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JA_PE25JA_PE25Working Group 4
JA_PE23work around for segmentation schedulerWorking Group 4
JA_PE21JA_PE21Working Group 4
JA_PE19work around for segmentation schedulerWorking Group 4
JA_PE17work-around for segmentation schedulerWorking Group 4
JA_PE15work-aroudn for aegmentation schedulerWorking Group 4
JA_PE13work-aroudn for aegmentation schedulerWorking Group 4
EARTH_OCCEarth occultation by JupiterWorking Group 4
JA_PE_OBSJA_PE generic for link obs<-> segmentsWorking Group 4
JA_PE69JA_PE69Working Group 4
JA_PE68JA_PE68Working Group 4
JA_PE67JA_PE67Working Group 4
JA_PE64JA_PE64Working Group 4
JA_PE66JA_PE66Working Group 4
JA_PE65JA_PE65Working Group 4
JA_PE63JA_PE63Working Group 4
JA_PE62JA_PE62Working Group 4
JA_PE61JA_PE61Working Group 4
JA_PE60JA_PE60Working Group 4
JA_PE1test 3_2Working Group 4
JA_PE59 Working Group 4
JA_PE58 Working Group 4
JA_PE57 Working Group 4
JA_PE56 Working Group 4
JA_PE55 Working Group 4
JA_PE54 Working Group 4
JA_PE53 Working Group 4
JA_PE52 Working Group 4
STAR_OCC Working Group 4
JA_PE51 Working Group 4
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
JA_PE34 Working Group 4
JA_PE32 Working Group 4
JA_PE30 Working Group 4
JA_PE28 Working Group 4
JA_PE26 Working Group 4
JA_PE24 Working Group 4
JA_PE22 Working Group 4
JA_PE20 Working Group 4
JA_PE18 Working Group 4
JA_PE16 Working Group 4
JA_PE14 Working Group 4
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
J_AURORA Working Group 4
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
JA_PH Working Group 4
JA_PE_noDL Working Group 4
JA_M Working Group 4
JA_INCL Working Group 4
EARTH_OCC_EGRESSEarth occultation by Jupiter. EgressWorking Group 4
EARTH_OCC_INGRESSEarth occultation by Jupiter. IngressWorking Group 4
INCLINED_NORTH Working Group 4
INCLINED_SOUTH Working Group 4
JUPITER_INCLINED_AURORA Working Group 4
JUPITER_PERIJOVEJupiter observationsWorking Group 4
JUPITER_PHASE_090 Working Group 4
JUPITER_PHASE_120_DEC Working Group 4
JUPITER_PHASE_120_INC Working Group 4
JUPITER_PHASE_135_DEC Working Group 4
JUPITER_PHASE_135_INC Working Group 4
JUPITER_PHASE_150_DEC Working Group 4
JUPITER_PHASE_150_INC Working Group 4
JUPITER_PHASE_165_DEC Working Group 4
JUPITER_PHASE_165_INC Working Group 4
JUPITER_PHASE_MAX Working Group 4
JUPITER_PHASE_MIN Working Group 4
JUPITER_MONITORING Working Group 4
PERIJOVE_DAYSIDE Working Group 4
PERIJOVE_NIGHTSIDE Working Group 4
PERIJOVE_TERMINATOR Working Group 4
JUPITER_CPIn 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. CP stands for corotation profileWorking Group 3
E_IS_OBSE_IS_OBSWorking Group 3
C_IS_OBSC_IS_OBSWorking Group 3

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