C_RS_20C13 | C_RS_20C13 | Working Group 2 |
C_RS_19C12 | C_RS_19C12 | Working Group 2 |
C_RS_18C11 | C_RS_18C11 | Working Group 2 |
C_RS_17C10 | C_RS_17C10 | Working Group 2 |
C_RS_16C9 | C_RS_16C9 | Working Group 2 |
C_RS_15C8 | C_RS_15C8 | Working Group 2 |
C_RS_14C7 | C_RS_14C7 | Working Group 2 |
C_RS_13C6 | C_RS_13C6 | Working Group 2 |
C_RS_12C5 | C_RS_12C5 | Working Group 2 |
C_RS_11C4 | C_RS_11C4 | Working Group 2 |
C_RS_10C3 | C_RS_10C3 | Working Group 2 |
C_RS_9C2 | C_RS_9C2 | Working Group 2 |
C_RS_6C1 | C_RS_6C1 | Working Group 2 |
E_RS_8E2 | E_RS_8E2 | Working Group 2 |
E_RS_7E1 | E_RS_7E1 | Working Group 2 |
G_RS_35G12 | G_RS_35G12 | Working Group 2 |
G_RS_34G11 | G_RS_34G11 | Working Group 2 |
G_RS_33G10 | G_RS_33G10 | Working Group 2 |
G_RS_32G9 | G_RS_32G9 | Working Group 2 |
G_RS_30G8 | G_RS_30G8 | Working Group 2 |
G_RS_27G7 | G_RS_27G7 | Working Group 2 |
G_RS_26G6 | G_RS_26G6 | Working Group 2 |
G_RS_1G1 | | Working Group 2 |
G_RS_5G5 | | 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 |
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_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 | | Working Group 2 |
CHAR_IRR1 | | Working Group 2 |
IO_RS | | Working Group 2 |
J_RING | | Working Group 2 |
EUROPA_FB_RS | | Working Group 2 |
CALLISTO_FB_RS | | Working Group 2 |
GANYMEDE_FB_RS | | Working Group 2 |
G_distant | | Working Group 2 |
E_RS | | Working Group 2 |
E_distant | | 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 | | 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 |
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
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 |
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 |
JM_PE29 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JM_PE27 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JM_PE25 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JM_PE23 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JM_PE21 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JM_PE19 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JM_PE17 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |