| CAL | | WGX |
|---|
| PR | | 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 |
|---|
| J_FD_EPHEM_C | | GENERIC |
|---|
| J_FD_EPHEM_E | | GENERIC |
|---|
| J_FD_EPHEM_G | | GENERIC |
|---|
| J_FD_NAV_FB | | GENERIC |
|---|
| J_FD_TCM | | GENERIC |
|---|
| J_FD_WOL | | GENERIC |
|---|
| J_FD_WOL_FB | | GENERIC |
|---|
| OPNAV_CAL | OPNAV_CAL | GENERIC |
|---|
| OPNAV_EUR | OPNAV_EUR | GENERIC |
|---|
| OPNAV_GAN | OPNAV_GAN | GENERIC |
|---|
| SPICE_ATT_GANYMEDE_PHASE | Default attitude during the Ganymede phase | GENERIC |
|---|
| SPICE_ATT_GOTOEARTH_COMMS | Earth communication segment | GENERIC |
|---|
| SPICE_ATT_GOTOJUPITER_TOUR_SUP_SOL_CONJ | Default attitude during superior solar conjunction | GENERIC |
|---|
| SPICE_ATT_GOTOTRANSFER_COLD_SUP_SOL_CONJ | Default attitude during cruise phase superior solar conjunctions 'cold' | GENERIC |
|---|
| SPICE_ATT_JUPITER_TOUR | Default attitude during the Tour phase | GENERIC |
|---|
| SPICE_ATT_TRANSFER_COLD | Default attitude during cruise phase | GENERIC |
|---|
| SPICE_ATT_TRANSFER_HOT | Default attitude during cruise phase applicable during the hot phases | GENERIC |
|---|
| EARTH_OCC | Earth occultation by Jupiter | Working Group 4 |
|---|
| J_AURORA | | Working Group 4 |
|---|
| JA_INCL | | Working Group 4 |
|---|
| JA_INCL_noDL | created for case 1 | Working Group 4 |
|---|
| JA_M | | Working Group 4 |
|---|
| JA_PE | | Working Group 4 |
|---|
| JA_PE_JANUS | In-situ cloned from JA_PE
Remote sensing: cloned from JA_PE removing MAJIS:
JANUS: 55.5*76/(76-8*4)=33.62kbps
SWI: 5.8 kbps
UVS: 2.25 kbps
total: 89.17 kbps | Working Group 4 |
|---|
| JA_PE_MAJIS | | Working Group 4 |
|---|
| JA_PE_noDL | | Working Group 4 |
|---|
| JA_PE_OBS | JA_PE generic for link obs<-> segments | Working Group 4 |
|---|
| JA_PE1 | test 3_2 | Working Group 4 |
|---|
| JA_PE10 | | Working Group 4 |
|---|
| JA_PE11 | | Working Group 4 |
|---|
| JA_PE12 | | Working Group 4 |
|---|
| JA_PE14 | | Working Group 4 |
|---|
| JA_PE16 | | Working Group 4 |
|---|
| JA_PE18 | | Working Group 4 |
|---|
| JA_PE19 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE2 | | Working Group 4 |
|---|
| JA_PE20 | | Working Group 4 |
|---|
| JA_PE21 | JA_PE21 | Working Group 4 |
|---|
| JA_PE22 | | Working Group 4 |
|---|
| JA_PE23 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE24 | | Working Group 4 |
|---|
| JA_PE25 | JA_PE25 | Working Group 4 |
|---|
| JA_PE26 | | Working Group 4 |
|---|
| JA_PE27 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE28 | | Working Group 4 |
|---|
| JA_PE29 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE3 | | Working Group 4 |
|---|
| JA_PE30 | | Working Group 4 |
|---|
| JA_PE31 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE32 | | Working Group 4 |
|---|
| JA_PE33 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE34 | | Working Group 4 |
|---|
| JA_PE35 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE36 | | Working Group 4 |
|---|
| JA_PE37 | | Working Group 4 |
|---|
| JA_PE38 | | Working Group 4 |
|---|
| JA_PE39 | | Working Group 4 |
|---|
| JA_PE4 | | Working Group 4 |
|---|
| JA_PE40 | | Working Group 4 |
|---|
| JA_PE41 | | Working Group 4 |
|---|
| JA_PE42 | | Working Group 4 |
|---|
| JA_PE43 | | Working Group 4 |
|---|
| JA_PE44 | | Working Group 4 |
|---|
| JA_PE45 | | Working Group 4 |
|---|
| JA_PE46 | | Working Group 4 |
|---|
| JA_PE47 | | Working Group 4 |
|---|
| JA_PE48 | | Working Group 4 |
|---|
| JA_PE49 | | Working Group 4 |
|---|
| JA_PE5 | | Working Group 4 |
|---|
| JA_PE50 | | Working Group 4 |
|---|
| JA_PE51 | | Working Group 4 |
|---|
| JA_PE52 | | Working Group 4 |
|---|
| JA_PE53 | | Working Group 4 |
|---|
| JA_PE54 | | Working Group 4 |
|---|
| JA_PE55 | | Working Group 4 |
|---|
| JA_PE56 | | Working Group 4 |
|---|
| JA_PE57 | | Working Group 4 |
|---|
| JA_PE58 | | Working Group 4 |
|---|
| JA_PE59 | | Working Group 4 |
|---|
| JA_PE6 | | Working Group 4 |
|---|
| JA_PE7 | | Working Group 4 |
|---|
| JA_PE8 | | Working Group 4 |
|---|
| JA_PE9 | | Working Group 4 |
|---|
| JA_PH | | Working Group 4 |
|---|
| STAR_OCC | | Working Group 4 |
|---|
| C_IS | | Working Group 3 |
|---|
| E_IS | | Working Group 3 |
|---|
| G_IS | | Working Group 3 |
|---|
| G_IS_4G4 | | Working Group 3 |
|---|
| JM_CB | | Working Group 3 |
|---|
| JM_ENA | | Working Group 3 |
|---|
| JM_GM | | Working Group 3 |
|---|
| JM_INCL | | Working Group 3 |
|---|
| JM_PE | 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) | Working Group 3 |
|---|
| JM_PE_OBS | Jupiter Magnetosphere perijove segments containing link to observations database | Working Group 3 |
|---|
| JM_PE_P4 | Perijoves with WG3 prime (--> 20/09/18: modified (discussion with OW). assuming ~2 times what is produced in G4-G5 scenario (~6.5-7 Gb). Corresponds roughly to 19kbps, copied from JA_INCL)
RS rate assumes no D/L suspension (case 2) | Working Group 3 |
|---|