| GANYMEDE_FLYBY_UVS | | Working Group 1 |
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| CALLISTO_FLYBY | | Working Group 1 |
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| CALLISTO_FLYBY_3GM | | Working Group 1 |
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| CALLISTO_FLYBY_GALA | | Working Group 1 |
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| CALLISTO_FLYBY_JANUS | | Working Group 1 |
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| CALLISTO_FLYBY_MAJIS | | Working Group 1 |
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| EUROPA_FLYBY | | Working Group 1 |
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| EUROPA_FLYBY_3GM | | Working Group 1 |
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| EUROPA_FLYBY_GALA | | Working Group 1 |
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| EUROPA_FLYBY_JANUS | | Working Group 1 |
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| EUROPA_FLYBY_MAJIS | | Working Group 1 |
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| GANYMEDE_FLYBY | | Working Group 1 |
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| GANYMEDE_FLYBY_3GM | | Working Group 1 |
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| GANYMEDE_FLYBY_GALA | | Working Group 1 |
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| GANYMEDE_FLYBY_JANUS | | Working Group 1 |
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| GANYMEDE_FLYBY_MAJIS | | Working Group 1 |
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| CALLISTO_FLYBY_RIME_AJS | Callisto active radar opportunity, anti-jovian side | Working Group 1 |
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| CALLISTO_FLYBY_RIME_JS | Callisto active radar opportunity, jovian side | Working Group 1 |
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| CALLISTO_RPWI_PASSIVRAD | Callisto passive radar opportunity for RPWI | Working Group 1 |
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| EUROPA_FLYBY_RIME_AJS | Europa active radar opportunity, anti-jovian side | Working Group 1 |
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| EUROPA_FLYBY_RIME_JS | Europa active radar opportunity, jovian side | Working Group 1 |
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| EUROPA_RPWI_PASSIVRAD | Europa passive radar opportunity for RPWI | Working Group 1 |
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| GANYMEDE_FLYBY_RIME_AJS | Ganymede active radar opportunity, anti-jovian side | Working Group 1 |
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| GANYMEDE_FLYBY_RIME_JS | Ganymede active radar opportunity, jovian side | Working Group 1 |
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| GANYMEDE_RPWI_PASSIVRAD | Ganymede passive radar opportunity for RPWI | Working Group 1 |
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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_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_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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| EUROPA_DISTANT | | Working Group 2 |
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| ASTRO_IRR2_SINOPE | | Working Group 2 |
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| ASTRO_IRR_ELARA | | Working Group 2 |
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| CALLISTO_DISTANT | | Working Group 2 |
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| CALLISTO_FLYBY_WG2 | | Working Group 2 |
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| CHARACTERIZATION_IRR2_CARME | | 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 |
|---|
| ASTRO_INNER | Astrometry inner moons | Working Group 2 |
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| ASTRO_IRR2_ANANKE | Astrometry irregular moon Ananke | Working Group 2 |
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| ASTRO_IRR2_CARME | Astrometry irregular moon Carme | Working Group 2 |
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| ASTRO_IRR1_CARPO | Astrometry irregular moon CARPO | Working Group 2 |
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| ASTRO_IRR1_CHALDENE | Astrometry irregular moon CHALDENE | Working Group 2 |
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| ASTRO_IRR1_HIMALIA | Astrometry irregular moon HIMALIA | Working Group 2 |
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| ASTRO_IRR1_KALLICHORE | Astrometry irregular moon KALLICHORE | Working Group 2 |
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| ASTRO_IRR1_LEDA | Astrometry irregular moon LEDA | Working Group 2 |
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| ASTRO_IRR1_LYSITHEA | Astrometry irregular moon LYSITHEA | Working Group 2 |
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| ASTRO_IRR1_TAYGETE | Astrometry irregular moon TAYGETE | Working Group 2 |
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| ASTRO_IRR1_THEMISTO | Astrometry irregular moon THEMISTO | Working Group 2 |
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| ASTRO_IRR2_PASIPHAE | astrometry measurement with inertial pointing to moon Pasiphae | Working Group 2 |
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| CALLISTO_FB_RS | Callisto Flyby remote sensing | Working Group 2 |
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| CHARACTERIZATION_IRR2_ANANKE | Characterization irregular moon ANANKE | Working Group 2 |
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| CHARACTERIZATION_IRR_ELARA | Characterization irregular moon Elara | Working Group 2 |
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| CHARACTERIZATION_IRR2_PASIPHAE | characterization irregular moon Pasiphae | Working Group 2 |
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| CHARACTERIZATION_IRR2_SINOPE | Characterization irregular moon Sinope | Working Group 2 |
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| CHAR_IRR1 | Characterization irregular moons group 1 (see list below) | Working Group 2 |
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| EUROPA_FB_RS | Europa Flyby remote sensing | Working Group 2 |
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| GANYMEDE_FB_RS | Ganymede flyby remote sensing | Working Group 2 |
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| IO_ECLIPSE | Io observation while Io is in eclipse. | Working Group 2 |
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| IO_TOR_DUST | Io torus dust | 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_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_HP | Ring high phase | Working Group 2 |
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| RING_LP | Ring low phase | Working Group 2 |
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| CALLISTO_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
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| EUROPA_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
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| GANYMEDE_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
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| CALLISTO_IONO | CALLISTO_IONO
In situ Callisto ionosphere observation | Working Group 3 |
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| EUROPA_IONO_IS | EUROPA_IONO_IS
In situ Europa ionosphere observation | Working Group 3 |
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| CALLISTO_ENA | Far approach energetic neutral atom imaging of Callisto | Working Group 3 |
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| EUROPA_ENA | Far approach energetic neutral atom imaging of Europa | 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_IONO | GANYMEDE_IONO
In situ Ganymede ionosphere 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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| CALLISTO_WAKE | In situ Callisto wake observation | 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_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_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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| GANYMEDE_GM | In situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environment | Working Group 3 |
|---|
| 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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| INCLINED_NORTH | | Working Group 4 |
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| INCLINED_SOUTH | | Working Group 4 |
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