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Group
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
STAR_OCC Working Group 4
JA_INCL_noDLcreated for case 1Working Group 4
EARTH_OCCEarth occultation by JupiterWorking 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_PE_OBSJA_PE generic for link obs<-> segmentsWorking Group 4
JA_PE21JA_PE21Working Group 4
JA_PE25JA_PE25Working Group 4
JA_PE60JA_PE60Working Group 4
JA_PE61JA_PE61Working Group 4
JA_PE62JA_PE62Working Group 4
JA_PE63JA_PE63Working Group 4
JA_PE64JA_PE64Working Group 4
JA_PE65JA_PE65Working Group 4
JA_PE66JA_PE66Working Group 4
JA_PE67JA_PE67Working Group 4
JA_PE68JA_PE68Working Group 4
JA_PE69JA_PE69Working Group 4
JA_INCLJupiter Atmosphere Inclined segments: at maximum (Northern) and/or minimum (Southern) latitudes. Pointing target uis Jupiter although pointing details are TBD (track, limb etc...)Working Group 4
JA_MJupiter Atmosphere Monitoring segments: at regular interval during the tour. Pointing taregt is Jupiter, although pointing type is TBD (slew scan, raster, nadir etc)Working Group 4
JA_PE17Jupiter Atmosphere prime segment around perijove pass. Pointing target is Jupiter although pointing details are TBD (track, limb, nadir etc)Working Group 4
JA_PHJupiter Atmosphere prime segment at min-90-max phase. pointing target is Jupiter although pointing type is TBD (limb, etc)Working Group 4
STAR_OCC_OBSSTAR_OCC_OBSWorking Group 4
JA_PE1test 3_2Working Group 4
JA_PE19work around for segmentation schedulerWorking Group 4
JA_PE23work around for segmentation schedulerWorking Group 4
JA_PE27work around for segmentation schedulerWorking Group 4
JA_PE29work around for segmentation schedulerWorking Group 4
JA_PE31work around for segmentation schedulerWorking Group 4
JA_PE33work around for segmentation schedulerWorking Group 4
JA_PE35work around for segmentation schedulerWorking Group 4
JA_PE13work-aroudn for aegmentation schedulerWorking Group 4
JA_PE15work-aroudn for aegmentation schedulerWorking 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_INCL Working Group 3
JM_PE_P4_noDL Working Group 3
JM_PE35 Working Group 3
TOR_RS 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
C_IS_OBSC_IS_OBSWorking Group 3
E_IS_OBSE_IS_OBSWorking Group 3
G_IS_OBSG_IS_OBSWorking Group 3
G_IS_3G3Ganymede in-situ observations around closest approachWorking Group 3
JM_GMJupiter Magnetosphere global monitoring. Large pointing flexibility, constraints mainly driven by PEPWorking Group 3
JM_PE_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
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
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
C_distant Working Group 2
C_RS Working Group 2
C_RS_10C4 Working Group 2
C_RS_11C5 Working Group 2
C_RS_12C6 Working Group 2
C_RS_13C7 Working Group 2
C_RS_14C8 Working Group 2
C_RS_15C9 Working Group 2
C_RS_16C10 Working Group 2
C_RS_19C11 Working Group 2
C_RS_20C12 Working Group 2
C_RS_21C13 Working Group 2
C_RS_26C19 Working Group 2
C_RS_30C21 Working Group 2
C_RS_5C1 Working Group 2
C_RS_8C2 Working Group 2
C_RS_9C3 Working Group 2
E_distant Working Group 2
E_RS Working Group 2
E_RS_6E1 Working Group 2
E_RS_7E2 Working Group 2
FB_RS Working Group 2
G_distant Working Group 2
G_RS_17G5 Working Group 2
G_RS_18G6 Working Group 2
G_RS_1G1 Working Group 2
G_RS_22G7 Working Group 2
G_RS_23G8 Working Group 2
G_RS_24G9 Working Group 2
G_RS_25G10 Working Group 2
G_RS_26G11 Working Group 2
G_RS_2G2 Working Group 2
G_RS_4G4 Working Group 2

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