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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
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
JMAG_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.JMAG
JMAG_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.JMAG
JUICE_PRIME_OBSERVATIONPlaceholder for JUICE SOC Observations.JUICE
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
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
JUPITER_CPSIn situ Jupiter current/plasma sheet 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
JUPITER_FD_EPHEM_CAL GENERIC
JUPITER_FD_EPHEM_EUR GENERIC
JUPITER_FD_EPHEM_GAN GENERIC
JUPITER_FD_NAV_FB GENERIC
JUPITER_FD_TCM GENERIC
JUPITER_FD_WOLFlight dynamics wheel off-loading slot, outside of Flyby preparation and recuperationGENERIC
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_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
JUPITER_INCLINED_AURORA Working Group 4
JUPITER_MONITORING Working Group 4
JUPITER_NULLIn situ Jupiter magnetic null searchWorking 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_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_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking Group 3
MAJIS_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.MAJIS
MAJIS_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.MAJIS
NAVCAM_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.NAVCAM
NAVCAM_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.NAVCAM
OPNAV_CALOPNAV_CALGENERIC
OPNAV_EUROPNAV_EURGENERIC
OPNAV_GANOPNAV_GANGENERIC
PEP_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.PEP
PEP_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.PEP
PERIJOVE_DAYSIDE Working Group 4
PERIJOVE_NIGHTSIDE Working Group 4
PERIJOVE_TERMINATOR Working Group 4
PR WGX
RADEM_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RADEM
RECOVERY GENERIC
RECOVERY_FLYBY20.5 hour recovery segments to be scheduled flybys Duration is derived from https://issues.cosmos.esa.int/juicewiki/display/SOCDEV/Downlink%2C+Recovery%2C+and+Eclipse+Scenario+AnalysisGENERIC
RIME_OBSERBATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RIME
RIME_PRIME_OBSERVATION RIME
RING_HPRing high phaseWorking Group 2
RING_LPRing low phaseWorking 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_PHASECURV_100 Working Group 2
RING_PHASECURV_110 Working Group 2
RING_PHASECURV_120 Working Group 2
RING_PHASECURV_130 Working Group 2
RING_PHASECURV_140 Working Group 2
RING_PHASECURV_150 Working Group 2
RING_PHASECURV_160 Working Group 2
RING_PHASECURV_170 Working Group 2
RING_PHASECURV_20 Working Group 2
RING_PHASECURV_30 Working Group 2
RING_PHASECURV_40 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_50 Working Group 2
RING_PHASECURV_60 Working Group 2
RING_PHASECURV_70 Working Group 2
RING_PHASECURV_80 Working Group 2
RING_PHASECURV_90 Working Group 2
RINGMATTERRINGMATTER. Observations of the main rings and the gossamer rings, imaging the ring ansae from moderately large elevation. The moderatly large elevation will reveal azimuthal structure in the rings and the presence of clumps at the resolution limit of the imaging.Working Group 2
RINGMOSAICRINGMOSAIC (Janus definition). impression of the extent of the whole ring systemWorking Group 2
RINGPHASE Working Group 2
RINGSPIRAL_HPRINGSPIRAL_HP (high phase, Janus def)Working Group 2
RINGSPIRAL_MPRINGSPIRAL_MP (medium phase: JANUS Def)Working Group 2
ROI_INTERSECTIONROI_INTERSECTIONWorking Group 2
RPWI_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RPWI
RPWI_PRIME_OBSERVATIONPlaceholder Segment to accomodate the detailed scenario observation plan generation process.RPWI
SHADOWEDGErings SHADOWEDGE. Imaging of the ring region intersected by the planetary shadow at moderate elevation and very high phase. Especially for the very faint gossamer rings and the Thebe extensionWorking Group 2
SHT_TESTSHT_TESTGENERIC
SOC_OBSERVATION SOC

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