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Description
1
Group
RINGMOSAIC_B2.0_B5.0_ph090_ph120RINGMOSAIC_B2.0_B5.0_ph090_ph120 B between 2 and 5deg phase between 90 and 120degWorking Group 2
RINGMOSAIC_B2.0_B5.0_ph120_ph150RINGMOSAIC_B2.0_B5.0_ph120_ph150 B between 2 and 5deg phase between 120 and 150degWorking Group 2
RINGMOSAIC_B2.0_B5.0_ph150_ph170RINGMOSAIC_B2.0_B5.0_ph150_ph170 B between 2 and 5deg phase between 150 and 170egWorking Group 2
RINGPHASE_120RINGPHASE_120Working Group 2
RINGPHASE_120_ALTERNATIVERINGPHASE_120_ALTERNATIVEWorking Group 2
RINGPHASE_150RINGPHASE_150Working Group 2
RINGPHASE_150_ALTERNATIVERINGPHASE_150_ALTERNATIVEWorking Group 2
RINGPHASE_170RINGPHASE_170Working Group 2
RINGPHASE_170_ALTERNATIVERINGPHASE_170_ALTERNATIVEWorking Group 2
RINGPHASE_30RINGPHASE_30Working Group 2
RINGPHASE_30_ALTERNATIVERINGPHASE_30_ALTERNATIVEWorking Group 2
RINGPHASE_60RINGPHASE_60Working Group 2
RINGPHASE_60_ALTERNATIVERINGPHASE_60_ALTERNATIVEWorking Group 2
RINGPHASE_90 Working Group 2
RINGPHASE_90_ALTERNATIVERINGPHASE_90_ALTERNATIVEWorking Group 2
RINGPHASE_ph003_ph008RINGPHASE_ph003_ph008 phase between 3 and 8 degWorking Group 2
RINGPHASE_ph025_ph035RINGPHASE_ph025_ph035 phase between 25 and 35degWorking Group 2
RINGPHASE_ph055_ph065RINGPHASE_ph055_ph065Working Group 2
RINGPHASE_ph085_ph095RINGPHASE_ph085_ph095 phase between85 and 95 degWorking Group 2
RINGPHASE_ph115_ph125RINGPHASE_ph115_ph125Working Group 2
RINGPHASE_ph145_ph155RINGPHASE_ph145_ph155Working Group 2
RINGPHASE_ph170_ph_180RINGPHASE_ph170_ph_180Working Group 2
RINGSPIRAL_HPRINGSPIRAL_HPWorking Group 2
RINGSPIRAL_MPRINGSPIRAL_MPWorking Group 2
ROI_INTERSECTIONROI_INTERSECTIONWorking Group 2
SHADOWEDGESHADOWEDGEWorking Group 2
C_IS Working Group 3
C_IS_OBSC_IS_OBSWorking Group 3
CALLISTO_ENA Working Group 3
CALLISTO_FLYBY_RPWI_IONO_AJS Working Group 3
CALLISTO_IONOCALLISTO_IONO Implementation in Geopipeline: Altitude to Callisto lower than 450 kmWorking Group 3
CALLISTO_WAKE Working Group 3
E_IS Working Group 3
E_IS_OBSE_IS_OBSWorking Group 3
EUROPA_ENA Working Group 3
EUROPA_FLYBY_RPWI_IONO_AJS Working Group 3
EUROPA_IONO_ISEUROPA_IONO_IS Implementation in geopipeline: 10 mn before and after closest approachWorking Group 3
EUROPA_TOR_IS Working Group 3
EUROPA_WAKE Working Group 3
G_IS Working Group 3
G_IS_3G3Ganymede in-situ observations around closest approachWorking Group 3
G_IS_4G4 Working Group 3
G_IS_OBSG_IS_OBSWorking Group 3
GANYMEDE_ENA Working Group 3
GANYMEDE_FLYBY_RPWI_IONO_AJS Working Group 3
GANYMEDE_GM Working Group 3
GANYMEDE_IONOGANYMEDE_IONO Implementation in geopipeline: Altitude below 450 kmWorking Group 3
GANYMEDE_WAKE 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_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_PE_P4_noDL 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
JM_PE35 Working Group 3
JUPITER_CB Working Group 3
JUPITER_CPSCurrent plasma sheet crossingWorking Group 3
JUPITER_ENA Working Group 3
JUPITER_GM Working Group 3
JUPITER_NULL Working Group 3
JUPITER_PDT Working Group 3
JUPITER_TAIL Working Group 3
TOR_RS Working Group 3
EARTH_OCCEarth occultation by JupiterWorking Group 4
EARTH_OCC_EGRESS Working Group 4
EARTH_OCC_INGRESS Working Group 4
INCLINED_NORTH Working Group 4
INCLINED_SOUTH Working Group 4
J_AURORA Working Group 4
JA_INCL Working Group 4
JA_INCL_noDLcreated for case 1Working Group 4
JA_M Working Group 4
JA_PE 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_PE_MAJIS Working Group 4
JA_PE_noDL 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_PE13work-aroudn for aegmentation schedulerWorking Group 4
JA_PE14 Working Group 4
JA_PE15work-aroudn for aegmentation schedulerWorking Group 4
JA_PE16 Working Group 4
JA_PE17work-around for segmentation schedulerWorking Group 4
JA_PE18 Working Group 4

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