Home › Core › Segment definitions

Select segment definition to view

3
Mnemonic
2
Description
1
Group
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
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_OBSJupiter Magnetosphere perijove segments containing link to observations databaseWorking Group 3
JUPITER_TAILIn situ search for signatures of local magnetic reconnection in the Jovian magnetotailWorking 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
GANYMEDE_GMIn situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environmentWorking 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_NULLIn situ Jupiter magnetic null searchWorking Group 3
JUPITER_CPSIn situ Jupiter current/plasma sheet 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_CPIn 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. CP stands for corotation profileWorking Group 3
GANYMEDE_WAKEIn situ Ganymede wake observationWorking Group 3
EUROPA_WAKEIn situ Europa wake observationWorking Group 3
EUROPA_TOR_ISIn situ Europa torus observationWorking Group 3
CALLISTO_WAKEIn situ Callisto wake 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
GANYMEDE_IONOGANYMEDE_IONO In situ Ganymede ionosphere observationWorking Group 3
G_IS_3G3Ganymede in-situ observations around closest approachWorking Group 3
G_IS_OBSG_IS_OBSWorking Group 3
GANYMEDE_ENAFar approach energetic neutral atom imaging of GanymedeWorking Group 3
EUROPA_ENAFar approach energetic neutral atom imaging of EuropaWorking Group 3
CALLISTO_ENAFar approach energetic neutral atom imaging of CallistoWorking Group 3
EUROPA_IONO_ISEUROPA_IONO_IS In situ Europa ionosphere observationWorking Group 3
E_IS_OBSE_IS_OBSWorking Group 3
CALLISTO_IONOCALLISTO_IONO In situ Callisto ionosphere observationWorking Group 3
C_IS_OBSC_IS_OBSWorking 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
TOR_RS Working Group 3
JM_PE35 Working Group 3
JM_PE_P4_noDL Working Group 3
JM_INCL Working Group 3
JM_GM Working Group 3
JM_ENA Working Group 3
JM_CB Working Group 3
GANYMEDE_FLYBY_RPWI_IONO_AJS Working Group 3
G_IS_4G4 Working Group 3
G_IS Working Group 3
EUROPA_FLYBY_RPWI_IONO_AJS Working Group 3
E_IS Working Group 3
CALLISTO_FLYBY_RPWI_IONO_AJS Working Group 3
C_IS Working Group 3
508_PasTest opportunity segment PasiphaeWorking Group 2
G_RS_9G6test 3_2Working Group 2
G_RS_26G12test 3_2Working Group 2
G_RS_24G10test 3_2Working Group 2
G_RS_21G9test 3_2Working Group 2
G_RS_20G8test 3_2Working Group 2
G_RS_19G7test 3_2Working Group 2
C_RS_8C1test 3_2Working Group 2
C_RS_23C12test 3_2Working Group 2
C_RS_22C11test 3_2Working Group 2
C_RS_18C10test 3_2Working Group 2
C_RS_17C9test 3_2Working Group 2
C_RS_16C8test 3_2Working Group 2
C_RS_15C7test 3_2Working Group 2
C_RS_14C6test 3_2Working Group 2
C_RS_13C5test 3_2Working Group 2
C_RS_12C4test 3_2Working Group 2
C_RS_11C3test 3_2Working Group 2
C_RS_10C2test 3_2Working Group 2
ROI_INTERSECTIONROI_INTERSECTIONWorking Group 2
RINGSPIRAL_MPRINGSPIRAL_MP (medium phase: JANUS Def)Working Group 2
RINGSPIRAL_HPRINGSPIRAL_HP (high phase, Janus def)Working Group 2
SHADOWEDGErings SHADOWEDGE. Imaging of the ring region intersected by the planetary shadow at moderate elevation and very high phase. Especially for the very faint gossamer rings and the Thebe extensionWorking Group 2
HIGHPHPROFILErings high phase profile (JANUS DEF)Working Group 2
RINGMOSAICRINGMOSAIC (Janus definition). impression of the extent of the whole ring systemWorking Group 2
RINGMATTERRINGMATTER. Observations of the main rings and the gossamer rings, imaging the ring ansae from moderately large elevation. The moderatly large elevation will reveal azimuthal structure in the rings and the presence of clumps at the resolution limit of the imaging.Working Group 2
RING_LPRing low phaseWorking Group 2
RING_HPRing high phaseWorking 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_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
J_SATjupiter satellite GENERICWorking Group 2
J_SAT_OBSJ_SAT_OBSWorking Group 2
J_SAT_IRR_SEARCHJ_SAT_IRR_SEARCH discover new irregular moonsWorking Group 2
J_SAT_572_11J1J_SAT_572_11J1Working Group 2
J_SAT_571_ErsJ_SAT_571_ErsWorking Group 2
J_SAT_570_17J9J_SAT_570_17J9Working Group 2
J_SAT_569_17J8J_SAT_569_17J8Working Group 2
J_SAT_568_17J7J_SAT_568_17J7Working Group 2
J_SAT_567_17J6J_SAT_567_17J6Working Group 2
J_SAT_566_17J5J_SAT_566_17J5Working Group 2
J_SAT_565_PdiJ_SAT_565_PdiWorking Group 2
J_SAT_564_17J3J_SAT_564_17J3Working Group 2
J_SAT_563_17J2J_SAT_563_17J2Working Group 2
J_SAT_562_ValJ_SAT_562_ValWorking Group 2
J_SAT_561_3J19J_SAT_561_3J19Working Group 2
J_SAT_560_EphJ_SAT_560_EphWorking Group 2
J_SAT_559_17J1J_SAT_559_17J1Working Group 2
J_SAT_558_PhiJ_SAT_558_PhiWorking Group 2
J_SAT_557_EirJ_SAT_557_EirWorking Group 2
J_SAT_556_11J2J_SAT_556_11J2Working Group 2
J_SAT_55508_3J24J_SAT_55508_3J24Working Group 2
J_SAT_55507_3J23J_SAT_55507_3J23Working Group 2

1 2 3 4 5 6 7 635 segment definitions