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Group
G_IS_OBSG_IS_OBSWorking Group 3
G_IS_3G3Ganymede in-situ observations around closest approachWorking Group 3
GANYMEDE_IONOGANYMEDE_IONO In situ Ganymede ionosphere 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
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
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
ASTRO_IRR_ELARA Working Group 2
ASTRO_IRR2_SINOPE Working Group 2
C_distant Working Group 2
CALLISTO_DISTANT Working Group 2
CHARACTERIZATION_IRR2_CARME Working Group 2
E_distant Working Group 2
E_RS Working Group 2
EUROPA_DISTANT Working Group 2
G_distant Working Group 2
G_RS_1G1 Working Group 2
G_RS_2G2 Working Group 2
G_RS_4G4 Working Group 2
G_RS_5G5 Working Group 2
GANYMEDE_DISTANT Working Group 2
IO_RS Working Group 2
J_RING Working Group 2
J_SAT_AITNE Working Group 2
J_SAT_ANANKE Working Group 2
J_SAT_AOEDE Working Group 2
J_SAT_ARCHE Working Group 2
J_SAT_AUTONOE Working Group 2
J_SAT_CARME Working Group 2
J_SAT_CARPO Working Group 2
J_SAT_DIA Working Group 2
J_SAT_EIRENE Working Group 2
J_SAT_ELARA Working Group 2
J_SAT_ERINOME Working Group 2
J_SAT_ERSA Working Group 2
J_SAT_EUKELADE Working Group 2
J_SAT_EUPHEME Working Group 2
J_SAT_EUPORIE Working Group 2
J_SAT_HARPALYKE Working Group 2
J_SAT_HEGEMONE Working Group 2
J_SAT_HELIKE Working Group 2
J_SAT_HERMIPPE Working Group 2
J_SAT_HERSE Working Group 2
J_SAT_HIMALIA Working Group 2
J_SAT_INN_AST_A Working Group 2
J_SAT_INN_AST_T Working Group 2
J_SAT_INN_CHAR_A Working Group 2
J_SAT_IOCASTE Working Group 2
J_SAT_IRR_AST_E Working Group 2
J_SAT_IRR_CHAR_E Working Group 2
J_SAT_ISONOE Working Group 2
J_SAT_KALE Working Group 2
J_SAT_KALLICHORE Working Group 2
J_SAT_KALYKE Working Group 2
J_SAT_LEDA Working Group 2
J_SAT_LYSITHEA Working Group 2
J_SAT_MEGACLITE Working Group 2
J_SAT_MNEME Working Group 2
J_SAT_ORTHOSIE Working Group 2
J_SAT_PANDIA Working Group 2
J_SAT_PASIPHAE Working Group 2
J_SAT_PASITHEE Working Group 2
J_SAT_PHILOPHROSYNE Working Group 2
J_SAT_S2003_J12 Working Group 2
J_SAT_S2003_J16 Working Group 2
J_SAT_S2003_J19 Working Group 2
J_SAT_S2003_J4 Working Group 2
J_SAT_S2003_J9 Working Group 2
J_SAT_S2010_J1 Working Group 2
J_SAT_S2010_J2 Working Group 2
J_SAT_S2011_J2 Working Group 2
J_SAT_S2016_J1 Working Group 2
J_SAT_S2017_J2 Working Group 2
J_SAT_S2017_J5 Working Group 2
J_SAT_S2017_J6 Working Group 2
J_SAT_S2017_J7 Working Group 2
J_SAT_S2017_J9 Working Group 2
J_SAT_SINOPE Working Group 2
J_SAT_TAYGETE Working Group 2

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