| TRANSIT_ET | Event tool support segment definition | GENERIC |
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| TRAJECTORY_SEGMENT | defined segment for moon coverage tool export functionnality | GENERIC |
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| TOR_RS | | Working Group 3 |
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| SUN_OCC_ET | Event tool support segment definition | GENERIC |
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| STELLAR_UVS_OCC_ET | | GENERIC |
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| STELLAR_OCC_ET | Event tool support segment definition | GENERIC |
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| STAR_OCC | | Working Group 4 |
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| SPICE_ATT_TRANSFER_HOT | Default attitude during cruise phase applicable during the hot phases | GENERIC |
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| SPICE_ATT_TRANSFER_COLD | Default attitude during cruise phase | GENERIC |
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| SPICE_ATT_JUPITER_TOUR | Default attitude during the Tour phase | GENERIC |
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| SPICE_ATT_GOTOTRANSFER_COLD_SUP_SOL_CONJ | Default attitude during cruise phase superior solar conjunctions 'cold' | GENERIC |
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| SPICE_ATT_GOTOMARS_NPO | | GENERIC |
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| SPICE_ATT_GOTOMARS_NOA_HOT | | GENERIC |
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| SPICE_ATT_GOTOJUPITER_TOUR_SUP_SOL_CONJ | Default attitude during superior solar conjunction | GENERIC |
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| SPICE_ATT_GOTOGANYMEDE_NPO | | GENERIC |
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| SPICE_ATT_GOTOGANYMEDE_NOA_HOT | | GENERIC |
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| SPICE_ATT_GOTOGANYMEDE_NOA | | GENERIC |
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| SPICE_ATT_GOTOEUROPA_NPO | | GENERIC |
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| SPICE_ATT_GOTOEUROPA_NOA_HOT | | GENERIC |
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| SPICE_ATT_GOTOEUROPA_NOA | | GENERIC |
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| SPICE_ATT_GOTOEARTH_NPO | | GENERIC |
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| SPICE_ATT_GOTOEARTH_NOA_HOT | | GENERIC |
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| SPICE_ATT_GOTOEARTH_NOA | | GENERIC |
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| SPICE_ATT_GOTOEARTH_COMMS | Earth communication segment | GENERIC |
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| SPICE_ATT_GOTOCALLISTO_NPO | | GENERIC |
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| SPICE_ATT_GOTOCALLISTO_NOA_HOT | | GENERIC |
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| SPICE_ATT_GOTOCALLISTO_NOA | | GENERIC |
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| SPICE_ATT_GANYMEDE_PHASE | Default attitude during the Ganymede phase | GENERIC |
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| RING_PHASECURV_90 | | Working Group 2 |
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| RING_PHASECURV_80 | | Working Group 2 |
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| RING_PHASECURV_70 | | Working Group 2 |
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| RING_PHASECURV_60 | | Working Group 2 |
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| RING_PHASECURV_50 | | Working Group 2 |
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| RING_PHASECURV_5 | Opportunity 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 deg | Working Group 2 |
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| RING_PHASECURV_40 | | Working Group 2 |
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| RING_PHASECURV_30 | | Working Group 2 |
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| RING_PHASECURV_20 | | Working Group 2 |
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| RING_PHASECURV_170 | | Working Group 2 |
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| RING_PHASECURV_160 | | Working Group 2 |
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| RING_PHASECURV_150 | | Working Group 2 |
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| RING_PHASECURV_140 | | Working Group 2 |
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| RING_PHASECURV_130 | | Working Group 2 |
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| RING_PHASECURV_120 | | Working Group 2 |
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| RING_PHASECURV_110 | | Working Group 2 |
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| RING_PHASECURV_100 | | Working Group 2 |
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| RING_PHASECURV_10 | Opportunity 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 deg | Working Group 2 |
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| RING_LP | Ring low phase | Working Group 2 |
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| RING_HP | Ring high phase | Working Group 2 |
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| PR | | WGX |
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| PERIJOVE_TERMINATOR | | Working Group 4 |
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| PERIJOVE_NIGHTSIDE | | Working Group 4 |
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| PERIJOVE_DAYSIDE | | Working Group 4 |
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| OPNAV_GAN | OPNAV_GAN | GENERIC |
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| OPNAV_EUR | OPNAV_EUR | GENERIC |
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| OPNAV_CAL | OPNAV_CAL | GENERIC |
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| JUPITER_TAIL | In situ search for signatures of local magnetic reconnection in the Jovian magnetotail | Working Group 3 |
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| JUPITER_PHASE_MIN | | Working Group 4 |
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| JUPITER_PHASE_MAX | | Working Group 4 |
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| JUPITER_PHASE_165_INC | | Working Group 4 |
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| JUPITER_PHASE_165_DEC | | Working Group 4 |
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| JUPITER_PHASE_150_INC | | Working Group 4 |
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| JUPITER_PHASE_150_DEC | | Working Group 4 |
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| JUPITER_PHASE_135_INC | | Working Group 4 |
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| JUPITER_PHASE_135_DEC | | Working Group 4 |
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| JUPITER_PHASE_120_INC | | Working Group 4 |
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| JUPITER_PHASE_120_DEC | | Working Group 4 |
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| JUPITER_PHASE_090 | | Working Group 4 |
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| JUPITER_PERIJOVE | Jupiter observations | Working Group 4 |
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| JUPITER_PDT | In situ Jupiter particle distribution transition region observation.
Maximize pitch angle coverage for PEP/JEI, JDC,JoEE, JENI (ion mode) | Working Group 3 |
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| JUPITER_NULL | In situ Jupiter magnetic null search | Working Group 3 |
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| JUPITER_MONITORING | | Working Group 4 |
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| JUPITER_INCLINED_AURORA | | Working Group 4 |
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| JUPITER_GM | In 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 |
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| JUPITER_FD_WOL_FB | In 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 |
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| JUPITER_FD_WOL | Flight dynamics wheel off-loading slot, outside of Flyby preparation and recuperation | GENERIC |
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| JUPITER_FD_TCM | | GENERIC |
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| JUPITER_FD_NAV_FB | | GENERIC |
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| JUPITER_FD_EPHEM_GAN | | GENERIC |
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| JUPITER_FD_EPHEM_EUR | | GENERIC |
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| JUPITER_FD_EPHEM_CAL | | GENERIC |
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| JUPITER_ENA | Imaging 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 torus | Working Group 3 |
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| JUPITER_CPS | In situ Jupiter current/plasma sheet observation | Working Group 3 |
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| JUPITER_CB | In 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 |
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| JMAG_CALROLL | 5 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 GOI | WGX |
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| JM_PE35 | | Working Group 3 |
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| JM_PE33 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE31 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE29 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE27 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE25 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE23 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE21 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE19 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE17 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE15 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE13 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
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| JM_PE_P4_noDL | | Working Group 3 |
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| JM_PE_P4 | Perijoves 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 |
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| JM_PE_OBS | Jupiter Magnetosphere perijove segments containing link to observations database | Working Group 3 |
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| JM_PE | assuming:
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 |
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