Select segment definition to view

GANYMEDE_FLYBY_JANUS Working Group 1
GANYMEDE_FLYBY_MAJIS Working Group 1
GANYMEDE_FLYBY_RIME_AJSGanymede active radar opportunity, anti-jovian sideWorking Group 1
GANYMEDE_FLYBY_RIME_JSGanymede active radar opportunity, jovian sideWorking Group 1
GANYMEDE_RPWI_PASSIVRADGanymede passive radar opportunity for RPWIWorking Group 1
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
CALLISTO_ENAFar approach energetic neutral atom imaging of CallistoWorking Group 3
CALLISTO_FLYBY_RPWI_IONO_AJS Working Group 3
CALLISTO_WAKEIn situ Callisto wake observationWorking Group 3
EUROPA_ENAFar approach energetic neutral atom imaging of EuropaWorking Group 3
EUROPA_FLYBY_RPWI_IONO_AJS Working Group 3
EUROPA_TOR_ISIn situ Europa torus observationWorking Group 3
EUROPA_WAKEIn situ Europa wake observationWorking Group 3
GANYMEDE_ENAFar approach energetic neutral atom imaging of GanymedeWorking Group 3
GANYMEDE_GMIn situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environmentWorking Group 3
GANYMEDE_FLYBY_RPWI_IONO_AJS Working Group 3
GANYMEDE_WAKEIn situ Ganymede wake observationWorking Group 3
JUPITER_CBIn situ Jupiter corotation breakdown region and plasma transport observation. Maximize the intervals for which co-rotation is measured to build spatial and temporal coverage of corotation profiles across the magnetosphere and also in the local moon environments.Working Group 3
JUPITER_CPSIn situ Jupiter current/plasma sheet observationWorking Group 3
JUPITER_ENAImaging of Jupiter's magnetosphere in energetic neutral atoms (ENAs).Maximize pitch angle coverage with PEP JEI,JDC,JoEE, JENI (ion mode) a) JENI has a broad FoV and captures Jupiter and the Io/Europa torus and magnetosphere at most times. No special pointing design required for JENI besides requiring an approximate nadir pointing (considerable offsets can still be acceptable) b) JNA disk-shaped/slit FoV has a slight offset from the XZ spacecraft plane, meaning that during nadir pointing, it images preferentially the northern or southern extension of the Europa/Io torus, whereas Jupiter may be in the edge or outside of the FoV, especially at large distances. Scans (small rotations around Sc-X) or periods with stable, small offset of the SC-xz plane from Nadir can help to better image stronger emissions from the equatorial torusWorking Group 3
JUPITER_GMIn situ mapping of global configuration and monitoring dynamics of the Jovian magnetospheric environment. corotation should be in the FoV of PEP/JDC or PEP/JEI. Conditions for coverage: ◦ Minimum angle less than about 11.25 deg (half-azimuthal sector size) of a JEI or JDC pixel from corotation ◦ Boresight angle of JDC or JEI less than ˜90 deg Conditions for ideal coverage: ◦ Minimum angle less than about 11.25 deg (half-azimuthal sector size) of a JEI or JDC pixel from corotation ◦ Boresight angle less than ˜75 deg (JEI) or 70 deg (JDC): corotation away from the FoV edge JDC is preferred for monitoring corotation, over JEI, when possible.Working Group 3
JUPITER_NULLIn situ Jupiter magnetic null searchWorking Group 3
JUPITER_PDTIn situ Jupiter particle distribution transition region observation. Maximize pitch angle coverage for PEP/JEI, JDC,JoEE, JENI (ion mode)Working Group 3
JUPITER_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking Group 3
EARTH_OCC_EGRESSEarth occultation by Jupiter. EgressWorking Group 4
EARTH_OCC_INGRESSEarth occultation by Jupiter. IngressWorking Group 4
INCLINED_NORTH Working Group 4
INCLINED_SOUTH Working Group 4
JUPITER_INCLINED_AURORA Working Group 4
JUPITER_PERIJOVEJupiter observationsWorking Group 4
JUPITER_PHASE_090 Working Group 4
JUPITER_PHASE_120_DEC Working Group 4
JUPITER_PHASE_120_INC Working Group 4
JUPITER_PHASE_135_DEC Working Group 4
JUPITER_PHASE_135_INC Working Group 4
JUPITER_PHASE_150_DEC Working Group 4
JUPITER_PHASE_150_INC Working Group 4
JUPITER_PHASE_165_DEC Working Group 4
JUPITER_PHASE_165_INC Working Group 4
JUPITER_PHASE_MAX Working Group 4
JUPITER_PHASE_MIN Working Group 4
JUPITER_MONITORING Working Group 4
PERIJOVE_DAYSIDE Working Group 4
PERIJOVE_NIGHTSIDE Working Group 4
PERIJOVE_TERMINATOR Working Group 4
EUR_CAL_TRANSIT_PRDouble transit in front of Jupiter (Europa, Callisto)WGX
GAN_CAL_TRANSIT_PRDouble transit in front of Jupiter (Ganymede, Callisto)WGX

1 2 3 4 5 6 7 660 segment definitions