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Description
1
Group
JA_PE44 Working Group 4
JA_PE45 Working Group 4
JA_PE46 Working Group 4
JA_PE47 Working Group 4
JA_PE48 Working Group 4
JA_PE49 Working Group 4
JA_PE5 Working Group 4
JA_PE50 Working Group 4
JA_PE51 Working Group 4
JA_PE52 Working Group 4
JA_PE53 Working Group 4
JA_PE54 Working Group 4
JA_PE55 Working Group 4
JA_PE56 Working Group 4
JA_PE57 Working Group 4
JA_PE58 Working Group 4
JA_PE59 Working Group 4
JA_PE6 Working Group 4
JA_PE60JA_PE60Working Group 4
JA_PE61JA_PE61Working Group 4
JA_PE62JA_PE62Working Group 4
JA_PE63JA_PE63Working Group 4
JA_PE64JA_PE64Working Group 4
JA_PE65JA_PE65Working Group 4
JA_PE66JA_PE66Working Group 4
JA_PE67JA_PE67Working Group 4
JA_PE68JA_PE68Working Group 4
JA_PE69JA_PE69Working Group 4
JA_PE7 Working Group 4
JA_PE8 Working Group 4
JA_PE9 Working Group 4
JA_PH Working Group 4
STAR_OCC Working Group 4
STAR_OCC_OBSSTAR_OCC_OBSWorking Group 4
C_IS Working Group 3
C_IS_OBSC_IS_OBSWorking Group 3
E_IS Working Group 3
E_IS_OBSE_IS_OBSWorking Group 3
G_IS Working Group 3
G_IS_3G3Ganymede in-situ observations around closest approachWorking Group 3
G_IS_4G4 Working Group 3
G_IS_OBSG_IS_OBSWorking Group 3
JM_CB Working Group 3
JM_ENA Working Group 3
JM_GM Working Group 3
JM_INCL Working Group 3
JM_PEassuming: 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_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
JM_PE_P4Perijoves 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_PE13share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE15share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE17share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE19share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE21share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE23share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE25share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE27share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE29share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE31share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE33share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE35 Working Group 3
TOR_RS Working Group 3
C_distant Working Group 2
C_RS Working Group 2
C_RS_10C2test 3_2Working Group 2
C_RS_10C3C_RS_10C3Working Group 2
C_RS_10C4 Working Group 2
C_RS_11C3test 3_2Working Group 2
C_RS_11C4C_RS_11C4Working Group 2
C_RS_11C5 Working Group 2
C_RS_12C4test 3_2Working Group 2
C_RS_12C5C_RS_12C5Working Group 2
C_RS_12C6 Working Group 2
C_RS_13C5test 3_2Working Group 2
C_RS_13C6C_RS_13C6Working Group 2
C_RS_13C7 Working Group 2
C_RS_14C6test 3_2Working Group 2
C_RS_14C7C_RS_14C7Working Group 2
C_RS_14C8 Working Group 2
C_RS_15C7test 3_2Working Group 2
C_RS_15C8C_RS_15C8Working Group 2
C_RS_15C9 Working Group 2
C_RS_16C10 Working Group 2
C_RS_16C8test 3_2Working Group 2
C_RS_16C9C_RS_16C9Working Group 2
C_RS_17C10C_RS_17C10Working Group 2
C_RS_17C9test 3_2Working Group 2
C_RS_18C10test 3_2Working Group 2
C_RS_18C11C_RS_18C11Working Group 2
C_RS_19C11 Working Group 2
C_RS_19C12C_RS_19C12Working Group 2
C_RS_20C12 Working Group 2
C_RS_20C13C_RS_20C13Working Group 2
C_RS_21C13 Working Group 2
C_RS_21C14C_RS_21C14Working Group 2
C_RS_22C11test 3_2Working Group 2
C_RS_22C15C_RS_22C15Working Group 2
C_RS_23C12test 3_2Working Group 2
C_RS_23C16C_RS_23C16Working Group 2

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