JA_PE35 | work around for segmentation scheduler | Working Group 4 |
JA_PE33 | work around for segmentation scheduler | Working Group 4 |
JA_PE31 | work around for segmentation scheduler | Working Group 4 |
JA_PE29 | work around for segmentation scheduler | Working Group 4 |
JA_PE27 | work around for segmentation scheduler | Working Group 4 |
JA_PE23 | work around for segmentation scheduler | Working Group 4 |
JA_PE19 | work around for segmentation scheduler | Working Group 4 |
G_GPH_1G1 | test 3_2 | Working Group 1 |
JA_PE1 | test 3_2 | Working Group 4 |
G_RS_9G6 | test 3_2 | Working Group 2 |
G_RS_26G12 | test 3_2 | Working Group 2 |
G_RS_24G10 | test 3_2 | Working Group 2 |
G_RS_21G9 | test 3_2 | Working Group 2 |
G_RS_20G8 | test 3_2 | Working Group 2 |
G_RS_19G7 | test 3_2 | Working Group 2 |
C_RS_8C1 | test 3_2 | Working Group 2 |
C_RS_23C12 | test 3_2 | Working Group 2 |
C_RS_22C11 | test 3_2 | Working Group 2 |
C_RS_18C10 | test 3_2 | Working Group 2 |
C_RS_17C9 | test 3_2 | Working Group 2 |
C_RS_16C8 | test 3_2 | Working Group 2 |
C_RS_15C7 | test 3_2 | Working Group 2 |
C_RS_14C6 | test 3_2 | Working Group 2 |
C_RS_13C5 | test 3_2 | Working Group 2 |
C_RS_12C4 | test 3_2 | Working Group 2 |
C_RS_11C3 | test 3_2 | Working Group 2 |
C_RS_10C2 | test 3_2 | Working Group 2 |
C_GPH_8C1 | test 3_2 | Working Group 1 |
C_GPH_22C11 | test 3_2 | Working Group 1 |
C_GPH_18C10 | test 3_2 | Working Group 1 |
C_GPH_16C8 | test 3_2 | Working Group 1 |
C_GPH_14C6 | test 3_2 | Working Group 1 |
C_GPH_13C5 | test 3_2 | Working Group 1 |
C_GPH_12C4 | Test 3_2 | Working Group 1 |
C_GPH_11C3 | test 3_2 | Working Group 1 |
C_GPH_10C2 | test 3_2 | Working Group 1 |
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 |
JM_PE15 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JM_PE13 | share prime high lat PJ between WG3 and WG4 | 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 |
OPNAV_GAN | OPNAV_GAN | GENERIC |
OPNAV_EUR | OPNAV_EUR | GENERIC |
OPNAV_CAL | OPNAV_CAL | GENERIC |
J_SAT | jupiter satellite GENERIC | Working Group 2 |
JM_PE_OBS | Jupiter Magnetosphere perijove segments containing link to observations database | Working Group 3 |
JA_PE25 | JA_PE25 | Working Group 4 |
JA_PE21 | JA_PE21 | Working Group 4 |
JA_PE_OBS | JA_PE generic for link obs<-> segments | 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 |
G_RS_3G3 | HAA as per 3GM UM
IS considering NIM | Working Group 2 |
G_GPH_OBS | Generic G_GPH containing link to obs def | Working Group 1 |
G_RS_OBS | G_RS GENERIC | Working Group 2 |
E_RS_OBS | Europa remote sensing generic segment containing obs database link | Working Group 2 |
E_GPH_OBS | Europa geophysics generic containing obs database link | Working Group 1 |
EARTH_OCC | Earth occultation by Jupiter | Working Group 4 |
SPICE_ATT_GOTOEARTH_COMMS | Earth communication segment | GENERIC |
SPICE_ATT_JUPITER_TOUR | Default attitude during the Tour phase | GENERIC |
SPICE_ATT_GANYMEDE_PHASE | Default attitude during the Ganymede phase | 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_TRANSFER_HOT | Default attitude during cruise phase applicable during the hot phases | GENERIC |
SPICE_ATT_TRANSFER_COLD | Default attitude during cruise phase | GENERIC |
C_GPH_15C7 | crema 3_2 | Working Group 1 |
JA_INCL_noDL | created for case 1 | Working Group 4 |
C_RS_OBS | Callisto Remote sensing GENERIC containing obs database link | Working Group 2 |
C_GPH_OBS | Callisto geophysics generic containing obs database link | Working Group 1 |
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 |
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 |
J_SAT_VALETUDO | | Working Group 2 |
J_SAT_THEMISTO | | Working Group 2 |
J_SAT_TAYGETE | | Working Group 2 |
J_SAT_SINOPE | | Working Group 2 |
J_SAT_PRAXIDIKE | | Working Group 2 |
J_SAT_PASITHEE | | Working Group 2 |
J_SAT_PASIPHAE | | Working Group 2 |
J_SAT_PANDIA | | Working Group 2 |
J_SAT_MEGACLITE | | Working Group 2 |
J_SAT_LYSITHEA | | Working Group 2 |
J_SAT_LEDA | | Working Group 2 |
J_SAT_KALLICHORE | | Working Group 2 |
J_SAT_ISONOE | | Working Group 2 |
J_SAT_IOCASTE | | Working Group 2 |
J_SAT_HIMALIA | | Working Group 2 |
J_SAT_HERSE | | Working Group 2 |
J_SAT_HERMIPPE | | Working Group 2 |
J_SAT_HELIKE | | Working Group 2 |
J_SAT_HEGEMONE | | Working Group 2 |
J_SAT_HARPALYKE | | Working Group 2 |
J_SAT_ERSA | | Working Group 2 |
J_SAT_ERINOME | | Working Group 2 |
J_SAT_ELARA | | Working Group 2 |