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Description
Group
C_RS_5C1 Working Group 2
G_RS_4G4 Working Group 2
G_RS_3G3HAA as per 3GM UM IS considering NIMWorking Group 2
G_RS_2G2 Working Group 2
J_AURORA Working Group 4
IO_RS Working Group 2
TOR_RS Working Group 3
J_RING Working Group 2
PR WGX
JM_INCL Working Group 3
JM_PE_P4_noDL Working Group 3
JA_PE_MAJIS Working Group 4
JA_PE_JANUSIn-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 kbpsWorking Group 4
JA_INCL_noDLcreated for case 1Working Group 4
JA_PE Working Group 4
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
DL_EXTassuming: 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)GENERIC
DL_assuming: JMAG: 2.31 kbps RPWI: 1.7*2.167 kbps (Ballparks numbers from the team) PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018)GENERIC
CAL WGX
JM_CB Working Group 3
JM_ENA Working Group 3
JM_GM Working Group 3
JA_PH Working Group 4
JA_PE_noDL Working Group 4
JA_M Working Group 4
JA_INCL Working Group 4
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
FB_RS Working Group 2
G_IS Working Group 3
G_GPH Working Group 1
G_distant Working Group 2
E_RS Working Group 2
E_IS Working Group 3
E_GPH Working Group 1
E_distant Working Group 2
C_RS Working Group 2
C_IS Working Group 3
C_GPH Working Group 1
C_distant Working Group 2

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