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J_SAT_ERSA Working Group 2
J_SAT_HARPALYKE Working Group 2
J_SAT_HEGEMONE Working Group 2
J_SAT_HELIKE Working Group 2
J_SAT_HERMIPPE Working Group 2
J_SAT_HERSE Working Group 2
J_SAT_HIMALIA Working Group 2
J_SAT_INN_AST_A Working Group 2
J_SAT_INN_AST_T Working Group 2
J_SAT_INN_CHAR_A Working Group 2
J_SAT_IOCASTE Working Group 2
J_SAT_IRR_AST_E Working Group 2
J_SAT_IRR_CHAR_E Working Group 2
J_SAT_ISONOE Working Group 2
J_SAT_KALLICHORE Working Group 2
J_SAT_LEDA Working Group 2
J_SAT_LYSITHEA Working Group 2
J_SAT_MEGACLITE Working Group 2
J_SAT_PANDIA Working Group 2
J_SAT_PASIPHAE Working Group 2
J_SAT_PASITHEE Working Group 2
J_SAT_PRAXIDIKE Working Group 2
J_SAT_SINOPE Working Group 2
J_SAT_TAYGETE Working Group 2
J_SAT_THEMISTO Working Group 2
J_SAT_VALETUDO Working Group 2
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_PE14 Working Group 4
JA_PE16 Working Group 4
JA_PE18 Working Group 4
JA_PE19work around for segmentation schedulerWorking Group 4
JA_PE2 Working Group 4
JA_PE20 Working Group 4
JA_PE21JA_PE21Working Group 4
JA_PE22 Working Group 4
JA_PE23work around for segmentation schedulerWorking Group 4
JA_PE24 Working Group 4
JA_PE25JA_PE25Working Group 4
JA_PE26 Working Group 4
JA_PE27work around for segmentation schedulerWorking Group 4
JA_PE28 Working Group 4
JA_PE29work around for segmentation schedulerWorking Group 4
JA_PE3 Working Group 4
JA_PE30 Working Group 4
JA_PE31work around for segmentation schedulerWorking Group 4
JA_PE32 Working Group 4
JA_PE33work around for segmentation schedulerWorking Group 4
JA_PE34 Working Group 4
JA_PE35work around for segmentation schedulerWorking 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
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

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