| 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 |
|---|
| JA_PE34 | | Working Group 4 |
|---|
| JA_PE32 | | Working Group 4 |
|---|
| JA_PE30 | | Working Group 4 |
|---|
| JA_PE28 | | Working Group 4 |
|---|
| JA_PE26 | | Working Group 4 |
|---|
| JA_PE24 | | Working Group 4 |
|---|
| JA_PE22 | | Working Group 4 |
|---|
| JA_PE20 | | Working Group 4 |
|---|
| JA_PE18 | | Working Group 4 |
|---|
| JA_PE16 | | Working Group 4 |
|---|
| JA_PE14 | | Working Group 4 |
|---|
| 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 |
|---|
| J_AURORA | | Working Group 4 |
|---|
| 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 |
|---|
| 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 |
|---|
| E_IS_OBS | E_IS_OBS | Working Group 3 |
|---|
| C_IS_OBS | C_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 |
|---|
| G_IS_4G4 | | Working Group 3 |
|---|
| JM_PE35 | | Working Group 3 |
|---|
| 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 |
|---|
| TOR_RS | | Working Group 3 |
|---|
| JM_INCL | | Working Group 3 |
|---|
| JM_PE_P4_noDL | | 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_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 |
|---|
| 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 |
|---|
| G_IS | | Working Group 3 |
|---|
| E_IS | | Working Group 3 |
|---|
| C_IS | | Working Group 3 |
|---|
| G_RS_36G11 | G_RS_36G11 | Working Group 2 |
|---|
| G_RS_35G10 | G_RS_35G10 | Working Group 2 |
|---|
| G_RS_34G9 | G_RS_34G9 | Working Group 2 |
|---|
| G_RS_32G8 | G_RS_32G8 | Working Group 2 |
|---|
| G_RS_28G7 | G_RS_28G7 | Working Group 2 |
|---|
| G_RS_27G6 | G_RS_27G6 | Working Group 2 |
|---|
| C_RS_33C23 | C_RS_33C23 | Working Group 2 |
|---|
| C_RS_31C22 | C_RS_31C22 | Working Group 2 |
|---|
| C_RS_30C21 | | Working Group 2 |
|---|
| C_RS_26C19 | | Working Group 2 |
|---|
| J_SAT_OBS | J_SAT_OBS | Working Group 2 |
|---|
| J_SAT_516_Met | J_SAT_516_Met | Working Group 2 |
|---|
| J_SAT_515_Adr | J_SAT_515_Adr | Working Group 2 |
|---|
| J_SAT_514_The | J_SAT_514_The | Working Group 2 |
|---|
| J_SAT_505_Ama | J_SAT_505_Ama | Working Group 2 |
|---|
| J_SAT_IRR_SEARCH | J_SAT_IRR_SEARCH
discover new irregular moons | Working Group 2 |
|---|
| J_SAT_520_Tay | J_SAT_520_Tay | Working Group 2 |
|---|
| J_SAT_559_17J1 | J_SAT_559_17J1 | Working Group 2 |
|---|
| J_SAT_55503_3J9 | J_SAT_55503_3J9 | Working Group 2 |
|---|
| J_SAT_548_Cyl | J_SAT_548_Cyl | Working Group 2 |
|---|
| J_SAT_566_17J5 | J_SAT_566_17J5 | Working Group 2 |
|---|
| J_SAT_556_11J2 | J_SAT_556_11J2 | Working Group 2 |
|---|
| J_SAT_568_17J7 | J_SAT_568_17J7 | Working Group 2 |
|---|
| J_SAT_569_17J8 | J_SAT_569_17J8 | Working Group 2 |
|---|
| J_SAT_562_Val | J_SAT_562_Val | Working Group 2 |
|---|
| J_SAT_567_17J6 | J_SAT_567_17J6 | Working Group 2 |
|---|
| J_SAT_564_17J3 | J_SAT_564_17J3 | Working Group 2 |
|---|
| J_SAT_543_Arc | J_SAT_543_Arc | Working Group 2 |
|---|
| J_SAT_537_Kle | J_SAT_537_Kle | Working Group 2 |
|---|
| J_SAT_538_Pst | J_SAT_538_Pst | Working Group 2 |
|---|
| J_SAT_554_16J1 | J_SAT_554_16J1 | Working Group 2 |
|---|
| J_SAT_542_Tlx | J_SAT_542_Tlx | Working Group 2 |
|---|
| J_SAT_541_Aoe | J_SAT_541_Aoe | Working Group 2 |
|---|