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Group
JUPITER_PHASE_MAX Working Group 4
JUPITER_PHASE_MIN Working Group 4
PERIJOVE_DAYSIDE Working Group 4
PERIJOVE_NIGHTSIDE Working Group 4
PERIJOVE_TERMINATOR Working Group 4
STAR_OCC Working Group 4
STAR_OCC_OBSSTAR_OCC_OBSWorking Group 4
SUN_OCCSolar occultation by Jupiter, as seen from the SC.Working Group 4
C_IS Working Group 3
C_IS_OBSC_IS_OBSWorking Group 3
CALLISTO_ENAFar approach energetic neutral atom imaging of CallistoWorking Group 3
CALLISTO_FLYBY_RPWI_IONO_AJS Working Group 3
CALLISTO_IONOCALLISTO_IONO In situ Callisto ionosphere observationWorking Group 3
CALLISTO_WAKEIn situ Callisto wake observationWorking Group 3
E_IS Working Group 3
E_IS_OBSE_IS_OBSWorking Group 3
EUROPA_ENAFar approach energetic neutral atom imaging of EuropaWorking Group 3
EUROPA_FLYBY_RPWI_IONO_AJS Working Group 3
EUROPA_IONO_ISEUROPA_IONO_IS In situ Europa ionosphere observationWorking Group 3
EUROPA_TOR_ISIn situ Europa torus observationWorking Group 3
EUROPA_WAKEIn situ Europa wake observationWorking Group 3
G_IS Working Group 3
G_IS_3G3Ganymede in-situ observations around closest approachWorking Group 3
G_IS_OBSG_IS_OBSWorking Group 3
GANYMEDE_ENAFar approach energetic neutral atom imaging of GanymedeWorking Group 3
GANYMEDE_FLYBY_RPWI_IONO_AJS Working Group 3
GANYMEDE_GMIn situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environmentWorking Group 3
GANYMEDE_IONOGANYMEDE_IONO In situ Ganymede ionosphere observationWorking Group 3
GANYMEDE_WAKEIn situ Ganymede wake observationWorking Group 3
JM_CB Working Group 3
JM_ENA Working Group 3
JM_GMJupiter Magnetosphere global monitoring. Large pointing flexibility, constraints mainly driven by PEPWorking Group 3
JM_INCL Working Group 3
JM_PE_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
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
JM_PE35 Working 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_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_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_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
JUPITER_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking Group 3
TOR_RS Working Group 3
ASTRO_INNERAstrometry inner moonsWorking Group 2
ASTRO_IRR_ELARA Working Group 2
ASTRO_IRR1_CARPOAstrometry irregular moon CARPOWorking Group 2
ASTRO_IRR1_CHALDENEAstrometry irregular moon CHALDENEWorking Group 2
ASTRO_IRR1_HIMALIAAstrometry irregular moon HIMALIAWorking Group 2
ASTRO_IRR1_KALLICHOREAstrometry irregular moon KALLICHOREWorking Group 2
ASTRO_IRR1_LEDAAstrometry irregular moon LEDAWorking Group 2
ASTRO_IRR1_LYSITHEAAstrometry irregular moon LYSITHEAWorking Group 2
ASTRO_IRR1_MEGACLITEASTRO_IRR1_MEGACLITEWorking Group 2
ASTRO_IRR1_TAYGETEAstrometry irregular moon TAYGETEWorking Group 2
ASTRO_IRR1_THEMISTOAstrometry irregular moon THEMISTOWorking Group 2
ASTRO_IRR2_ANANKEAstrometry irregular moon AnankeWorking Group 2
ASTRO_IRR2_CARMEAstrometry irregular moon CarmeWorking Group 2
ASTRO_IRR2_PASIPHAEastrometry measurement with inertial pointing to moon PasiphaeWorking Group 2
ASTRO_IRR2_SINOPE Working Group 2
C_distant 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_16C9: Prime surface and exosphere segment defined as 24 hours centered at CA. WG1 (gravity) is rider. Pointing is mainly surface and/or limb (details TBD)Working 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_28C19C_RS_28C19Working Group 2
C_RS_29C20C_RS_29C20Working Group 2
C_RS_31C21C_RS_31C21Working Group 2
C_RS_6C1C_RS_6C1Working Group 2
C_RS_9C2C_RS_9C2Working Group 2
C_RS_OBSCallisto Remote sensing GENERIC containing obs database linkWorking Group 2
CALLISTO_DISTANT Working Group 2
CALLISTO_FB_RSCallisto Flyby remote sensingWorking Group 2
CHAR_IRR1Characterization irregular moons group 1 (see list below)Working Group 2
CHARACTERIZATION_IRR_ELARACharacterization irregular moon ElaraWorking Group 2
CHARACTERIZATION_IRR2_ANANKECharacterization irregular moon ANANKEWorking Group 2
CHARACTERIZATION_IRR2_CARME Working Group 2
CHARACTERIZATION_IRR2_PASIPHAEcharacterization irregular moon PasiphaeWorking Group 2
CHARACTERIZATION_IRR2_SINOPECharacterization irregular moon SinopeWorking Group 2

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