IO_ECLIPSE | Io observation while Io is in eclipse. | Working Group 2 |
ASTRO_IRR1_THEMISTO | Astrometry irregular moon THEMISTO | Working Group 2 |
ASTRO_IRR1_TAYGETE | Astrometry irregular moon TAYGETE | Working Group 2 |
ASTRO_IRR1_LYSITHEA | Astrometry irregular moon LYSITHEA | Working Group 2 |
ASTRO_IRR1_LEDA | Astrometry irregular moon LEDA | Working Group 2 |
ASTRO_IRR1_KALLICHORE | Astrometry irregular moon KALLICHORE | Working Group 2 |
ASTRO_IRR1_HIMALIA | Astrometry irregular moon HIMALIA | Working Group 2 |
ASTRO_IRR1_CHALDENE | Astrometry irregular moon CHALDENE | Working Group 2 |
ASTRO_IRR1_CARPO | Astrometry irregular moon 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 | Ring low phase | Working Group 2 |
RING_HP | Ring high phase | Working Group 2 |
ASTRO_IRR2_CARME | Astrometry irregular moon Carme | Working Group 2 |
CHARACTERIZATION_IRR2_ANANKE | Characterization irregular moon ANANKE | Working Group 2 |
ASTRO_IRR2_ANANKE | Astrometry irregular moon Ananke | Working Group 2 |
EUROPA_DISTANT | | Working Group 2 |
ASTRO_INNER | Astrometry inner moons | Working Group 2 |
CHAR_IRR1 | Characterization irregular moons group 1 (see list below) | Working Group 2 |
EUROPA_FB_RS | Europa Flyby remote sensing | Working Group 2 |
CALLISTO_FB_RS | Callisto Flyby remote sensing | Working Group 2 |
GANYMEDE_FB_RS | Ganymede flyby remote sensing | 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 | characterization irregular moon Pasiphae | Working Group 2 |
CHARACTERIZATION_IRR2_SINOPE | Characterization irregular moon Sinope | Working Group 2 |
CHARACTERIZATION_IRR_ELARA | Characterization irregular moon 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 | Io torus dust | Working Group 2 |