| 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 |
| 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_PE_OBS | Jupiter Magnetosphere perijove segments containing link to observations database | 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 |
| JM_INCL | | Working Group 3 |
| JM_GM | Jupiter Magnetosphere global monitoring.
Large pointing flexibility, constraints mainly driven by PEP | Working Group 3 |
| JM_ENA | | Working Group 3 |
| JM_CB | | Working Group 3 |
| GANYMEDE_WAKE | In situ Ganymede wake observation | Working Group 3 |
| GANYMEDE_IONO | GANYMEDE_IONO
In situ Ganymede ionosphere observation | Working Group 3 |
| GANYMEDE_GM | In situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environment | Working Group 3 |
| GANYMEDE_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
| GANYMEDE_ENA | Far approach energetic neutral atom imaging of Ganymede | Working Group 3 |
| G_IS_OBS | G_IS_OBS | Working Group 3 |
| G_IS_4G4 | | Working Group 3 |
| G_IS_3G3 | Ganymede in-situ observations around closest approach | Working Group 3 |
| G_IS | | Working Group 3 |
| EUROPA_WAKE | In situ Europa wake observation | Working Group 3 |
| EUROPA_TOR_IS | In situ Europa torus observation | Working Group 3 |
| EUROPA_IONO_IS | EUROPA_IONO_IS
In situ Europa ionosphere observation | Working Group 3 |
| EUROPA_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
| EUROPA_ENA | Far approach energetic neutral atom imaging of Europa | Working Group 3 |
| E_IS_OBS | E_IS_OBS | Working Group 3 |
| E_IS | | Working Group 3 |
| CALLISTO_WAKE | In situ Callisto wake observation | Working Group 3 |
| CALLISTO_IONO | CALLISTO_IONO
In situ Callisto ionosphere observation | Working Group 3 |
| CALLISTO_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
| CALLISTO_ENA | Far approach energetic neutral atom imaging of Callisto | Working Group 3 |
| C_IS_OBS | C_IS_OBS | Working Group 3 |
| C_IS | | Working Group 3 |
| SUN_OCC | Solar occultation by Jupiter, as seen from the SC. | Working Group 4 |
| STAR_OCC_OBS | STAR_OCC_OBS | Working Group 4 |
| STAR_OCC | | Working Group 4 |
| PERIJOVE_TERMINATOR | | Working Group 4 |
| PERIJOVE_NIGHTSIDE | | Working Group 4 |
| PERIJOVE_DAYSIDE | | Working Group 4 |
| JUPITER_PHASE_MIN | | Working Group 4 |
| JUPITER_PHASE_MAX | | Working Group 4 |
| JUPITER_PHASE_165_INC | | Working Group 4 |
| JUPITER_PHASE_165_DEC | | Working Group 4 |
| JUPITER_PHASE_150_INC | | Working Group 4 |
| JUPITER_PHASE_150_DEC | | Working Group 4 |
| JUPITER_PHASE_135_INC | | Working Group 4 |
| JUPITER_PHASE_135_DEC | | Working Group 4 |
| JUPITER_PHASE_120_INC | | Working Group 4 |
| JUPITER_PHASE_120_DEC | | Working Group 4 |
| JUPITER_PHASE_090 | | Working Group 4 |
| JUPITER_PERIJOVE | Jupiter observations | Working Group 4 |
| JUPITER_MONITORING | | Working Group 4 |
| JUPITER_INCLINED_AURORA | | 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_PE9 | | Working Group 4 |
| JA_PE8 | | Working Group 4 |
| JA_PE7 | | Working Group 4 |
| JA_PE69 | JA_PE69 | Working Group 4 |
| JA_PE68 | JA_PE68 | Working Group 4 |
| JA_PE67 | JA_PE67 | Working Group 4 |
| JA_PE66 | JA_PE66 | Working Group 4 |
| JA_PE65 | JA_PE65 | Working Group 4 |
| JA_PE64 | JA_PE64 | Working Group 4 |
| JA_PE63 | JA_PE63 | Working Group 4 |
| JA_PE62 | JA_PE62 | Working Group 4 |
| JA_PE61 | JA_PE61 | Working Group 4 |
| JA_PE60 | JA_PE60 | Working Group 4 |
| JA_PE6 | | Working Group 4 |
| JA_PE59 | | Working Group 4 |
| JA_PE58 | | Working Group 4 |
| JA_PE57 | | Working Group 4 |
| JA_PE56 | | Working Group 4 |
| JA_PE55 | | Working Group 4 |
| JA_PE54 | | Working Group 4 |
| JA_PE53 | | Working Group 4 |
| JA_PE52 | | Working Group 4 |
| JA_PE51 | | Working Group 4 |
| JA_PE50 | | Working Group 4 |
| JA_PE5 | | Working Group 4 |
| JA_PE49 | | Working Group 4 |
| JA_PE48 | | Working Group 4 |
| JA_PE47 | | Working Group 4 |
| JA_PE46 | | Working Group 4 |
| 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_PE4 | | Working Group 4 |
| JA_PE39 | | Working Group 4 |
| JA_PE38 | | Working Group 4 |
| JA_PE37 | | Working Group 4 |
| JA_PE36 | | Working Group 4 |
| JA_PE35 | work around for segmentation scheduler | Working Group 4 |