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Group
G_RS_25G10 Working Group 2
G_RS_24G9 Working Group 2
G_RS_24G10test 3_2Working Group 2
G_RS_23G8 Working Group 2
G_RS_22G7 Working Group 2
G_RS_21G9test 3_2Working Group 2
G_RS_20G8test 3_2Working Group 2
G_RS_1G1 Working Group 2
G_RS_19G7test 3_2Working Group 2
G_RS_18G6 Working Group 2
G_RS_17G5 Working Group 2
G_distant Working Group 2
FB_RS Working Group 2
EUROPA_FLYBY_WG2 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_7E2 Working Group 2
E_RS_6E1 Working 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_FLYBY_WG2 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_9C3 Working Group 2
C_RS_8C2 Working Group 2
C_RS_8C1test 3_2Working Group 2
C_RS_5C1 Working Group 2
C_RS_23C12test 3_2Working Group 2
C_RS_22C11test 3_2Working Group 2
C_RS_21C13 Working Group 2
C_RS_20C12 Working Group 2
C_RS_19C11 Working Group 2
C_RS_18C10test 3_2Working Group 2
C_RS_17C9test 3_2Working Group 2
C_RS_16C8test 3_2Working Group 2
C_RS_16C10 Working Group 2
C_RS_15C9 Working Group 2
C_RS_15C7test 3_2Working Group 2
C_RS_14C8 Working Group 2
C_RS_14C6test 3_2Working Group 2
C_RS_13C7 Working Group 2
C_RS_13C5test 3_2Working Group 2
C_RS_12C6 Working Group 2
C_RS_12C4test 3_2Working Group 2
C_RS_11C5 Working Group 2
C_RS_11C3test 3_2Working Group 2
C_RS_10C4 Working Group 2
C_RS_10C2test 3_2Working Group 2
C_RS Working 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_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_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
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
JM_PE_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
JM_PEassuming: JMAG: 2.31 kbps RPWI: 1.7*2.167 kbps PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018)Working Group 3
JM_INCL Working Group 3
JM_GM Working Group 3
JM_ENA Working Group 3
JM_CB Working Group 3
GANYMEDE_WAKEIn situ Ganymede wake observationWorking Group 3
GANYMEDE_IONOGANYMEDE_IONO In situ Ganymede ionosphere observationWorking Group 3

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