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2
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3
Description
1
Group
CAL WGX
PR WGX
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
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
J_FD_EPHEM_C GENERIC
J_FD_EPHEM_E GENERIC
J_FD_EPHEM_G GENERIC
J_FD_NAV_FB GENERIC
J_FD_TCM GENERIC
J_FD_WOL GENERIC
J_FD_WOL_FB GENERIC
OPNAV_CALOPNAV_CALGENERIC
OPNAV_EUROPNAV_EURGENERIC
OPNAV_GANOPNAV_GANGENERIC
SPICE_ATT_GANYMEDE_PHASEDefault attitude during the Ganymede phaseGENERIC
SPICE_ATT_GOTOEARTH_COMMSEarth communication segmentGENERIC
SPICE_ATT_GOTOJUPITER_TOUR_SUP_SOL_CONJDefault attitude during superior solar conjunctionGENERIC
SPICE_ATT_GOTOTRANSFER_COLD_SUP_SOL_CONJDefault attitude during cruise phase superior solar conjunctions 'cold'GENERIC
SPICE_ATT_JUPITER_TOURDefault attitude during the Tour phaseGENERIC
SPICE_ATT_TRANSFER_COLDDefault attitude during cruise phaseGENERIC
SPICE_ATT_TRANSFER_HOTDefault attitude during cruise phase applicable during the hot phasesGENERIC
EARTH_OCCEarth occultation by JupiterWorking Group 4
J_AURORA Working Group 4
JA_INCL Working Group 4
JA_M Working Group 4
JA_PE Working Group 4
JA_PE_OBSJA_PE generic for link obs<-> segmentsWorking Group 4
JA_PE1test 3_2Working Group 4
JA_PE10 Working Group 4
JA_PE11 Working Group 4
JA_PE12 Working Group 4
JA_PE14 Working Group 4
JA_PE16 Working Group 4
JA_PE18 Working Group 4
JA_PE2 Working Group 4
JA_PE20 Working Group 4
JA_PE22 Working Group 4
JA_PE24 Working Group 4
JA_PE26 Working Group 4
JA_PE28 Working Group 4
JA_PE3 Working Group 4
JA_PE30 Working Group 4
JA_PE32 Working Group 4
JA_PE34 Working Group 4
JA_PE36 Working Group 4
JA_PE37 Working Group 4
JA_PE38 Working Group 4
JA_PE39 Working Group 4
JA_PE4 Working Group 4
JA_PE40 Working Group 4
JA_PE41 Working Group 4
JA_PE42 Working Group 4
JA_PE43 Working Group 4
JA_PE44 Working Group 4
JA_PE45 Working Group 4
JA_PE46 Working Group 4
JA_PE47 Working Group 4
JA_PE48 Working Group 4
JA_PE49 Working Group 4
JA_PE5 Working Group 4
JA_PE50 Working Group 4
JA_PE51 Working Group 4
JA_PE52 Working Group 4
JA_PE53 Working Group 4
JA_PE54 Working Group 4
JA_PE55 Working Group 4
JA_PE56 Working Group 4
JA_PE57 Working Group 4
JA_PE58 Working Group 4
JA_PE59 Working Group 4
JA_PE6 Working Group 4
JA_PE7 Working Group 4
JA_PE8 Working Group 4
JA_PE9 Working Group 4
JA_PH Working Group 4
STAR_OCC Working Group 4
C_IS Working Group 3
E_IS Working Group 3
G_IS Working Group 3
G_IS_4G4 Working Group 3
JM_CB Working Group 3
JM_ENA Working Group 3
JM_GM Working Group 3
JM_INCL Working 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_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
TOR_RS Working Group 3
C_distant Working Group 2

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