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_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 |
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_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_TOR_DUST | | 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 |
ASTRO_IRR1_CARPO | ASTRO_IRR1_CARPO | Working Group 2 |
ASTRO_IRR1_CHALDENE | ASTRO_IRR1_CHALDENE | Working Group 2 |
ASTRO_IRR1_HIMALIA | ASTRO_IRR1_HIMALIA | Working Group 2 |
ASTRO_IRR1_KALLICHORE | ASTRO_IRR1_KALLICHORE | Working Group 2 |
ASTRO_IRR1_LEDA | ASTRO_IRR1_LEDA | Working Group 2 |
ASTRO_IRR1_LYSITHEA | ASTRO_IRR1_LYSITHEA | Working Group 2 |
ASTRO_IRR1_MAGACLITE | ASTRO_IRR1_MAGACLITE | Working Group 2 |
ASTRO_IRR1_MEGACLITE | ASTRO_IRR1_MEGACLITE | Working Group 2 |
ASTRO_IRR1_TAYGETE | ASTRO_IRR1_TAYGETE | Working Group 2 |
ASTRO_IRR1_THEMISTO | ASTRO_IRR1_THEMISTO | Working Group 2 |
ASTRO_IRR2_PASIPHAE | astrometry measurement with inertial pointing to moon Pasiphae | Working Group 2 |
RINGMOSAIC_B1.0_B2.0_ph005_ph030 | B between 1 and 2deg
phase between 005 and 030deg | Working Group 2 |
C_RS_10C3 | C_RS_10C3 | Working Group 2 |
C_RS_11C4 | C_RS_11C4 | Working Group 2 |
C_RS_12C5 | C_RS_12C5 | Working Group 2 |
C_RS_13C6 | C_RS_13C6 | Working Group 2 |
C_RS_14C7 | C_RS_14C7 | Working Group 2 |
C_RS_15C8 | C_RS_15C8 | Working Group 2 |
C_RS_16C9 | C_RS_16C9 | Working Group 2 |
C_RS_17C10 | C_RS_17C10 | Working Group 2 |
C_RS_18C11 | C_RS_18C11 | Working Group 2 |
C_RS_19C12 | C_RS_19C12 | Working Group 2 |
C_RS_20C13 | C_RS_20C13 | Working Group 2 |
C_RS_21C14 | C_RS_21C14 | Working Group 2 |
C_RS_22C15 | C_RS_22C15 | Working Group 2 |
C_RS_23C16 | C_RS_23C16 | Working Group 2 |
C_RS_24C17 | C_RS_24C17 | Working Group 2 |
C_RS_25C18 | C_RS_25C18 | Working Group 2 |
C_RS_28C19 | C_RS_28C19 | Working Group 2 |
C_RS_29C20 | C_RS_29C20 | Working Group 2 |
C_RS_31C21 | C_RS_31C21 | Working Group 2 |
C_RS_6C1 | C_RS_6C1 | Working Group 2 |
C_RS_9C2 | C_RS_9C2 | Working Group 2 |
C_RS_OBS | Callisto Remote sensing GENERIC containing obs database link | Working Group 2 |
E_RS_7E1 | E_RS_7E1 | Working Group 2 |
E_RS_8E2 | E_RS_8E2 | Working Group 2 |
E_RS_OBS | Europa remote sensing generic segment containing obs database link | Working Group 2 |
G_RS_OBS | G_RS GENERIC | Working Group 2 |
G_RS_26G6 | G_RS_26G6 | Working Group 2 |
G_RS_27G7 | G_RS_27G7 | Working Group 2 |
G_RS_30G8 | G_RS_30G8 | Working Group 2 |
G_RS_32G9 | G_RS_32G9 | Working Group 2 |
G_RS_33G10 | G_RS_33G10 | Working Group 2 |
G_RS_34G11 | G_RS_34G11 | Working Group 2 |
G_RS_35G12 | G_RS_35G12 | Working Group 2 |
G_RS_3G3 | HAA as per 3GM UM
IS considering NIM | Working Group 2 |
HIGHPHPROFILE_ALTERNATIVE | HIGHPHPROFILE ALTERNATIVE provided by e mail from JANUS team (email from JS on 24/6); alternative times are proposed for this observation that has equally good conditions. Sometimes there is not alternative, sometimes one, sometimes two. | Working Group 2 |
HIGHPHPROFILE | HIGHPHPROFILE, segment identified in absolute time by JANUS team (email from JS on 24/6) | Working Group 2 |
IO_ECLIPSE | Io observation while Io is in eclipse. | Working Group 2 |
IO_MAJ_COMPOSITION | IO_MAJ_COMPOSITION | Working Group 2 |
IO_MAJ_HOTSPOTS | IO_MAJ_HOTSPOTS | Working Group 2 |
J_SAT_505_Ama | J_SAT_505_Ama | Working Group 2 |
J_SAT_506_Him | J_SAT_506_Him | Working Group 2 |
J_SAT_507_Ela | J_SAT_507_Ela | Working Group 2 |
J_SAT_508_Pas | J_SAT_508_Pas | Working Group 2 |
J_SAT_509_Sin | J_SAT_509_Sin | Working Group 2 |
J_SAT_510_Lys | J_SAT_510_Lys | Working Group 2 |
J_SAT_511_Car | J_SAT_511_Car | Working Group 2 |
J_SAT_512_Ana | J_SAT_512_Ana | Working Group 2 |
J_SAT_513_Led | J_SAT_513_Led | Working Group 2 |