GANYMEDE_FLYBY_UVS | | Working Group 1 |
EUROPA_FLYBY_RIME_AJS | | Working Group 1 |
CALLISTO_FLYBY | | Working Group 1 |
CALLISTO_FLYBY_3GM | | Working Group 1 |
CALLISTO_FLYBY_GALA | | Working Group 1 |
CALLISTO_FLYBY_JANUS | | Working Group 1 |
CALLISTO_FLYBY_MAJIS | | Working Group 1 |
CALLISTO_FLYBY_RIME_AJS | | Working Group 1 |
CALLISTO_FLYBY_RIME_JS | | Working Group 1 |
CALLISTO_RPWI_PASSIVRAD | | Working Group 1 |
EUROPA_FLYBY | | Working Group 1 |
EUROPA_FLYBY_3GM | | Working Group 1 |
EUROPA_FLYBY_GALA | | Working Group 1 |
EUROPA_FLYBY_JANUS | | Working Group 1 |
EUROPA_FLYBY_MAJIS | | Working Group 1 |
EUROPA_FLYBY_RIME_JS | | Working Group 1 |
EUROPA_RPWI_PASSIVRAD | | Working Group 1 |
GANYMEDE_FLYBY | | Working Group 1 |
GANYMEDE_FLYBY_3GM | | Working Group 1 |
GANYMEDE_FLYBY_GALA | | Working Group 1 |
GANYMEDE_FLYBY_JANUS | | Working Group 1 |
GANYMEDE_FLYBY_MAJIS | | Working Group 1 |
GANYMEDE_FLYBY_RIME_AJS | | Working Group 1 |
GANYMEDE_FLYBY_RIME_JS | | Working Group 1 |
GANYMEDE_RPWI_PASSIVRAD | | Working Group 1 |
IO_ECLIPSE | Io observation while Io is in eclipse. | Working Group 2 |
ASTRO_IRR1_THEMISTO | ASTRO_IRR1_THEMISTO | Working Group 2 |
ASTRO_IRR1_TAYGETE | ASTRO_IRR1_TAYGETE | Working Group 2 |
ASTRO_IRR1_MAGACLITE | ASTRO_IRR1_MAGACLITE | Working Group 2 |
ASTRO_IRR1_LYSITHEA | ASTRO_IRR1_LYSITHEA | Working Group 2 |
ASTRO_IRR1_LEDA | ASTRO_IRR1_LEDA | Working Group 2 |
ASTRO_IRR1_KALLICHORE | ASTRO_IRR1_KALLICHORE | Working Group 2 |
ASTRO_IRR1_HIMALIA | ASTRO_IRR1_HIMALIA | Working Group 2 |
ASTRO_IRR1_CHALDENE | ASTRO_IRR1_CHALDENE | Working Group 2 |
ASTRO_IRR1_CARPO | ASTRO_IRR1_CARPO | Working Group 2 |
RING_PHASECURV_170 | | Working Group 2 |
RING_PHASECURV_160 | | Working Group 2 |
RING_PHASECURV_150 | | Working Group 2 |
RING_PHASECURV_140 | | Working Group 2 |
RING_PHASECURV_130 | | Working Group 2 |
RING_PHASECURV_120 | | Working Group 2 |
RING_PHASECURV_110 | | Working Group 2 |
RING_PHASECURV_100 | | Working Group 2 |
RING_PHASECURV_90 | | Working Group 2 |
RING_PHASECURV_80 | | Working Group 2 |
RING_PHASECURV_70 | | Working Group 2 |
RING_PHASECURV_60 | | Working Group 2 |
RING_PHASECURV_50 | | Working Group 2 |
RING_PHASECURV_40 | | Working Group 2 |
RING_PHASECURV_30 | | Working Group 2 |
RING_PHASECURV_20 | | Working Group 2 |
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 |
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 |
RING_LP | | Working Group 2 |
RING_HP | | Working Group 2 |
ASTRO_IRR2_CARME | | Working Group 2 |
CHARACTERIZATION_IRR2_ANANKE | | Working Group 2 |
ASTRO_IRR2_ANANKE | | Working Group 2 |
EUROPA_DISTANT | | Working Group 2 |
ASTRO_INNER | | Working Group 2 |
CHAR_IRR1 | | Working Group 2 |
EUROPA_FB_RS | | Working Group 2 |
CALLISTO_FB_RS | | Working Group 2 |
GANYMEDE_FB_RS | | Working Group 2 |
ASTRO_IRR2_PASIPHAE | astrometry measurement with inertial pointing to moon Pasiphae | Working Group 2 |
ASTRO_IRR2_SINOPE | | Working Group 2 |
ASTRO_IRR_ELARA | | Working Group 2 |
CALLISTO_DISTANT | | Working Group 2 |
CALLISTO_FLYBY_WG2 | | Working Group 2 |
CHARACTERIZATION_IRR2_CARME | | Working Group 2 |
CHARACTERIZATION_IRR2_PASIPHAE | | Working Group 2 |
CHARACTERIZATION_IRR2_SINOPE | | Working Group 2 |
CHARACTERIZATION_IRR_ELARA | | Working Group 2 |
EUROPA_FLYBY_WG2 | | Working Group 2 |
GANYMEDE_DISTANT | | Working Group 2 |
GANYMEDE_FLYBY_WG2 | | Working Group 2 |
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 |
IO_TOR_DUST | | Working Group 2 |
CALLISTO_IONO | CALLISTO_IONO
Implementation in Geopipeline:
Altitude to Callisto lower than 450 km | Working Group 3 |
EUROPA_IONO_IS | EUROPA_IONO_IS
Implementation in geopipeline:
10 mn before and after closest approach | Working Group 3 |
GANYMEDE_IONO | GANYMEDE_IONO
Implementation in geopipeline:
Altitude below 450 km | Working Group 3 |
CALLISTO_ENA | | Working Group 3 |
CALLISTO_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
CALLISTO_WAKE | | Working Group 3 |
EUROPA_ENA | | Working Group 3 |
EUROPA_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
EUROPA_TOR_IS | | Working Group 3 |
EUROPA_WAKE | | Working Group 3 |
GANYMEDE_ENA | | Working Group 3 |
GANYMEDE_GM | | Working Group 3 |
GANYMEDE_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
GANYMEDE_WAKE | | Working Group 3 |
JUPITER_CB | | Working Group 3 |
JUPITER_CPS | Current plasma sheet crossing | Working Group 3 |
JUPITER_ENA | | Working Group 3 |
JUPITER_GM | | Working Group 3 |
JUPITER_NULL | | Working Group 3 |
JUPITER_PDT | | Working Group 3 |
JUPITER_TAIL | | Working Group 3 |
EARTH_OCC_EGRESS | | Working Group 4 |