| GANYMEDE_GM | In situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environment | Working Group 3 |
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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_TAIL | In situ search for signatures of local magnetic reconnection in the Jovian magnetotail | Working Group 3 |
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| JM_GM | Jupiter Magnetosphere global monitoring.
Large pointing flexibility, constraints mainly driven by PEP | 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_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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| STAR_OCC | | Working Group 4 |
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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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| 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_MONITORING | | Working Group 4 |
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| JUPITER_INCLINED_AURORA | | Working Group 4 |
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| JA_PE9 | | Working Group 4 |
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| JA_PE8 | | Working Group 4 |
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| JA_PE7 | | Working Group 4 |
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| JA_PE6 | | Working Group 4 |
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| JA_PE59 | | Working Group 4 |
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| JA_PE58 | | Working Group 4 |
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| JA_PE57 | | Working Group 4 |
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| JA_PE56 | | Working Group 4 |
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| JA_PE55 | | Working Group 4 |
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| JA_PE54 | | Working Group 4 |
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| JA_PE53 | | Working Group 4 |
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| JA_PE52 | | Working Group 4 |
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| JA_PE51 | | Working Group 4 |
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| JA_PE50 | | Working Group 4 |
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| JA_PE5 | | Working Group 4 |
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| JA_PE49 | | Working Group 4 |
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| JA_PE48 | | Working Group 4 |
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| JA_PE47 | | Working Group 4 |
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| JA_PE46 | | Working Group 4 |
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| JA_PE45 | | Working Group 4 |
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| JA_PE44 | | Working Group 4 |
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| JA_PE43 | | Working Group 4 |
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| JA_PE42 | | Working Group 4 |
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| JA_PE41 | | Working Group 4 |
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| JA_PE40 | | Working Group 4 |
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| JA_PE4 | | Working Group 4 |
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| JA_PE39 | | Working Group 4 |
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| JA_PE38 | | Working Group 4 |
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| JA_PE37 | | Working Group 4 |
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| JA_PE36 | | Working Group 4 |
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| JA_PE34 | | Working Group 4 |
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| JA_PE32 | | Working Group 4 |
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| JA_PE30 | | Working Group 4 |
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| JA_PE3 | | Working Group 4 |
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| JA_PE28 | | Working Group 4 |
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| JA_PE26 | | Working Group 4 |
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| JA_PE24 | | Working Group 4 |
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| JA_PE22 | | Working Group 4 |
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| JA_PE20 | | Working Group 4 |
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| JA_PE2 | | Working Group 4 |
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| JA_PE18 | | Working Group 4 |
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| JA_PE16 | | Working Group 4 |
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| JA_PE14 | | Working Group 4 |
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| JA_PE12 | | Working Group 4 |
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| JA_PE11 | | Working Group 4 |
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| JA_PE10 | | Working Group 4 |
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| JA_PE | | Working Group 4 |
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| J_AURORA | | Working Group 4 |
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| INCLINED_SOUTH | | Working Group 4 |
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| INCLINED_NORTH | | Working Group 4 |
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| EARTH_OCC | Earth occultation by Jupiter | Working Group 4 |
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| EARTH_OCC_EGRESS | Earth occultation by Jupiter. Egress | Working Group 4 |
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| EARTH_OCC_INGRESS | Earth occultation by Jupiter. Ingress | Working Group 4 |
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| JA_PE_OBS | JA_PE generic for link obs<-> segments | Working Group 4 |
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| JA_INCL | Jupiter Atmosphere Inclined segments: at maximum (Northern) and/or minimum (Southern) latitudes.
Pointing target uis Jupiter although pointing details are TBD (track, limb etc...) | Working Group 4 |
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| JA_M | Jupiter Atmosphere Monitoring segments: at regular interval during the tour.
Pointing taregt is Jupiter, although pointing type is TBD (slew scan, raster, nadir etc) | Working Group 4 |
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| JA_PH | Jupiter Atmosphere prime segment at min-90-max phase.
pointing target is Jupiter although pointing type is TBD (limb, etc) | Working Group 4 |
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| JUPITER_PERIJOVE | Jupiter observations | Working Group 4 |
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| JA_PE1 | test 3_2 | Working Group 4 |
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| STELLAR_UVS_OCC_ET | | 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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| J_FD_NAV_FB | | GENERIC |
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| J_FD_EPHEM_G | | GENERIC |
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| J_FD_EPHEM_E | | GENERIC |
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| J_FD_EPHEM_C | | GENERIC |
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