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RPWI
SWI_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.SWI
UVS_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.UVS
UVS_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.UVS
SOC_PRIME_OBSERVATIONPlaceholder for SOC Prime ObservationSOC
JUICE_PRIME_OBSERVATIONPlaceholder for JUICE SOC Observations.JUICE
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_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
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_CPIn 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. CP stands for corotation profileWorking 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_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

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