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Mnemonic
Description
Group
TRANSIT_ETEvent tool support segment definitionGENERIC
TRAJECTORY_SEGMENTdefined segment for moon coverage tool export functionnalityGENERIC
TOR_RS Working Group 3
SUN_OCC_ETEvent tool support segment definitionGENERIC
STELLAR_OCC_ETEvent tool support segment definitionGENERIC
STAR_OCC Working Group 4
SPICE_ATT_TRANSFER_HOTDefault attitude during cruise phase applicable during the hot phasesGENERIC
SPICE_ATT_TRANSFER_COLDDefault attitude during cruise phaseGENERIC
SPICE_ATT_JUPITER_TOURDefault attitude during the Tour phaseGENERIC
SPICE_ATT_GOTOTRANSFER_COLD_SUP_SOL_CONJDefault attitude during cruise phase superior solar conjunctions 'cold'GENERIC
SPICE_ATT_GOTOMARS_NPO GENERIC
SPICE_ATT_GOTOMARS_NOA_HOT GENERIC
SPICE_ATT_GOTOJUPITER_TOUR_SUP_SOL_CONJDefault attitude during superior solar conjunctionGENERIC
SPICE_ATT_GOTOGANYMEDE_NPO GENERIC
SPICE_ATT_GOTOGANYMEDE_NOA_HOT GENERIC
SPICE_ATT_GOTOGANYMEDE_NOA GENERIC
SPICE_ATT_GOTOEUROPA_NPO GENERIC
SPICE_ATT_GOTOEUROPA_NOA_HOT GENERIC
SPICE_ATT_GOTOEUROPA_NOA GENERIC
SPICE_ATT_GOTOEARTH_NPO GENERIC
SPICE_ATT_GOTOEARTH_NOA_HOT GENERIC
SPICE_ATT_GOTOEARTH_NOA GENERIC
SPICE_ATT_GOTOEARTH_COMMSEarth communication segmentGENERIC
SPICE_ATT_GOTOCALLISTO_NPO GENERIC
SPICE_ATT_GOTOCALLISTO_NOA_HOT GENERIC
SPICE_ATT_GOTOCALLISTO_NOA GENERIC
SPICE_ATT_GANYMEDE_PHASEDefault attitude during the Ganymede phaseGENERIC
RING_PHASECURV_90 Working Group 2
RING_PHASECURV_80 Working Group 2
RING_PHASECURV_70 Working Group 2
RING_PHASECURV_60 Working Group 2
RING_PHASECURV_50 Working Group 2
RING_PHASECURV_5Opportunity implementation in geopipeline SC distance to Jupiter larger than 8e5 km SC elevation above the rings lower than 0.5 deg Only one Ansae tested for phase conditions - value must be between 5 deg and 10 degWorking Group 2
RING_PHASECURV_40 Working Group 2
RING_PHASECURV_30 Working Group 2
RING_PHASECURV_20 Working Group 2
RING_PHASECURV_170 Working Group 2
RING_PHASECURV_160 Working Group 2
RING_PHASECURV_150 Working Group 2
RING_PHASECURV_140 Working Group 2
RING_PHASECURV_130 Working Group 2
RING_PHASECURV_120 Working Group 2
RING_PHASECURV_110 Working Group 2
RING_PHASECURV_100 Working Group 2
RING_PHASECURV_10Opportunity implementation in geopipeline SC distance to Jupiter larger than 8e5 km SC elevation above the rings lower than 0.5 deg Only one Ansae tested for phase conditions - value must be between 10 deg and 20 degWorking Group 2
RING_LP Working Group 2
RING_HP Working Group 2
PR WGX
PERIJOVE_TERMINATOR Working Group 4
PERIJOVE_NIGHTSIDE Working Group 4
PERIJOVE_DAYSIDE Working Group 4
OPNAV_GANOPNAV_GANGENERIC
OPNAV_EUROPNAV_EURGENERIC
OPNAV_CALOPNAV_CALGENERIC
JUPITER_TAIL Working Group 3
JUPITER_PHASE_MIN Working Group 4
JUPITER_PHASE_MAX Working Group 4
JUPITER_PHASE_165_INC Working Group 4
JUPITER_PHASE_165_DEC Working Group 4
JUPITER_PHASE_150_INC Working Group 4
JUPITER_PHASE_150_DEC Working Group 4
JUPITER_PHASE_135_INC Working Group 4
JUPITER_PHASE_135_DEC Working Group 4
JUPITER_PHASE_120_INC Working Group 4
JUPITER_PHASE_120_DEC Working Group 4
JUPITER_PHASE_090 Working Group 4
JUPITER_PERIJOVEJupiter observations Working Group 4
JUPITER_PDT Working Group 3
JUPITER_NULL Working Group 3
JUPITER_MONITORING Working Group 4
JUPITER_INCLINED_AURORA Working Group 4
JUPITER_GM Working Group 3
JUPITER_FD_WOL_FBIn the last week before the fly-by a WOL slot shall be combined with the TCM slot at To– 3 days (i.e. a single 3-hr slot). Another 2-hour WOL slot shall be reserved at To + 12 hours.GENERIC
JUPITER_FD_WOLFlight dynamics wheel off-loading slot, outside of Flyby preparation and recuperationGENERIC
JUPITER_FD_TCM GENERIC
JUPITER_FD_NAV_FB GENERIC
JUPITER_FD_EPHEM_GAN GENERIC
JUPITER_FD_EPHEM_EUR GENERIC
JUPITER_FD_EPHEM_CAL GENERIC
JUPITER_ENA Working Group 3
JUPITER_CPSCurrent plasma sheet crossingWorking Group 3
JUPITER_CB Working Group 3
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_PE35 Working Group 3
JM_PE33share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE31share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE29share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE27share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE25share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE23share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE21share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE19share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE17share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE15share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE13share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE_P4_noDL Working 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_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking 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_INCL Working Group 3

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