C_IS | | Working Group 3 |
C_IS_OBS | C_IS_OBS | Working Group 3 |
E_IS | | Working Group 3 |
E_IS_OBS | E_IS_OBS | Working Group 3 |
G_IS | | Working Group 3 |
G_IS_3G3 | Ganymede in-situ observations around closest approach | Working Group 3 |
G_IS_4G4 | | Working Group 3 |
G_IS_OBS | G_IS_OBS | 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_INCL | | 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_PE_OBS | Jupiter Magnetosphere perijove segments containing link to observations database | 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_P4_noDL | | Working Group 3 |
JM_PE13 | 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_PE17 | 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_PE21 | 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_PE25 | 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_PE29 | 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_PE33 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JM_PE35 | | Working Group 3 |
TOR_RS | | Working Group 3 |