| 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_PE39 | | Working Group 4 |
|---|
| JA_PE38 | | Working Group 4 |
|---|
| JA_PE37 | | Working Group 4 |
|---|
| JA_PE36 | | Working Group 4 |
|---|
| JM_PE35 | | Working Group 3 |
|---|
| JA_PE34 | | Working Group 4 |
|---|
| JM_PE33 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE32 | | Working Group 4 |
|---|
| JM_PE31 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE30 | | Working Group 4 |
|---|
| JM_PE29 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE28 | | Working Group 4 |
|---|
| JM_PE27 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE26 | | Working Group 4 |
|---|
| JM_PE25 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE24 | | Working Group 4 |
|---|
| JM_PE23 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE22 | | Working Group 4 |
|---|
| JM_PE21 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE20 | | Working Group 4 |
|---|
| JM_PE19 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE18 | | Working Group 4 |
|---|
| JM_PE17 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE16 | | Working Group 4 |
|---|
| JM_PE15 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE14 | | Working Group 4 |
|---|
| JM_PE13 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JA_PE12 | | Working Group 4 |
|---|
| JA_PE11 | | Working Group 4 |
|---|
| JA_PE10 | | Working Group 4 |
|---|
| JA_PE9 | | Working Group 4 |
|---|
| JA_PE8 | | Working Group 4 |
|---|
| JA_PE7 | | Working Group 4 |
|---|
| 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 |
|---|
| JA_PE | | Working Group 4 |
|---|
| 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_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 |
|---|
| 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 |
|---|