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Group
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_IRR_SEARCHJ_SAT_IRR_SEARCH discover new irregular moonsWorking Group 2
J_SAT_572_11J1J_SAT_572_11J1Working Group 2
J_SAT_571_ErsJ_SAT_571_ErsWorking Group 2
J_SAT_570_17J9J_SAT_570_17J9Working Group 2
J_SAT_569_17J8J_SAT_569_17J8Working Group 2
J_SAT_568_17J7J_SAT_568_17J7Working Group 2
J_SAT_567_17J6J_SAT_567_17J6Working Group 2
J_SAT_566_17J5J_SAT_566_17J5Working Group 2
J_SAT_565_PdiJ_SAT_565_PdiWorking Group 2
J_SAT_564_17J3J_SAT_564_17J3Working Group 2
J_SAT_563_17J2J_SAT_563_17J2Working Group 2
J_SAT_562_ValJ_SAT_562_ValWorking Group 2
J_SAT_561_3J19J_SAT_561_3J19Working Group 2
J_SAT_560_EphJ_SAT_560_EphWorking Group 2
J_SAT_559_17J1J_SAT_559_17J1Working Group 2
J_SAT_558_PhiJ_SAT_558_PhiWorking Group 2
J_SAT_557_EirJ_SAT_557_EirWorking Group 2
J_SAT_556_11J2J_SAT_556_11J2Working Group 2
J_SAT_55508_3J24J_SAT_55508_3J24Working Group 2
J_SAT_55507_3J23J_SAT_55507_3J23Working Group 2
J_SAT_55506_3J16J_SAT_55506_3J16Working Group 2
J_SAT_55505_3J12J_SAT_55505_3J12Working Group 2
J_SAT_55504_3J10J_SAT_55504_3J10Working Group 2
J_SAT_55503_3J9J_SAT_55503_3J9Working Group 2
J_SAT_55502_3J4J_SAT_55502_3J4Working Group 2
J_SAT_55501_3J2J_SAT_55501_3J2Working Group 2
J_SAT_555_3J18J_SAT_555_3J18Working Group 2
J_SAT_554_16J1J_SAT_554_16J1Working Group 2
J_SAT_553_DiaJ_SAT_553_DiaWorking Group 2
J_SAT_552_10J2J_SAT_552_10J2Working Group 2
J_SAT_551_10J1J_SAT_551_10J1Working Group 2
J_SAT_550_HrsJ_SAT_550_HrsWorking Group 2
J_SAT_549_KorJ_SAT_549_KorWorking Group 2
J_SAT_548_CylJ_SAT_548_CylWorking Group 2
J_SAT_547_EukJ_SAT_547_EukWorking Group 2
J_SAT_546_CrpJ_SAT_546_CrpWorking Group 2
J_SAT_545_HlkJ_SAT_545_HlkWorking Group 2
J_SAT_544_KchJ_SAT_544_KchWorking Group 2
J_SAT_543_ArcJ_SAT_543_ArcWorking Group 2
J_SAT_542_TlxJ_SAT_542_TlxWorking Group 2
J_SAT_541_AoeJ_SAT_541_AoeWorking Group 2
J_SAT_540_MneJ_SAT_540_MneWorking Group 2
J_SAT_539_HegJ_SAT_539_HegWorking Group 2
J_SAT_538_PstJ_SAT_538_PstWorking Group 2
J_SAT_537_KleJ_SAT_537_KleWorking Group 2
J_SAT_536_SpoJ_SAT_536_SpoWorking Group 2
J_SAT_535_OrtJ_SAT_535_OrtWorking Group 2
J_SAT_534_EupJ_SAT_534_EupWorking Group 2
J_SAT_533_EuaJ_SAT_533_EuaWorking Group 2
J_SAT_532_EydJ_SAT_532_EydWorking Group 2
J_SAT_531_AitJ_SAT_531_AitWorking Group 2
J_SAT_530_HerJ_SAT_530_HerWorking Group 2
J_SAT_529_ThyJ_SAT_529_ThyWorking Group 2
J_SAT_528_AutJ_SAT_528_AutWorking Group 2
J_SAT_527_PraJ_SAT_527_PraWorking Group 2
J_SAT_526_IsoJ_SAT_526_IsoWorking Group 2
J_SAT_525_EriJ_SAT_525_EriWorking Group 2
J_SAT_524_IocJ_SAT_524_IocWorking Group 2
J_SAT_523_KlkJ_SAT_523_KlkWorking Group 2
J_SAT_522_HarJ_SAT_522_HarWorking Group 2
J_SAT_521_ChaJ_SAT_521_ChaWorking Group 2
J_SAT_520_TayJ_SAT_520_TayWorking Group 2
J_SAT_519_MegJ_SAT_519_MegWorking Group 2
J_SAT_518_ThmJ_SAT_518_ThmWorking Group 2
J_SAT_517_ClhJ_SAT_517_ClhWorking 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_513_LedJ_SAT_513_LedWorking Group 2
J_SAT_512_AnaJ_SAT_512_AnaWorking Group 2
J_SAT_511_CarJ_SAT_511_CarWorking Group 2
J_SAT_510_LysJ_SAT_510_LysWorking Group 2
J_SAT_509_SinJ_SAT_509_SinWorking Group 2
J_SAT_508_PasJ_SAT_508_PasWorking Group 2
J_SAT_507_ElaJ_SAT_507_ElaWorking Group 2
J_SAT_506_HimJ_SAT_506_HimWorking 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
JA_PE_JANUSIn-situ cloned from JA_PE Remote sensing: cloned from JA_PE removing MAJIS: JANUS: 55.5*76/(76-8*4)=33.62kbps SWI: 5.8 kbps UVS: 2.25 kbps total: 89.17 kbpsWorking Group 4
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

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