| TOR_RS | | Working Group 3 |
| SWI_PRIME_OBSERVATION | | SWI |
| STAR_OCC | | Working Group 4 |
| SOC_OBSERVATION | | SOC |
| RIME_PRIME_OBSERVATION | | RIME |
| PR | | WGX |
| JM_PE35 | | Working Group 3 |
| JM_INCL | | Working Group 3 |
| JM_ENA | | Working Group 3 |
| JM_CB | | Working Group 3 |
| JA_PE9 | | Working Group 4 |
| JA_PE8 | | Working Group 4 |
| JA_PE7 | | Working Group 4 |
| JA_PE6 | | Working Group 4 |
| JA_PE59 | | Working Group 4 |
| JA_PE58 | | Working Group 4 |
| JA_PE57 | | Working Group 4 |
| JA_PE56 | | Working Group 4 |
| JA_PE55 | | Working Group 4 |
| JA_PE54 | | Working Group 4 |
| JA_PE53 | | Working Group 4 |
| JA_PE52 | | Working Group 4 |
| JA_PE51 | | Working Group 4 |
| JA_PE50 | | Working Group 4 |
| JA_PE5 | | Working Group 4 |
| JA_PE49 | | Working Group 4 |
| JA_PE48 | | Working Group 4 |
| JA_PE47 | | Working Group 4 |
| JA_PE46 | | Working Group 4 |
| JA_PE45 | | Working Group 4 |
| JA_PE44 | | Working Group 4 |
| JA_PE43 | | Working Group 4 |
| JA_PE42 | | Working Group 4 |
| JA_PE41 | | Working Group 4 |
| JA_PE40 | | Working Group 4 |
| JA_PE4 | | Working Group 4 |
| JA_PE39 | | Working Group 4 |
| JA_PE38 | | Working Group 4 |
| JA_PE37 | | Working Group 4 |
| JA_PE36 | | Working Group 4 |
| JA_PE34 | | Working Group 4 |
| JA_PE32 | | Working Group 4 |
| JA_PE30 | | Working Group 4 |
| JA_PE3 | | Working Group 4 |
| JA_PE28 | | Working Group 4 |
| JA_PE26 | | Working Group 4 |
| JA_PE24 | | Working Group 4 |
| JA_PE22 | | Working Group 4 |
| JA_PE20 | | Working Group 4 |
| JA_PE2 | | Working Group 4 |
| JA_PE18 | | Working Group 4 |
| JA_PE16 | | Working Group 4 |
| JA_PE14 | | Working Group 4 |
| JA_PE12 | | Working Group 4 |
| JA_PE11 | | Working Group 4 |
| JA_PE10 | | Working Group 4 |
| J_RING | | Working Group 2 |
| J_AURORA | | Working Group 4 |
| IO_RS | | Working Group 2 |
| G_RS_5G5 | | Working Group 2 |
| G_RS_4G4 | | Working Group 2 |
| G_RS_2G2 | | Working Group 2 |
| G_RS_1G1 | | Working Group 2 |
| G_IS | | Working Group 3 |
| G_GPH_2G2 | | Working Group 1 |
| G_distant | | Working Group 2 |
| E_RS | | Working Group 2 |
| E_IS | | Working Group 3 |
| E_distant | | Working Group 2 |
| CAL | | WGX |
| C_RS_30C21 | | Working Group 2 |
| C_RS_26C19 | | Working Group 2 |
| C_IS | | Working Group 3 |
| C_GPH_17C10 | | Working Group 1 |
| C_distant | | Working Group 2 |
| 3GM_OBSERVATION | | 3GM |
| CALIB | all calibrations activities to be included as part of the segmentation (e.g. calibration roll etc...) | WGX |
| 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 |
| ECLIPSE_BATTERY_RECOVERY_STANDARD | Battery recharge after eclipse
pointing should be default power optimised pointing | GENERIC |
| ECLIPSE_BATTERY_RECOVERY_FAST | Battery recharge after eclipse | GENERIC |
| 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
Geophysics prime segment, defined based on GALA (transmitting) operational range of altitude above Callisto < 2000 km.
Assumed Nadir pointing | Working Group 1 |
| C_GPH_18C11 | C_GPH_18C11 | Working Group 1 |
| C_GPH_19C12 | C_GPH_19C12 | 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_26C19 | C_GPH_26C19 | Working Group 1 |
| C_GPH_29C20 | C_GPH_29C20 | Working Group 1 |
| 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 |