Home › Core › Segment definitions

Select segment definition to view

Mnemonic
1
Description
2
Group
SPICE_ATT_GOTOEUROPA_NPO GENERIC
SPICE_ATT_GOTOEUROPA_NOA GENERIC
SPICE_ATT_GOTOMARS_NPO GENERIC
SPICE_ATT_GOTOMARS_NOA_HOT GENERIC
SPICE_ATT_GOTOGANYMEDE_NPO GENERIC
SPICE_ATT_GOTOGANYMEDE_NOA GENERIC
SPICE_ATT_GOTOEARTH_NPO GENERIC
SPICE_ATT_GOTOCALLISTO_NOA_HOT GENERIC
SPICE_ATT_GOTOEARTH_NOA_HOT GENERIC
SPICE_ATT_GOTOCALLISTO_NPO GENERIC
SPICE_ATT_GOTOCALLISTO_NOA GENERIC
JUPITER_FD_TCM GENERIC
JUPITER_FD_NAV_FB GENERIC
PR WGX
CAL WGX
JANUS_DESIGNER_OBSERVATION JANUS
PEPLO_DESIGNER_OBSERVATION PEPLO
RIME_DESIGNER_OBSERVATION RIME
RIME_RIDER_OBSERVATION RIME
RIME_PRIME_OBSERVATION RIME
SWI_DESIGNER_OBSERVATION SWI
SWI_RIDER_OBSERVATION SWI
SWI_PRIME_OBSERVATION SWI
JMAG_DESIGNER_OBSERVATION JMAG
3GM_OBSERVATION 3GM
GALA_DESIGNER_OBSERVATION GALA
RADEM_DESIGNER_OBSERVATION RADEM
NAVCAM_DESIGNER_OBSERVATION NAVCAM
SOC_DESIGNER_OBSERVATION SOC
SOC_OBSERVATION SOC
PEPHI_DESIGNER_OBSERVATION PEPHI
PEPHI_OBSERVATION PEPHI
PEPHI_PRIME_OBSERVATION PEPHI
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
RECOVERY_FLYBY15.15 hours recovery segments to be scheduled after flybys/eclipse, when standard instrument mode is assumed Duration is derived from https://issues.cosmos.esa.int/juicewiki/display/SOCDEV/Downlink%2C+Recovery%2C+and+Eclipse+Scenario+Analysis Pointing should be power optimizedGENERIC
BATTERY_RECHARGE20.5 hour recovery segments to be scheduled after very demanding periods. For the moment only after flybys and eclipses. Duration is derived from https://issues.cosmos.esa.int/juicewiki/display/SOCDEV/Downlink%2C+Recovery%2C+and+Eclipse+Scenario+AnalysisGENERIC
JMAG_CALROLL5 calibration roll needed by JMAG. 2 as soon as possible after JOI. 3 during phase 5: one at the start of phase 5, the last 2 as late as possible before GOIWGX
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
ASTRO_IRR1_MEGACLITEASTRO_IRR1_MEGACLITEWorking Group 2
ASTRO_INNERAstrometry inner moonsWorking Group 2
ASTRO_IRR2_ANANKEAstrometry irregular moon AnankeWorking Group 2
ASTRO_IRR2_CARMEAstrometry irregular moon CarmeWorking Group 2
ASTRO_IRR1_CARPOAstrometry irregular moon CARPOWorking Group 2
ASTRO_IRR1_CHALDENEAstrometry irregular moon CHALDENEWorking Group 2
ASTRO_IRR1_HIMALIAAstrometry irregular moon HIMALIAWorking Group 2
ASTRO_IRR1_KALLICHOREAstrometry irregular moon KALLICHOREWorking Group 2
ASTRO_IRR1_LEDAAstrometry irregular moon LEDAWorking Group 2
ASTRO_IRR1_LYSITHEAAstrometry irregular moon LYSITHEAWorking Group 2
ASTRO_IRR1_TAYGETEAstrometry irregular moon TAYGETEWorking Group 2
ASTRO_IRR1_THEMISTOAstrometry irregular moon THEMISTOWorking Group 2
ASTRO_IRR2_PASIPHAEastrometry measurement with inertial pointing to moon PasiphaeWorking Group 2
ECLIPSE_BATTERY_RECOVERY_STANDARDBattery recharge after eclipse pointing should be default power optimised pointingGENERIC
ECLIPSE_BATTERY_RECOVERY_FASTBattery recharge after eclipseGENERIC
C_GPH_10C3C_GPH_10C3Working Group 1
C_GPH_11C4C_GPH_11C4Working Group 1
C_GPH_12C5C_GPH_12C5Working Group 1
C_GPH_13C6C_GPH_13C6Working Group 1
C_GPH_14C7C_GPH_14C7Working Group 1
C_GPH_15C8C_GPH_15C8Working Group 1
C_GPH_16C9C_GPH_16C9 Geophysics prime segment, defined based on GALA (transmitting) operational range of altitude above Callisto < 2000 km. Assumed Nadir pointingWorking Group 1
C_GPH_18C11C_GPH_18C11Working Group 1
C_GPH_19C12C_GPH_19C12Working Group 1
C_GPH_20C13C_GPH_20C13Working Group 1
C_GPH_21C14C_GPH_21C14Working Group 1
C_GPH_22C15C_GPH_22C15Working Group 1
C_GPH_23C16C_GPH_23C13Working Group 1
C_GPH_24C17C_GPH_24C17Working Group 1
C_GPH_25C18C_GPH_25C18Working Group 1
C_GPH_28C19C_GPH_28C19Working Group 1
C_IS_OBSC_IS_OBSWorking Group 3
C_RS_10C3C_RS_10C3Working Group 2
C_RS_11C4C_RS_11C4Working Group 2
C_RS_12C5C_RS_12C5Working Group 2
C_RS_13C6C_RS_13C6Working Group 2
C_RS_14C7C_RS_14C7Working Group 2
C_RS_15C8C_RS_15C8Working Group 2
C_RS_16C9C_RS_16C9: Prime surface and exosphere segment defined as 24 hours centered at CA. WG1 (gravity) is rider. Pointing is mainly surface and/or limb (details TBD)Working Group 2
C_RS_17C10C_RS_17C10Working Group 2
C_RS_18C11C_RS_18C11Working Group 2
C_RS_19C12C_RS_19C12Working Group 2
C_RS_20C13C_RS_20C13Working Group 2
C_RS_21C14C_RS_21C14Working Group 2
C_RS_22C15C_RS_22C15Working Group 2
C_RS_23C16C_RS_23C16Working Group 2
C_RS_24C17C_RS_24C17Working Group 2
C_RS_25C18C_RS_25C18Working Group 2
C_RS_28C19C_RS_28C19Working Group 2
C_RS_29C20C_RS_29C20Working Group 2
C_RS_31C21C_RS_31C21Working Group 2
C_RS_6C1C_RS_6C1Working Group 2
C_RS_9C2C_RS_9C2Working Group 2
CALLISTO_FLYBY_RIME_AJSCallisto active radar opportunity, anti-jovian sideWorking Group 1
CALLISTO_FLYBY_RIME_JSCallisto active radar opportunity, jovian sideWorking Group 1
CALLISTO_FB_RSCallisto Flyby remote sensingWorking Group 2
C_GPH_OBSCallisto geophysics generic containing obs database linkWorking Group 1
CALLISTO_RPWI_PASSIVRADCallisto passive radar opportunity for RPWIWorking Group 1
C_RS_OBSCallisto Remote sensing GENERIC containing obs database linkWorking Group 2
CALLISTO_IONOCALLISTO_IONO In situ Callisto ionosphere observationWorking Group 3
CHARACTERIZATION_IRR2_ANANKECharacterization irregular moon ANANKEWorking Group 2
CHARACTERIZATION_IRR_ELARACharacterization irregular moon ElaraWorking Group 2

1 2 3 4 5 6 553 segment definitions