| JM_INCL | | 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_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 |
|---|
| G_IS | | Working Group 3 |
|---|
| G_distant | | Working Group 2 |
|---|
| E_RS | | Working Group 2 |
|---|
| E_IS | | Working Group 3 |
|---|
| E_distant | | Working Group 2 |
|---|
| C_IS | | Working Group 3 |
|---|
| C_distant | | Working Group 2 |
|---|