C_distant | | Working Group 2 |
C_GPH_10C3 | C_GPH_10C3 | Working Group 1 |
C_GPH_11C4 | C_GPH_11C4 | Working Group 1 |
C_GPH_12C5 | C_GPH_12C5 | Working Group 1 |
C_GPH_13C6 | C_GPH_13C6 | Working Group 1 |
C_GPH_14C7 | C_GPH_14C7 | Working Group 1 |
C_GPH_15C8 | C_GPH_15C8 | Working Group 1 |
C_GPH_16C9 | C_GPH_16C9 | Working Group 1 |
C_GPH_18C11 | C_GPH_18C11 | Working Group 1 |
C_GPH_19C12 | C_GPH_19C12 | Working Group 1 |
C_GPH_20C13 | C_GPH_20C13 | Working Group 1 |
C_GPH_21C14 | C_GPH_21C14 | Working Group 1 |
C_GPH_22C15 | C_GPH_22C15 | Working Group 1 |
C_GPH_23C16 | C_GPH_23C13 | Working Group 1 |
C_GPH_24C17 | C_GPH_24C17 | Working Group 1 |
C_GPH_25C18 | C_GPH_25C18 | Working Group 1 |
C_GPH_28C19 | C_GPH_28C19 | Working Group 1 |
C_GPH_OBS | Callisto geophysics generic containing obs database link | Working Group 1 |
C_IS | | Working Group 3 |
C_IS_OBS | C_IS_OBS | Working Group 3 |
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 |
CAL | | WGX |
DL_ | assuming:
JMAG: 2.31 kbps
RPWI: 1.7*2.167 kbps (Ballparks numbers from the team)
PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018) | GENERIC |
DL_EXT | assuming:
JMAG: 2.31 kbps
RPWI: 1.7*2.167 kbps
PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018) | GENERIC |
E_distant | | Working Group 2 |
E_GPH | | Working Group 1 |
E_GPH_7E1 | E_GPH_7E1 | Working Group 1 |
E_GPH_8E2 | E_GPH_8E2 | Working Group 1 |
E_GPH_OBS | Europa geophysics generic containing obs database link | Working Group 1 |
E_IS | | Working Group 3 |
E_IS_OBS | E_IS_OBS | Working Group 3 |
E_RS | | 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 |
EARTH_OCC | Earth occultation by Jupiter | Working Group 4 |
G_distant | | Working Group 2 |
G_GPH_1G1 | test 3_2 | Working Group 1 |
G_GPH_26G6 | G_GPH_26G6 | Working Group 1 |
G_GPH_2G2 | | Working Group 1 |
G_GPH_3G3 | G_GPH_3G3 | Working Group 1 |
G_GPH_5G5 | G_GPH_5G5 | Working Group 1 |
G_GPH_OBS | Generic G_GPH containing link to obs def | Working Group 1 |
G_IS | | Working Group 3 |
G_IS_3G3 | Ganymede in-situ observations around closest approach | Working Group 3 |
G_IS_OBS | G_IS_OBS | Working Group 3 |
G_RS_1G1 | | Working Group 2 |
G_RS_26G6 | G_RS_26G6 | Working Group 2 |
G_RS_27G7 | G_RS_27G7 | Working Group 2 |
G_RS_2G2 | | 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 |
G_RS_4G4 | | Working Group 2 |
G_RS_5G5 | | Working Group 2 |
G_RS_OBS | G_RS GENERIC | Working Group 2 |
IO_RS | | Working Group 2 |
J_AURORA | | Working Group 4 |
J_FD_TCM | | GENERIC |
J_FD_WOL | | GENERIC |
J_FD_WOL_FB | | GENERIC |
J_RING | | Working Group 2 |
J_SAT | jupiter satellite GENERIC | 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 |
J_SAT_514_The | J_SAT_514_The | Working Group 2 |
J_SAT_515_Adr | J_SAT_515_Adr | Working Group 2 |
J_SAT_516_Met | J_SAT_516_Met | Working Group 2 |
J_SAT_517_Clh | J_SAT_517_Clh | Working Group 2 |