| 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 |
|---|
| JA_INCL_noDL | created for case 1 | Working Group 4 |
|---|
| EARTH_OCC | Earth occultation by Jupiter | 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_OBS | JA_PE generic for link obs<-> segments | Working Group 4 |
|---|
| JA_PE21 | JA_PE21 | Working Group 4 |
|---|
| JA_PE25 | JA_PE25 | Working Group 4 |
|---|
| JA_PE60 | JA_PE60 | Working Group 4 |
|---|
| JA_PE61 | JA_PE61 | Working Group 4 |
|---|
| JA_PE62 | JA_PE62 | Working Group 4 |
|---|
| JA_PE63 | JA_PE63 | Working Group 4 |
|---|
| JA_PE64 | JA_PE64 | Working Group 4 |
|---|
| JA_PE65 | JA_PE65 | Working Group 4 |
|---|
| JA_PE66 | JA_PE66 | Working Group 4 |
|---|
| JA_PE67 | JA_PE67 | Working Group 4 |
|---|
| JA_PE68 | JA_PE68 | Working Group 4 |
|---|
| JA_PE69 | JA_PE69 | Working Group 4 |
|---|
| STAR_OCC_OBS | STAR_OCC_OBS | Working Group 4 |
|---|
| JA_PE1 | test 3_2 | Working Group 4 |
|---|
| JA_PE19 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE23 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE27 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE29 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE31 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE33 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE35 | work around for segmentation scheduler | Working Group 4 |
|---|
| JA_PE13 | work-aroudn for aegmentation scheduler | Working Group 4 |
|---|
| JA_PE15 | work-aroudn for aegmentation scheduler | Working Group 4 |
|---|
| JA_PE17 | work-around for segmentation scheduler | 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_P4_noDL | | Working Group 3 |
|---|
| JM_PE35 | | Working Group 3 |
|---|
| TOR_RS | | 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 |
|---|
| C_IS_OBS | C_IS_OBS | Working Group 3 |
|---|
| E_IS_OBS | E_IS_OBS | Working Group 3 |
|---|
| G_IS_OBS | G_IS_OBS | Working Group 3 |
|---|
| G_IS_3G3 | Ganymede in-situ observations around closest approach | 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 |
|---|
| JM_PE13 | 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_PE17 | 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_PE21 | 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_PE25 | 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_PE29 | 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_PE33 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| C_distant | | Working Group 2 |
|---|
| C_RS | | Working Group 2 |
|---|
| C_RS_10C4 | | Working Group 2 |
|---|
| C_RS_11C5 | | Working Group 2 |
|---|
| C_RS_12C6 | | Working Group 2 |
|---|
| C_RS_13C7 | | Working Group 2 |
|---|
| C_RS_14C8 | | Working Group 2 |
|---|
| C_RS_15C9 | | Working Group 2 |
|---|
| C_RS_16C10 | | Working Group 2 |
|---|
| C_RS_19C11 | | Working Group 2 |
|---|
| C_RS_20C12 | | Working Group 2 |
|---|
| C_RS_21C13 | | Working Group 2 |
|---|
| C_RS_26C19 | | Working Group 2 |
|---|
| C_RS_30C21 | | Working Group 2 |
|---|
| C_RS_5C1 | | Working Group 2 |
|---|
| C_RS_8C2 | | Working Group 2 |
|---|
| C_RS_9C3 | | Working Group 2 |
|---|
| E_distant | | Working Group 2 |
|---|
| E_RS | | Working Group 2 |
|---|
| E_RS_6E1 | | Working Group 2 |
|---|
| E_RS_7E2 | | Working Group 2 |
|---|
| FB_RS | | Working Group 2 |
|---|
| G_distant | | Working Group 2 |
|---|
| G_RS_17G5 | | Working Group 2 |
|---|
| G_RS_18G6 | | Working Group 2 |
|---|
| G_RS_1G1 | | Working Group 2 |
|---|
| G_RS_22G7 | | Working Group 2 |
|---|
| G_RS_23G8 | | Working Group 2 |
|---|
| G_RS_24G9 | | Working Group 2 |
|---|
| G_RS_25G10 | | Working Group 2 |
|---|
| G_RS_26G11 | | Working Group 2 |
|---|
| G_RS_2G2 | | Working Group 2 |
|---|
| G_RS_4G4 | | Working Group 2 |
|---|
| G_RS_5G5 | | Working Group 2 |
|---|
| IO_RS | | Working Group 2 |
|---|
| J_RING | | Working Group 2 |
|---|
| J_SAT_AITNE | | Working Group 2 |
|---|