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Mnemonic
Description
Group
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_27G6G_GPH_27G6Working 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_27G6G_RS_27G6Working Group 2
G_RS_27G7G_RS_27G7Working Group 2
G_RS_28G7G_RS_28G7Working Group 2
G_RS_30G8G_RS_30G8Working Group 2
G_RS_32G8G_RS_32G8Working 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_34G9G_RS_34G9Working Group 2
G_RS_35G10G_RS_35G10Working Group 2
G_RS_35G12G_RS_35G12Working Group 2
G_RS_36G11G_RS_36G11Working 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_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
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
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
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_506_HimJ_SAT_506_HimWorking Group 2
J_SAT_507_ElaJ_SAT_507_ElaWorking Group 2
J_SAT_508_PasJ_SAT_508_PasWorking Group 2
J_SAT_509_SinJ_SAT_509_SinWorking Group 2
J_SAT_510_LysJ_SAT_510_LysWorking Group 2
J_SAT_511_CarJ_SAT_511_CarWorking Group 2
J_SAT_512_AnaJ_SAT_512_AnaWorking Group 2
J_SAT_513_LedJ_SAT_513_LedWorking 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_517_ClhJ_SAT_517_ClhWorking Group 2
J_SAT_518_ThmJ_SAT_518_ThmWorking Group 2
J_SAT_519_MegJ_SAT_519_MegWorking Group 2
J_SAT_520_TayJ_SAT_520_TayWorking Group 2
J_SAT_521_ChaJ_SAT_521_ChaWorking Group 2
J_SAT_522_HarJ_SAT_522_HarWorking Group 2
J_SAT_523_KlkJ_SAT_523_KlkWorking Group 2
J_SAT_524_IocJ_SAT_524_IocWorking Group 2
J_SAT_525_EriJ_SAT_525_EriWorking Group 2
J_SAT_526_IsoJ_SAT_526_IsoWorking Group 2
J_SAT_527_PraJ_SAT_527_PraWorking Group 2
J_SAT_528_AutJ_SAT_528_AutWorking Group 2
J_SAT_529_ThyJ_SAT_529_ThyWorking Group 2
J_SAT_530_HerJ_SAT_530_HerWorking Group 2
J_SAT_531_AitJ_SAT_531_AitWorking Group 2
J_SAT_532_EydJ_SAT_532_EydWorking Group 2
J_SAT_533_EuaJ_SAT_533_EuaWorking Group 2
J_SAT_534_EupJ_SAT_534_EupWorking Group 2
J_SAT_535_OrtJ_SAT_535_OrtWorking Group 2
J_SAT_536_SpoJ_SAT_536_SpoWorking Group 2
J_SAT_537_KleJ_SAT_537_KleWorking Group 2
J_SAT_538_PstJ_SAT_538_PstWorking Group 2
J_SAT_539_HegJ_SAT_539_HegWorking Group 2
J_SAT_540_MneJ_SAT_540_MneWorking Group 2
J_SAT_541_AoeJ_SAT_541_AoeWorking Group 2
J_SAT_542_TlxJ_SAT_542_TlxWorking Group 2
J_SAT_543_ArcJ_SAT_543_ArcWorking Group 2
J_SAT_544_KchJ_SAT_544_KchWorking Group 2
J_SAT_545_HlkJ_SAT_545_HlkWorking Group 2
J_SAT_546_CrpJ_SAT_546_CrpWorking Group 2
J_SAT_547_EukJ_SAT_547_EukWorking Group 2
J_SAT_548_CylJ_SAT_548_CylWorking Group 2
J_SAT_549_KorJ_SAT_549_KorWorking Group 2
J_SAT_550_HrsJ_SAT_550_HrsWorking Group 2
J_SAT_551_10J1J_SAT_551_10J1Working Group 2
J_SAT_552_10J2J_SAT_552_10J2Working Group 2
J_SAT_553_DiaJ_SAT_553_DiaWorking Group 2
J_SAT_554_16J1J_SAT_554_16J1Working Group 2
J_SAT_555_3J18J_SAT_555_3J18Working Group 2

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