| JA_PE6 | | Working Group 4 |
|---|
| JA_PE5 | | Working Group 4 |
|---|
| JA_PE4 | | Working Group 4 |
|---|
| JA_PE3 | | Working Group 4 |
|---|
| JA_PE2 | | Working Group 4 |
|---|
| G_RS_26G11 | | Working Group 2 |
|---|
| G_RS_25G10 | | Working Group 2 |
|---|
| G_RS_24G9 | | Working Group 2 |
|---|
| G_RS_23G8 | | Working Group 2 |
|---|
| G_RS_22G7 | | Working Group 2 |
|---|
| C_RS_21C13 | | Working Group 2 |
|---|
| C_RS_20C12 | | Working Group 2 |
|---|
| C_RS_19C11 | | Working Group 2 |
|---|
| G_RS_18G6 | | Working Group 2 |
|---|
| G_RS_17G5 | | Working Group 2 |
|---|
| C_RS_16C10 | | Working Group 2 |
|---|
| C_RS_15C9 | | Working Group 2 |
|---|
| C_RS_14C8 | | Working Group 2 |
|---|
| C_RS_13C7 | | Working Group 2 |
|---|
| C_RS_12C6 | | Working Group 2 |
|---|
| C_RS_11C5 | | Working Group 2 |
|---|
| C_RS_10C4 | | Working Group 2 |
|---|
| C_RS_9C3 | | Working Group 2 |
|---|
| C_RS_8C2 | | Working Group 2 |
|---|
| E_RS_7E2 | | Working Group 2 |
|---|
| E_RS_6E1 | | Working Group 2 |
|---|
| C_RS_5C1 | | Working Group 2 |
|---|
| G_RS_4G4 | | Working Group 2 |
|---|
| G_RS_3G3 | HAA as per 3GM UM
IS considering NIM | Working Group 2 |
|---|
| G_RS_2G2 | | Working Group 2 |
|---|
| J_AURORA | | Working Group 4 |
|---|
| IO_RS | | Working Group 2 |
|---|
| TOR_RS | | Working Group 3 |
|---|
| J_RING | | Working Group 2 |
|---|
| PR | | WGX |
|---|
| JM_INCL | | Working Group 3 |
|---|
| JM_PE_P4_noDL | | Working Group 3 |
|---|
| JA_PE_MAJIS | | 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_INCL_noDL | created for case 1 | Working Group 4 |
|---|
| JA_PE | | Working Group 4 |
|---|
| 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 |
|---|
| 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 |
|---|
| DL_ | Downlink communication prime segments.
pointing: HGA pointing to Earth | GENERIC |
|---|
| CAL | | WGX |
|---|
| JM_CB | | Working Group 3 |
|---|
| JM_ENA | | Working Group 3 |
|---|
| JM_GM | Jupiter Magnetosphere global monitoring.
Large pointing flexibility, constraints mainly driven by PEP | Working Group 3 |
|---|
| JA_PH | Jupiter Atmosphere prime segment at min-90-max phase.
pointing target is Jupiter although pointing type is TBD (limb, etc) | Working Group 4 |
|---|
| JA_PE_noDL | | Working Group 4 |
|---|
| JA_M | Jupiter Atmosphere Monitoring segments: at regular interval during the tour.
Pointing taregt is Jupiter, although pointing type is TBD (slew scan, raster, nadir etc) | Working Group 4 |
|---|
| JA_INCL | Jupiter Atmosphere Inclined segments: at maximum (Northern) and/or minimum (Southern) latitudes.
Pointing target uis Jupiter although pointing details are TBD (track, limb etc...) | Working Group 4 |
|---|
| 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 |
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| FB_RS | | Working Group 2 |
|---|
| G_IS | | Working Group 3 |
|---|
| G_GPH | | Working Group 1 |
|---|
| G_distant | | Working Group 2 |
|---|
| E_RS | | Working Group 2 |
|---|
| E_IS | | Working Group 3 |
|---|
| E_GPH | | Working Group 1 |
|---|
| E_distant | | Working Group 2 |
|---|
| C_RS | | Working Group 2 |
|---|
| C_IS | | Working Group 3 |
|---|
| C_GPH | | Working Group 1 |
|---|
| C_distant | | Working Group 2 |
|---|