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JA_PE20 Working Group 4
JM_PE19share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE18 Working Group 4
JM_PE17share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE16 Working Group 4
JM_PE15share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE14 Working Group 4
JM_PE13share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE12 Working Group 4
JA_PE11 Working Group 4
JA_PE10 Working Group 4
JA_PE9 Working Group 4
JA_PE8 Working Group 4
JA_PE7 Working Group 4
JA_PE6 Working Group 4
JA_PE5 Working Group 4
JA_PE4 Working Group 4
JA_PE3 Working Group 4
JA_PE2 Working Group 4
G_RS_4G4 Working Group 2
G_RS_3G3HAA as per 3GM UM IS considering NIMWorking Group 2
G_RS_2G2 Working Group 2
ASTRO_INNERAstrometry inner moonsWorking Group 2
CHAR_IRR1Characterization irregular moons group 1 (see list below)Working Group 2
J_AURORA Working Group 4
IO_RS Working Group 2
TOR_RS Working Group 3
J_RING Working Group 2
PR WGX
EUROPA_FB_RSEuropa Flyby remote sensingWorking Group 2
CALLISTO_FB_RSCallisto Flyby remote sensingWorking Group 2
GANYMEDE_FB_RSGanymede flyby remote sensingWorking Group 2
JMAG_CALROLL5 calibration roll needed by JMAG. 2 as soon as possible after JOI. 3 during phase 5: one at the start of phase 5, the last 2 as late as possible before GOIWGX
JM_INCL Working Group 3
DL_EXTassuming: 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)GENERIC
DL_assuming: JMAG: 2.31 kbps RPWI: 1.7*2.167 kbps (Ballparks numbers from the team) PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018)GENERIC
CAL WGX
JM_CB Working Group 3
JM_ENA Working Group 3
JM_GM Working Group 3
JA_PH Working Group 4
JA_M Working Group 4
JA_INCL Working Group 4
G_IS Working Group 3
G_distant Working Group 2
E_RS Working Group 2
E_IS Working Group 3
E_GPH Working Group 1
E_distant Working Group 2
C_IS Working Group 3
C_distant Working Group 2
GAN_EUR_TRANSIT_PRDouble transit in front of Jupiter (Europa, Ganymede)WGX
CALLISTO_FLYBY Working Group 1
CALLISTO_FLYBY_3GM Working Group 1
CALLISTO_FLYBY_GALA Working Group 1
CALLISTO_FLYBY_JANUS Working Group 1
CALLISTO_FLYBY_MAJIS Working Group 1
CALLISTO_FLYBY_RIME_AJSCallisto active radar opportunity, anti-jovian sideWorking Group 1
CALLISTO_FLYBY_RIME_JSCallisto active radar opportunity, jovian sideWorking Group 1
CALLISTO_RPWI_PASSIVRADCallisto passive radar opportunity for RPWIWorking Group 1
EUROPA_FLYBY Working Group 1
EUROPA_FLYBY_3GM Working Group 1
EUROPA_FLYBY_GALA Working Group 1
EUROPA_FLYBY_JANUS Working Group 1
EUROPA_FLYBY_MAJIS Working Group 1
EUROPA_FLYBY_RIME_JSEuropa active radar opportunity, jovian sideWorking Group 1
EUROPA_RPWI_PASSIVRADEuropa passive radar opportunity for RPWIWorking Group 1
GANYMEDE_FLYBY Working Group 1
GANYMEDE_FLYBY_3GM Working Group 1
GANYMEDE_FLYBY_GALA Working Group 1
GANYMEDE_FLYBY_JANUS Working Group 1
GANYMEDE_FLYBY_MAJIS Working Group 1
GANYMEDE_FLYBY_RIME_AJSGanymede active radar opportunity, anti-jovian sideWorking Group 1
GANYMEDE_FLYBY_RIME_JSGanymede active radar opportunity, jovian sideWorking Group 1
GANYMEDE_RPWI_PASSIVRADGanymede passive radar opportunity for RPWIWorking Group 1
ASTRO_IRR2_PASIPHAEastrometry measurement with inertial pointing to moon PasiphaeWorking Group 2
ASTRO_IRR2_SINOPE Working Group 2
ASTRO_IRR_ELARA Working Group 2
CALLISTO_DISTANT Working Group 2
CHARACTERIZATION_IRR2_CARME Working Group 2
CHARACTERIZATION_IRR2_PASIPHAEcharacterization irregular moon PasiphaeWorking Group 2
CHARACTERIZATION_IRR2_SINOPECharacterization irregular moon SinopeWorking Group 2
CHARACTERIZATION_IRR_ELARACharacterization irregular moon ElaraWorking 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
IO_TOR_DUSTIo torus dustWorking Group 2
CALLISTO_ENAFar approach energetic neutral atom imaging of CallistoWorking Group 3
CALLISTO_FLYBY_RPWI_IONO_AJS Working Group 3
CALLISTO_WAKEIn situ Callisto wake observationWorking Group 3
EUROPA_ENAFar approach energetic neutral atom imaging of EuropaWorking Group 3
EUROPA_FLYBY_RPWI_IONO_AJS Working Group 3
EUROPA_TOR_ISIn situ Europa torus observationWorking Group 3
EUROPA_WAKEIn situ Europa wake observationWorking Group 3
GANYMEDE_ENAFar approach energetic neutral atom imaging of GanymedeWorking Group 3
GANYMEDE_GMIn situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environmentWorking Group 3
GANYMEDE_FLYBY_RPWI_IONO_AJS Working Group 3
GANYMEDE_WAKEIn situ Ganymede wake 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
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

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