| CHARACTERIZATION_IRR_ELARA | Characterization irregular moon Elara | Working Group 2 |
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| EUROPA_FLYBY_WG2 | | Working Group 2 |
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| GANYMEDE_DISTANT | | Working Group 2 |
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| GANYMEDE_FLYBY_WG2 | | Working Group 2 |
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| IO_MONITORING | - JANUS minimum distance = 7.00e+05 km
- MAJIS minimum distance = 8.00e+05 km
- SWI minimum distance = 6.00e+05 km (able to resolve target when angular size is > 1 mrad)
| Working Group 2 |
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| IO_TOR_DUST | Io torus dust | Working Group 2 |
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| CALLISTO_ENA | Far approach energetic neutral atom imaging of Callisto | Working Group 3 |
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| CALLISTO_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
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| CALLISTO_WAKE | In situ Callisto wake observation | Working Group 3 |
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| EUROPA_ENA | Far approach energetic neutral atom imaging of Europa | Working Group 3 |
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| EUROPA_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
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| EUROPA_TOR_IS | In situ Europa torus observation | Working Group 3 |
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| EUROPA_WAKE | In situ Europa wake observation | Working Group 3 |
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| GANYMEDE_ENA | Far approach energetic neutral atom imaging of Ganymede | Working Group 3 |
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| GANYMEDE_GM | In situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environment | Working Group 3 |
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| GANYMEDE_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
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| GANYMEDE_WAKE | In situ Ganymede wake 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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| JUPITER_CPS | In situ Jupiter current/plasma sheet observation | Working Group 3 |
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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_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_NULL | In situ Jupiter magnetic null search | Working Group 3 |
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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_TAIL | In situ search for signatures of local magnetic reconnection in the Jovian magnetotail | Working Group 3 |
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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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| INCLINED_NORTH | | Working Group 4 |
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| INCLINED_SOUTH | | Working Group 4 |
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| JUPITER_INCLINED_AURORA | | Working Group 4 |
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| JUPITER_PERIJOVE | Jupiter observations | Working Group 4 |
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| JUPITER_PHASE_090 | | Working Group 4 |
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| JUPITER_PHASE_120_DEC | | Working Group 4 |
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| JUPITER_PHASE_120_INC | | Working Group 4 |
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| JUPITER_PHASE_135_DEC | | Working Group 4 |
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| JUPITER_PHASE_135_INC | | Working Group 4 |
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| JUPITER_PHASE_150_DEC | | Working Group 4 |
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| JUPITER_PHASE_150_INC | | Working Group 4 |
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| JUPITER_PHASE_165_DEC | | Working Group 4 |
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| JUPITER_PHASE_165_INC | | Working Group 4 |
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| JUPITER_PHASE_MAX | | Working Group 4 |
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| JUPITER_PHASE_MIN | | Working Group 4 |
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| JUPITER_MONITORING | | Working Group 4 |
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| PERIJOVE_DAYSIDE | | Working Group 4 |
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| PERIJOVE_NIGHTSIDE | | Working Group 4 |
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| PERIJOVE_TERMINATOR | | Working Group 4 |
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| EUR_CAL_TRANSIT_PR | Double transit in front of Jupiter (Europa, Callisto) | WGX |
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| GAN_CAL_TRANSIT_PR | Double transit in front of Jupiter (Ganymede, Callisto) | WGX |
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