| IO_ECLIPSE | Io observation while Io is in eclipse. | Working Group 2 |
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| ASTRO_IRR1_THEMISTO | ASTRO_IRR1_THEMISTO | Working Group 2 |
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| ASTRO_IRR1_TAYGETE | ASTRO_IRR1_TAYGETE | Working Group 2 |
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| ASTRO_IRR1_MAGACLITE | ASTRO_IRR1_MAGACLITE | Working Group 2 |
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| ASTRO_IRR1_LYSITHEA | ASTRO_IRR1_LYSITHEA | Working Group 2 |
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| ASTRO_IRR1_LEDA | ASTRO_IRR1_LEDA | Working Group 2 |
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| ASTRO_IRR1_KALLICHORE | ASTRO_IRR1_KALLICHORE | Working Group 2 |
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| ASTRO_IRR1_HIMALIA | ASTRO_IRR1_HIMALIA | Working Group 2 |
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| ASTRO_IRR1_CHALDENE | ASTRO_IRR1_CHALDENE | Working Group 2 |
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| ASTRO_IRR1_CARPO | ASTRO_IRR1_CARPO | 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_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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| 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_LP | | Working Group 2 |
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| RING_HP | | Working Group 2 |
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| ASTRO_IRR2_CARME | | Working Group 2 |
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| CHARACTERIZATION_IRR2_ANANKE | | Working Group 2 |
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| ASTRO_IRR2_ANANKE | | Working Group 2 |
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| EUROPA_DISTANT | | Working Group 2 |
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| ASTRO_INNER | | Working Group 2 |
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| CHAR_IRR1 | | Working Group 2 |
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| EUROPA_FB_RS | | Working Group 2 |
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| CALLISTO_FB_RS | | Working Group 2 |
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| GANYMEDE_FB_RS | | 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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| 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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| CHARACTERIZATION_IRR2_PASIPHAE | | Working Group 2 |
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| CHARACTERIZATION_IRR2_SINOPE | | Working Group 2 |
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| CHARACTERIZATION_IRR_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 | | Working Group 2 |
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