C_RS_14C6 | test 3_2 | Working Group 2 |
C_RS_13C5 | test 3_2 | Working Group 2 |
C_RS_12C4 | test 3_2 | Working Group 2 |
C_RS_11C3 | test 3_2 | Working Group 2 |
C_RS_10C2 | test 3_2 | 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 |
J_SAT_INN_AST_A | | Working Group 2 |
J_SAT_IRR_AST_E | | Working Group 2 |
J_SAT_INN_CHAR_A | | Working Group 2 |
J_SAT_INN_AST_T | | Working Group 2 |
J_SAT_IRR_CHAR_E | | Working Group 2 |
J_SAT | jupiter satellite GENERIC | Working Group 2 |
G_RS_26G11 | | Working Group 2 |
G_RS_25G10 | | Working Group 2 |
G_RS_24G9 | | Working Group 2 |
G_RS_23G8 | | Working Group 2 |
G_RS_22G7 | | Working Group 2 |
C_RS_21C13 | | Working Group 2 |
C_RS_20C12 | | Working Group 2 |
C_RS_19C11 | | Working Group 2 |
G_RS_18G6 | | Working Group 2 |
G_RS_17G5 | | Working Group 2 |
C_RS_16C10 | | Working Group 2 |
C_RS_15C9 | | Working Group 2 |
C_RS_14C8 | | Working Group 2 |
C_RS_13C7 | | Working Group 2 |
C_RS_12C6 | | Working Group 2 |
C_RS_11C5 | | Working Group 2 |
C_RS_10C4 | | Working Group 2 |
C_RS_9C3 | | Working Group 2 |
C_RS_8C2 | | Working Group 2 |
E_RS_7E2 | | Working Group 2 |
E_RS_6E1 | | Working Group 2 |
C_RS_5C1 | | Working Group 2 |
G_RS_4G4 | | Working Group 2 |
G_RS_3G3 | HAA as per 3GM UM
IS considering NIM | Working Group 2 |
G_RS_2G2 | | Working Group 2 |
ASTRO_INNER | Astrometry inner moons | Working Group 2 |
CHAR_IRR1 | Characterization irregular moons group 1 (see list below) | Working Group 2 |
IO_RS | | Working Group 2 |
J_RING | | 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 |
FB_RS | | Working Group 2 |
G_distant | | Working Group 2 |
E_RS | | Working Group 2 |
E_distant | | Working Group 2 |
C_RS | | Working Group 2 |
C_distant | | 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 |
JUPITER_CP | 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.
CP stands for corotation profile | Working Group 3 |
E_IS_OBS | E_IS_OBS | Working Group 3 |
C_IS_OBS | C_IS_OBS | Working Group 3 |
G_IS_OBS | G_IS_OBS | Working Group 3 |
G_IS_3G3 | Ganymede in-situ observations around closest approach | Working Group 3 |
JM_PE_OBS | Jupiter Magnetosphere perijove segments containing link to observations database | Working Group 3 |
CALLISTO_IONO | CALLISTO_IONO
In situ Callisto ionosphere observation | Working Group 3 |
EUROPA_IONO_IS | EUROPA_IONO_IS
In situ Europa ionosphere observation | Working Group 3 |
GANYMEDE_IONO | GANYMEDE_IONO
In situ Ganymede ionosphere observation | Working Group 3 |
G_IS_4G4 | | Working Group 3 |
JM_PE35 | | Working Group 3 |
JM_PE33 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JM_PE31 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |