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JA_PE35work around for segmentation schedulerWorking Group 4
JA_PE33work around for segmentation schedulerWorking Group 4
JA_PE31work around for segmentation schedulerWorking Group 4
JA_PE29work around for segmentation schedulerWorking Group 4
JA_PE27work around for segmentation schedulerWorking Group 4
JA_PE23work around for segmentation schedulerWorking Group 4
JA_PE19work around for segmentation schedulerWorking Group 4
EUR_CAL_GAN_TRANSIT_PRTriple transit in front of JupiterWGX
G_GPH_1G1test 3_2Working Group 1
C_GPH_8C1test 3_2Working Group 1
C_GPH_22C11test 3_2Working Group 1
C_GPH_18C10test 3_2Working Group 1
C_GPH_16C8test 3_2Working Group 1
C_GPH_14C6test 3_2Working Group 1
C_GPH_13C5test 3_2Working Group 1
C_GPH_12C4Test 3_2Working Group 1
C_GPH_11C3test 3_2Working Group 1
C_GPH_10C2test 3_2Working Group 1
G_RS_9G6test 3_2Working Group 2
G_RS_26G12test 3_2Working Group 2
G_RS_24G10test 3_2Working Group 2
G_RS_21G9test 3_2Working Group 2
G_RS_20G8test 3_2Working Group 2
G_RS_19G7test 3_2Working Group 2
C_RS_8C1test 3_2Working Group 2
C_RS_23C12test 3_2Working Group 2
C_RS_22C11test 3_2Working Group 2
C_RS_18C10test 3_2Working Group 2
C_RS_17C9test 3_2Working Group 2
C_RS_16C8test 3_2Working Group 2
C_RS_15C7test 3_2Working Group 2
C_RS_14C6test 3_2Working Group 2
C_RS_13C5test 3_2Working Group 2
C_RS_12C4test 3_2Working Group 2
C_RS_11C3test 3_2Working Group 2
C_RS_10C2test 3_2Working Group 2
JA_PE1test 3_2Working Group 4
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
FB_BATTERY_RECOVERY_STANDARDSegment to allow for battery rechargeGENERIC
FB_BATTERY_RECOVERY_FASTSegment to allow for battery rechargeGENERIC
RING_LPRing low phaseWorking Group 2
RING_HPRing high phaseWorking Group 2
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
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_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
OPNAV_GANOPNAV_GANGENERIC
OPNAV_EUROPNAV_EURGENERIC
OPNAV_CALOPNAV_CALGENERIC
J_SATjupiter satellite GENERICWorking Group 2
JUPITER_PERIJOVEJupiter observationsWorking Group 4
JM_PE_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
JA_PE25JA_PE25Working Group 4
JA_PE21JA_PE21Working Group 4
JA_PE_OBSJA_PE generic for link obs<-> segmentsWorking Group 4
IO_TOR_DUSTIo torus dustWorking Group 2
IO_ECLIPSEIo observation while Io is in eclipse.Working Group 2
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
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_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking Group 3
JUPITER_GMIn situ mapping of global configuration and monitoring dynamics of the Jovian magnetospheric environment. corotation should be in the FoV of PEP/JDC or PEP/JEI. Conditions for coverage: ◦ Minimum angle less than about 11.25 deg (half-azimuthal sector size) of a JEI or JDC pixel from corotation ◦ Boresight angle of JDC or JEI less than ˜90 deg Conditions for ideal coverage: ◦ Minimum angle less than about 11.25 deg (half-azimuthal sector size) of a JEI or JDC pixel from corotation ◦ Boresight angle less than ˜75 deg (JEI) or 70 deg (JDC): corotation away from the FoV edge JDC is preferred for monitoring corotation, over JEI, when possible.Working Group 3
GANYMEDE_GMIn situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environmentWorking Group 3
JUPITER_PDTIn situ Jupiter particle distribution transition region observation. Maximize pitch angle coverage for PEP/JEI, JDC,JoEE, JENI (ion mode)Working Group 3
JUPITER_NULLIn situ Jupiter magnetic null searchWorking Group 3
JUPITER_CPSIn situ Jupiter current/plasma sheet observationWorking Group 3
JUPITER_CBIn 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.Working Group 3
GANYMEDE_WAKEIn situ Ganymede wake observationWorking Group 3
EUROPA_WAKEIn situ Europa wake observationWorking Group 3
EUROPA_TOR_ISIn situ Europa torus observationWorking Group 3
CALLISTO_WAKEIn situ Callisto wake observationWorking Group 3
JUPITER_ENAImaging of Jupiter's magnetosphere in energetic neutral atoms (ENAs).Maximize pitch angle coverage with PEP JEI,JDC,JoEE, JENI (ion mode) a) JENI has a broad FoV and captures Jupiter and the Io/Europa torus and magnetosphere at most times. No special pointing design required for JENI besides requiring an approximate nadir pointing (considerable offsets can still be acceptable) b) JNA disk-shaped/slit FoV has a slight offset from the XZ spacecraft plane, meaning that during nadir pointing, it images preferentially the northern or southern extension of the Europa/Io torus, whereas Jupiter may be in the edge or outside of the FoV, especially at large distances. Scans (small rotations around Sc-X) or periods with stable, small offset of the SC-xz plane from Nadir can help to better image stronger emissions from the equatorial torusWorking Group 3
G_RS_3G3HAA as per 3GM UM IS considering NIMWorking Group 2
G_GPH_OBSGeneric G_GPH containing link to obs defWorking Group 1
GANYMEDE_IONOGANYMEDE_IONO In situ Ganymede ionosphere observationWorking Group 3
GANYMEDE_RPWI_PASSIVRADGanymede passive radar opportunity for RPWIWorking Group 1
GANYMEDE_FB_RSGanymede flyby remote sensingWorking Group 2
GANYMEDE_FLYBY_RIME_JSGanymede active radar opportunity, jovian sideWorking Group 1
GANYMEDE_FLYBY_RIME_AJSGanymede active radar opportunity, anti-jovian sideWorking Group 1
G_RS_OBSG_RS GENERICWorking Group 2
JUPITER_FD_WOLFlight dynamics wheel off-loading slot, outside of Flyby preparation and recuperationGENERIC
GANYMEDE_ENAFar approach energetic neutral atom imaging of GanymedeWorking Group 3
EUROPA_ENAFar approach energetic neutral atom imaging of EuropaWorking Group 3
CALLISTO_ENAFar approach energetic neutral atom imaging of CallistoWorking Group 3
TRANSIT_ETEvent tool support segment definitionGENERIC
SUN_OCC_ETEvent tool support segment definitionGENERIC
STELLAR_OCC_ETEvent tool support segment definitionGENERIC
FLYBY_ETEvent tool support segment definitionGENERIC
EARTH_OCC_ETEvent tool support segment definitionGENERIC
EUROPA_IONO_ISEUROPA_IONO_IS In situ Europa ionosphere observationWorking Group 3
E_RS_OBSEuropa remote sensing generic segment containing obs database linkWorking Group 2
EUROPA_RPWI_PASSIVRADEuropa passive radar opportunity for RPWIWorking Group 1

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