Home › Core › Segment definitions

Select segment definition to view

Mnemonic
Description
Group
RING_PHASECURV_70 Working Group 2
RING_PHASECURV_60 Working Group 2
RING_PHASECURV_50 Working Group 2
RING_PHASECURV_40 Working Group 2
RING_PHASECURV_30 Working Group 2
RING_PHASECURV_20 Working Group 2
RING_PHASECURV_10Opportunity implementation in geopipeline SC distance to Jupiter larger than 8e5 km SC elevation above the rings lower than 0.5 deg Only one Ansae tested for phase conditions - value must be between 10 deg and 20 degWorking Group 2
RING_PHASECURV_5Opportunity implementation in geopipeline SC distance to Jupiter larger than 8e5 km SC elevation above the rings lower than 0.5 deg Only one Ansae tested for phase conditions - value must be between 5 deg and 10 degWorking Group 2
RING_LPRing low phaseWorking Group 2
RING_HPRing high phaseWorking Group 2
ASTRO_IRR2_CARMEAstrometry irregular moon CarmeWorking Group 2
CHARACTERIZATION_IRR2_ANANKECharacterization irregular moon ANANKEWorking Group 2
ASTRO_IRR2_ANANKEAstrometry irregular moon AnankeWorking Group 2
EUROPA_DISTANT Working Group 2
J_SAT_INN_AST_A Working Group 2
J_SAT_IRR_AST_E Working Group 2
J_SAT_INN_CHAR_A Working Group 2
J_SAT_INN_AST_T Working Group 2
J_SAT_IRR_CHAR_E Working Group 2
J_SATjupiter satellite GENERICWorking Group 2
G_RS_26G11 Working Group 2
G_RS_25G10 Working Group 2
G_RS_24G9 Working Group 2
G_RS_23G8 Working Group 2
G_RS_22G7 Working Group 2
C_RS_21C13 Working Group 2
C_RS_20C12 Working Group 2
C_RS_19C11 Working Group 2
G_RS_18G6 Working Group 2
G_RS_17G5 Working Group 2
C_RS_16C10 Working Group 2
C_RS_15C9 Working Group 2
C_RS_14C8 Working Group 2
C_RS_13C7 Working Group 2
C_RS_12C6 Working Group 2
C_RS_11C5 Working Group 2
C_RS_10C4 Working Group 2
C_RS_9C3 Working Group 2
C_RS_8C2 Working Group 2
E_RS_7E2 Working Group 2
E_RS_6E1 Working Group 2
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
ASTRO_INNERAstrometry inner moonsWorking Group 2
CHAR_IRR1Characterization irregular moons group 1 (see list below)Working Group 2
IO_RS Working Group 2
J_RING Working Group 2
EUROPA_FB_RSEuropa Flyby remote sensingWorking Group 2
CALLISTO_FB_RSCallisto Flyby remote sensingWorking Group 2
GANYMEDE_FB_RSGanymede flyby remote sensingWorking Group 2
FB_RS Working Group 2
G_distant Working Group 2
E_RS Working Group 2
E_distant Working Group 2
C_RS Working Group 2
C_distant Working Group 2
ASTRO_IRR2_PASIPHAEastrometry measurement with inertial pointing to moon PasiphaeWorking Group 2
ASTRO_IRR2_SINOPE Working Group 2
ASTRO_IRR_ELARA Working Group 2
CALLISTO_DISTANT Working Group 2
CALLISTO_FLYBY_WG2 Working Group 2
CHARACTERIZATION_IRR2_CARME Working Group 2
CHARACTERIZATION_IRR2_PASIPHAEcharacterization irregular moon PasiphaeWorking Group 2
CHARACTERIZATION_IRR2_SINOPECharacterization irregular moon SinopeWorking Group 2
CHARACTERIZATION_IRR_ELARACharacterization irregular moon ElaraWorking Group 2
EUROPA_FLYBY_WG2 Working Group 2
GANYMEDE_DISTANT Working Group 2
GANYMEDE_FLYBY_WG2 Working Group 2
IO_MONITORING- JANUS minimum distance = 7.00e+05 km - MAJIS minimum distance = 8.00e+05 km - SWI minimum distance = 6.00e+05 km (able to resolve target when angular size is > 1 mrad) Working Group 2
IO_TOR_DUSTIo torus dustWorking Group 2
JM_PE_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
CALLISTO_IONOCALLISTO_IONO In situ Callisto ionosphere observationWorking Group 3
EUROPA_IONO_ISEUROPA_IONO_IS In situ Europa ionosphere observationWorking Group 3
GANYMEDE_IONOGANYMEDE_IONO In situ Ganymede ionosphere observationWorking Group 3
G_IS_4G4 Working Group 3
JM_PE35 Working Group 3
JM_PE33share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE31share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE29share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE27share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE25share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE23share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE21share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE19share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE17share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE15share prime high lat PJ between WG3 and WG4Working Group 3
JM_PE13share prime high lat PJ between WG3 and WG4Working Group 3
TOR_RS Working Group 3
JM_INCL Working Group 3
JM_CB Working Group 3
JM_ENA Working Group 3
JM_GMJupiter Magnetosphere global monitoring. Large pointing flexibility, constraints mainly driven by PEPWorking 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
G_IS Working Group 3
E_IS Working Group 3
C_IS Working Group 3
CALLISTO_ENAFar approach energetic neutral atom imaging of CallistoWorking Group 3
CALLISTO_FLYBY_RPWI_IONO_AJS Working Group 3

1 2 3 4 334 segment definitions