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JA_PE50 Working Group 4
JA_PE49 Working Group 4
JA_PE48 Working Group 4
JA_PE47 Working Group 4
JA_PE46 Working Group 4
JA_PE45 Working Group 4
JA_PE44 Working Group 4
JA_PE43 Working Group 4
JA_PE42 Working Group 4
JA_PE41 Working Group 4
JA_PE40 Working Group 4
JA_PE39 Working Group 4
JA_PE38 Working Group 4
JA_PE37 Working Group 4
JA_PE36 Working Group 4
JM_PE35 Working Group 3
JA_PE34 Working Group 4
JM_PE33share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE32 Working Group 4
JM_PE31share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE30 Working Group 4
JM_PE29share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE28 Working Group 4
JM_PE27share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE26 Working Group 4
JM_PE25share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE24 Working Group 4
JM_PE23share prime high lat PJ between WG3 and WG4Working Group 3
JA_PE22 Working Group 4
JM_PE21share prime high lat PJ between WG3 and WG4Working Group 3
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_26G11 Working Group 2
G_RS_25G10 Working Group 2
G_RS_24G9 Working Group 2
G_RS_23G8 Working Group 2
G_RS_22G7 Working Group 2
C_RS_21C13 Working Group 2
C_RS_20C12 Working Group 2
C_RS_19C11 Working Group 2
G_RS_18G6 Working Group 2
G_RS_17G5 Working Group 2
C_RS_16C10 Working Group 2
C_RS_15C9 Working Group 2
C_RS_14C8 Working Group 2
C_RS_13C7 Working Group 2
C_RS_12C6 Working Group 2
C_RS_11C5 Working Group 2
C_RS_10C4 Working Group 2
C_RS_9C3 Working Group 2
C_RS_8C2 Working Group 2
E_RS_7E2 Working Group 2
E_RS_6E1 Working Group 2
C_RS_5C1 Working Group 2
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
JM_PE_P4_noDL Working Group 3
JA_PE_MAJIS Working Group 4
JA_PE_JANUSIn-situ cloned from JA_PE Remote sensing: cloned from JA_PE removing MAJIS: JANUS: 55.5*76/(76-8*4)=33.62kbps SWI: 5.8 kbps UVS: 2.25 kbps total: 89.17 kbpsWorking Group 4
JA_INCL_noDLcreated for case 1Working Group 4
JA_PE Working Group 4
JM_PE_P4Perijoves with WG3 prime (--> 20/09/18: modified (discussion with OW). assuming ~2 times what is produced in G4-G5 scenario (~6.5-7 Gb). Corresponds roughly to 19kbps, copied from JA_INCL) RS rate assumes no D/L suspension (case 2)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_PE_noDL Working Group 4

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