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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_508_PasJ_SAT_508_PasWorking Group 2
J_SAT_507_ElaJ_SAT_507_ElaWorking Group 2
J_SAT_505_AmaJ_SAT_505_AmaWorking Group 2
J_SATjupiter satellite GENERICWorking Group 2
J_RING Working Group 2
IO_TOR_DUSTIo torus dustWorking Group 2
IO_RS 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
IO_MAJ_HOTSPOTSIO_MAJ_HOTSPOTSWorking Group 2
IO_MAJ_COMPOSITIONIO_MAJ_COMPOSITIONWorking Group 2
IO_ECLIPSEIo observation while Io is in eclipse.Working Group 2
HIGHPHPROFILErings high phase profile (JANUS DEF)Working Group 2
GANYMEDE_FB_RSGanymede flyby remote sensingWorking Group 2
GANYMEDE_DISTANT Working Group 2
G_RS_OBSG_RS GENERICWorking Group 2
G_RS_5G5 Working Group 2
G_RS_4G4 Working Group 2
G_RS_3G3HAA as per 3GM UM IS considering NIMWorking Group 2
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_2G2 Working Group 2
G_RS_27G7G_RS_27G7Working Group 2
G_RS_26G6G_RS_26G6Working Group 2
G_RS_1G1 Working Group 2
G_distant Working Group 2
EUROPA_FB_RSEuropa Flyby remote sensingWorking Group 2
EUROPA_DISTANT Working Group 2
E_RS_OBSEuropa remote sensing generic segment containing obs database linkWorking Group 2
E_RS_8E2E_RS_8E2Working Group 2
E_RS_7E1E_RS_7E1Working Group 2
E_RS Working Group 2
E_distant Working Group 2
CHARACTERIZATION_IRR2_SINOPECharacterization irregular moon SinopeWorking Group 2
CHARACTERIZATION_IRR2_PASIPHAEcharacterization irregular moon PasiphaeWorking Group 2
CHARACTERIZATION_IRR2_CARME Working Group 2
CHARACTERIZATION_IRR2_ANANKECharacterization irregular moon ANANKEWorking Group 2
CHARACTERIZATION_IRR_ELARACharacterization irregular moon ElaraWorking Group 2
CHAR_IRR1Characterization irregular moons group 1 (see list below)Working Group 2
CALLISTO_FB_RSCallisto Flyby remote sensingWorking Group 2
CALLISTO_DISTANT Working Group 2
C_RS_OBSCallisto Remote sensing GENERIC containing obs database linkWorking Group 2
C_RS_9C2C_RS_9C2Working Group 2
C_RS_6C1C_RS_6C1Working Group 2
C_RS_31C21C_RS_31C21Working Group 2
C_RS_29C20C_RS_29C20Working Group 2
C_RS_28C19C_RS_28C19Working Group 2
C_RS_25C18C_RS_25C18Working Group 2
C_RS_24C17C_RS_24C17Working Group 2
C_RS_23C16C_RS_23C16Working Group 2
C_RS_22C15C_RS_22C15Working Group 2
C_RS_21C14C_RS_21C14Working Group 2
C_RS_20C13C_RS_20C13Working Group 2
C_RS_19C12C_RS_19C12Working Group 2
C_RS_18C11C_RS_18C11Working Group 2
C_RS_17C10C_RS_17C10Working Group 2
C_RS_16C9C_RS_16C9Working Group 2
C_RS_15C8C_RS_15C8Working Group 2
C_RS_14C7C_RS_14C7Working Group 2
C_RS_13C6C_RS_13C6Working Group 2
C_RS_12C5C_RS_12C5Working Group 2
C_RS_11C4C_RS_11C4Working Group 2
C_RS_10C3C_RS_10C3Working Group 2
C_distant Working Group 2
ASTRO_IRR2_SINOPE Working Group 2
ASTRO_IRR2_PASIPHAEastrometry measurement with inertial pointing to moon PasiphaeWorking Group 2
ASTRO_IRR2_CARMEAstrometry irregular moon CarmeWorking Group 2
ASTRO_IRR2_ANANKEAstrometry irregular moon AnankeWorking Group 2
ASTRO_IRR1_THEMISTOAstrometry irregular moon THEMISTOWorking Group 2
ASTRO_IRR1_TAYGETEAstrometry irregular moon TAYGETEWorking Group 2
ASTRO_IRR1_MEGACLITEASTRO_IRR1_MEGACLITEWorking Group 2
ASTRO_IRR1_LYSITHEAAstrometry irregular moon LYSITHEAWorking Group 2
ASTRO_IRR1_LEDAAstrometry irregular moon LEDAWorking Group 2
ASTRO_IRR1_KALLICHOREAstrometry irregular moon KALLICHOREWorking Group 2
ASTRO_IRR1_HIMALIAAstrometry irregular moon HIMALIAWorking Group 2
ASTRO_IRR1_CHALDENEAstrometry irregular moon CHALDENEWorking Group 2
ASTRO_IRR1_CARPOAstrometry irregular moon CARPOWorking Group 2
ASTRO_IRR_ELARA Working Group 2
ASTRO_INNERAstrometry inner moonsWorking Group 2
TOR_RS Working Group 3
JUPITER_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking 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_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_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
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
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
JM_PE35 Working 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

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