G_RS_5G5 | | Working Group 2 |
GANYMEDE_DISTANT | | Working Group 2 |
GANYMEDE_FLYBY_WG2 | | Working Group 2 |
IO_RS | | Working Group 2 |
J_RING | | Working Group 2 |
J_SAT_AITNE | | Working Group 2 |
J_SAT_ANANKE | | Working Group 2 |
J_SAT_AOEDE | | Working Group 2 |
J_SAT_ARCHE | | Working Group 2 |
J_SAT_AUTONOE | | Working Group 2 |
J_SAT_CALLIRRHOE | | Working Group 2 |
J_SAT_CARME | | Working Group 2 |
J_SAT_CARPO | | Working Group 2 |
J_SAT_CHALDENE | | Working Group 2 |
J_SAT_DIA | | Working Group 2 |
J_SAT_EIRENE | | Working Group 2 |
J_SAT_ELARA | | Working Group 2 |
J_SAT_ERINOME | | Working Group 2 |
J_SAT_ERSA | | Working Group 2 |
J_SAT_EUANTHE | | Working Group 2 |
J_SAT_EUKELADE | | Working Group 2 |
J_SAT_EUPHEME | | Working Group 2 |
J_SAT_EUPORIE | | Working Group 2 |
J_SAT_HARPALYKE | | Working Group 2 |
J_SAT_HEGEMONE | | Working Group 2 |
J_SAT_HELIKE | | Working Group 2 |
J_SAT_HERMIPPE | | Working Group 2 |
J_SAT_HERSE | | Working Group 2 |
J_SAT_HIMALIA | | Working Group 2 |
J_SAT_INN_AST_A | | Working Group 2 |
J_SAT_INN_AST_T | | Working Group 2 |
J_SAT_INN_CHAR_A | | Working Group 2 |
J_SAT_IOCASTE | | Working Group 2 |
J_SAT_IRR_AST_E | | Working Group 2 |
J_SAT_IRR_CHAR_E | | Working Group 2 |
J_SAT_ISONOE | | Working Group 2 |
J_SAT_KALE | | Working Group 2 |
J_SAT_KALLICHORE | | Working Group 2 |
J_SAT_KALYKE | | Working Group 2 |
J_SAT_LEDA | | Working Group 2 |
J_SAT_LYSITHEA | | Working Group 2 |
J_SAT_MEGACLITE | | Working Group 2 |
J_SAT_MNEME | | Working Group 2 |
J_SAT_ORTHOSIE | | Working Group 2 |
J_SAT_PANDIA | | Working Group 2 |
J_SAT_PASIPHAE | | Working Group 2 |
J_SAT_PASITHEE | | Working Group 2 |
J_SAT_PHILOPHROSYNE | | Working Group 2 |
J_SAT_PRAXIDIKE | | Working Group 2 |
J_SAT_S2003_J10 | | Working Group 2 |
J_SAT_S2003_J12 | | Working Group 2 |
J_SAT_S2003_J16 | | Working Group 2 |
J_SAT_S2003_J19 | | Working Group 2 |
J_SAT_S2003_J4 | | Working Group 2 |
J_SAT_S2003_J9 | | Working Group 2 |
J_SAT_S2010_J1 | | Working Group 2 |
J_SAT_S2010_J2 | | Working Group 2 |
J_SAT_S2011_J2 | | Working Group 2 |
J_SAT_S2016_J1 | | Working Group 2 |
J_SAT_S2017_J2 | | Working Group 2 |
J_SAT_S2017_J3 | | Working Group 2 |
J_SAT_S2017_J5 | | Working Group 2 |
J_SAT_S2017_J6 | | Working Group 2 |
J_SAT_S2017_J7 | | Working Group 2 |
J_SAT_S2017_J9 | | Working Group 2 |
J_SAT_SINOPE | | Working Group 2 |
J_SAT_TAYGETE | | Working Group 2 |
J_SAT_THEMISTO | | Working Group 2 |
J_SAT_THYONE | | Working Group 2 |
J_SAT_VALETUDO | | Working Group 2 |
RING_PHASECURV_100 | | Working Group 2 |
RING_PHASECURV_110 | | Working Group 2 |
RING_PHASECURV_120 | | Working Group 2 |
RING_PHASECURV_130 | | Working Group 2 |
RING_PHASECURV_140 | | Working Group 2 |
RING_PHASECURV_150 | | Working Group 2 |
RING_PHASECURV_160 | | Working Group 2 |
RING_PHASECURV_170 | | Working Group 2 |
RING_PHASECURV_20 | | Working Group 2 |
RING_PHASECURV_30 | | Working Group 2 |
RING_PHASECURV_40 | | Working Group 2 |
RING_PHASECURV_50 | | Working Group 2 |
RING_PHASECURV_60 | | Working Group 2 |
RING_PHASECURV_70 | | Working Group 2 |
RING_PHASECURV_80 | | Working Group 2 |
RING_PHASECURV_90 | | Working Group 2 |
RINGPHASE | | Working Group 2 |
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_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 |