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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_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
JM_PE_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
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
RINGPHASE Working Group 2
C_RS_30C21 Working Group 2
C_RS_26C19 Working Group 2
G_RS_1G1 Working Group 2
G_RS_5G5 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_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_40 Working Group 2
RING_PHASECURV_30 Working Group 2
RING_PHASECURV_20 Working Group 2
EUROPA_DISTANT Working Group 2
G_RS_4G4 Working Group 2
G_RS_2G2 Working Group 2
IO_RS Working Group 2
J_RING Working Group 2
G_distant Working Group 2
E_RS Working Group 2
E_distant Working Group 2
C_distant Working Group 2
CALLISTO_DISTANT Working Group 2
GANYMEDE_DISTANT Working Group 2
IO_MONITORING- JANUS minimum distance = 7.00e+05 km - MAJIS minimum distance = 8.00e+05 km - SWI minimum distance = 6.00e+05 km (able to resolve target when angular size is > 1 mrad) Working Group 2
C_RS_10C3C_RS_10C3Working Group 2
C_RS_11C4C_RS_11C4Working Group 2
C_RS_12C5C_RS_12C5Working Group 2
C_RS_13C6C_RS_13C6Working Group 2
C_RS_14C7C_RS_14C7Working Group 2
C_RS_15C8C_RS_15C8Working Group 2
C_RS_16C9C_RS_16C9Working Group 2
C_RS_17C10C_RS_17C10Working Group 2
C_RS_18C11C_RS_18C11Working Group 2
C_RS_19C12C_RS_19C12Working Group 2
C_RS_20C13C_RS_20C13Working Group 2
C_RS_21C14C_RS_21C14Working Group 2
C_RS_22C15C_RS_22C15Working Group 2
C_RS_23C16C_RS_23C16Working Group 2
C_RS_24C17C_RS_24C17Working Group 2
C_RS_25C18C_RS_25C18Working Group 2
C_RS_29C20C_RS_29C20Working Group 2
C_RS_31C22C_RS_31C22Working Group 2
C_RS_33C23C_RS_33C23Working Group 2
C_RS_6C1C_RS_6C1Working Group 2
C_RS_9C2C_RS_9C2Working Group 2
CALLISTO_FB_RSCallisto Flyby remote sensingWorking Group 2
C_RS_OBSCallisto Remote sensing GENERIC containing obs database linkWorking Group 2
E_RS_7E1E_RS_7E1Working Group 2
E_RS_8E2E_RS_8E2Working Group 2
EUROPA_FB_RSEuropa Flyby remote sensingWorking Group 2
E_RS_OBSEuropa remote sensing generic segment containing obs database linkWorking Group 2
G_RS_OBSG_RS GENERICWorking Group 2
G_RS_27G6G_RS_27G6Working Group 2
G_RS_28G7G_RS_28G7Working Group 2
G_RS_32G8G_RS_32G8Working Group 2
G_RS_34G9G_RS_34G9Working Group 2
G_RS_35G10G_RS_35G10Working Group 2
G_RS_36G11G_RS_36G11Working Group 2
GANYMEDE_FB_RSGanymede flyby remote sensingWorking Group 2
G_RS_3G3HAA as per 3GM UM IS considering NIMWorking Group 2
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_SATjupiter satellite GENERICWorking 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_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_HPRing high phaseWorking Group 2
RING_LPRing low phaseWorking Group 2

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