| JM_PE21 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
| JM_PE23 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
| JM_PE25 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
| JM_PE27 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
| JM_PE29 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
| JM_PE31 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
| JM_PE33 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
| JM_PE35 | | Working Group 3 |
| JUPITER_CB | In 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_CPS | In situ Jupiter current/plasma sheet observation | Working Group 3 |
| JUPITER_ENA | Imaging 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 torus | Working Group 3 |
| JUPITER_GM | In 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_NULL | In situ Jupiter magnetic null search | Working Group 3 |
| JUPITER_PDT | In situ Jupiter particle distribution transition region observation.
Maximize pitch angle coverage for PEP/JEI, JDC,JoEE, JENI (ion mode) | Working Group 3 |
| JUPITER_TAIL | In situ search for signatures of local magnetic reconnection in the Jovian magnetotail | Working Group 3 |
| TOR_RS | | Working Group 3 |
| EARTH_OCC | Earth occultation by Jupiter | Working Group 4 |
| EARTH_OCC_EGRESS | Earth occultation by Jupiter. Egress | Working Group 4 |
| EARTH_OCC_INGRESS | Earth occultation by Jupiter. Ingress | Working Group 4 |
| INCLINED_NORTH | | Working Group 4 |
| INCLINED_SOUTH | | Working Group 4 |
| J_AURORA | | Working Group 4 |
| JA_INCL | Jupiter Atmosphere Inclined segments: at maximum (Northern) and/or minimum (Southern) latitudes.
Pointing target uis Jupiter although pointing details are TBD (track, limb etc...) | Working Group 4 |
| JA_M | Jupiter Atmosphere Monitoring segments: at regular interval during the tour.
Pointing taregt is Jupiter, although pointing type is TBD (slew scan, raster, nadir etc) | Working Group 4 |
| JA_PE | | Working Group 4 |
| JA_PE_OBS | JA_PE generic for link obs<-> segments | Working Group 4 |
| JA_PE1 | test 3_2 | Working Group 4 |
| JA_PE10 | | Working Group 4 |
| JA_PE11 | | Working Group 4 |
| JA_PE12 | | Working Group 4 |
| JA_PE14 | | Working Group 4 |
| JA_PE16 | | Working Group 4 |
| JA_PE18 | | Working Group 4 |
| JA_PE2 | | Working Group 4 |
| JA_PE20 | | Working Group 4 |
| JA_PE22 | | Working Group 4 |
| JA_PE24 | | Working Group 4 |
| JA_PE26 | | Working Group 4 |
| JA_PE28 | | Working Group 4 |
| JA_PE3 | | Working Group 4 |
| JA_PE30 | | Working Group 4 |
| JA_PE32 | | Working Group 4 |
| JA_PE34 | | Working Group 4 |
| JA_PE36 | | Working Group 4 |
| JA_PE37 | | Working Group 4 |
| JA_PE38 | | Working Group 4 |
| JA_PE39 | | Working Group 4 |
| JA_PE4 | | Working Group 4 |
| JA_PE40 | | Working Group 4 |
| JA_PE41 | | Working Group 4 |
| JA_PE42 | | Working Group 4 |
| JA_PE43 | | Working Group 4 |
| JA_PE44 | | Working Group 4 |
| JA_PE45 | | Working Group 4 |
| JA_PE46 | | Working Group 4 |
| JA_PE47 | | Working Group 4 |
| JA_PE48 | | Working Group 4 |
| JA_PE49 | | Working Group 4 |
| JA_PE5 | | Working Group 4 |
| JA_PE50 | | Working Group 4 |
| JA_PE51 | | Working Group 4 |
| JA_PE52 | | Working Group 4 |
| JA_PE53 | | Working Group 4 |
| JA_PE54 | | Working Group 4 |
| JA_PE55 | | Working Group 4 |
| JA_PE56 | | Working Group 4 |
| JA_PE57 | | Working Group 4 |
| JA_PE58 | | Working Group 4 |
| JA_PE59 | | Working Group 4 |
| JA_PE6 | | Working Group 4 |
| JA_PE7 | | Working Group 4 |
| JA_PE8 | | Working Group 4 |
| JA_PE9 | | Working Group 4 |
| JA_PH | Jupiter Atmosphere prime segment at min-90-max phase.
pointing target is Jupiter although pointing type is TBD (limb, etc) | Working Group 4 |
| JUPITER_INCLINED_AURORA | | Working Group 4 |
| JUPITER_MONITORING | | Working Group 4 |
| JUPITER_PERIJOVE | Jupiter observations | Working 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 |
| PERIJOVE_DAYSIDE | | Working Group 4 |
| PERIJOVE_NIGHTSIDE | | Working Group 4 |
| PERIJOVE_TERMINATOR | | Working Group 4 |
| STAR_OCC | | Working Group 4 |
| DL_ | Downlink communication prime segments.
pointing: HGA pointing to Earth | GENERIC |
| DL_EXT | assuming:
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 |
| EARTH_OCC_ET | Event tool support segment definition | GENERIC |
| ECLIPSE_BATTERY_RECOVERY_FAST | Battery recharge after eclipse | GENERIC |
| ECLIPSE_BATTERY_RECOVERY_STANDARD | Battery recharge after eclipse
pointing should be default power optimised pointing | GENERIC |
| FB_BATTERY_RECOVERY_FAST | Segment to allow for battery recharge.
Pointing should be default power optimised | GENERIC |
| FB_BATTERY_RECOVERY_STANDARD | Segment to allow for battery recharge.
Attitude should be default power optimised. | GENERIC |
| FLYBY_ET | Event tool support segment definition | GENERIC |