| 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 | | Working Group 4 |
|---|
| JM_CB | | Working Group 3 |
|---|
| JM_ENA | | Working Group 3 |
|---|
| JM_GM | | Working Group 3 |
|---|
| JM_INCL | | Working Group 3 |
|---|
| JM_PE | 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) | Working Group 3 |
|---|
| JM_PE_OBS | Jupiter Magnetosphere perijove segments containing link to observations database | Working Group 3 |
|---|
| JM_PE13 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE15 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE17 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| JM_PE19 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
|---|
| 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 |
|---|
| JMAG_CALROLL | 5 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 GOI | WGX |
|---|
| 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_FD_EPHEM_GAN | | GENERIC |
|---|
| JUPITER_FD_NAV_FB | | GENERIC |
|---|
| JUPITER_FD_TCM | | GENERIC |
|---|
| JUPITER_FD_WOL | Flight dynamics wheel off-loading slot, outside of Flyby preparation and recuperation | GENERIC |
|---|
| JUPITER_FD_WOL_FB | In the last week before the fly-by a WOL slot shall be combined with the
TCM slot at To– 3 days (i.e. a single 3-hr slot). Another 2-hour WOL slot shall be reserved at To + 12 hours. | GENERIC |
|---|
| 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_INCLINED_AURORA | | Working Group 4 |
|---|
| JUPITER_MONITORING | | Working Group 4 |
|---|
| 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_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 |
|---|
| JUPITER_TAIL | In situ search for signatures of local magnetic reconnection in the Jovian magnetotail | Working Group 3 |
|---|
| OPNAV_CAL | OPNAV_CAL | GENERIC |
|---|
| OPNAV_EUR | OPNAV_EUR | GENERIC |
|---|
| OPNAV_GAN | OPNAV_GAN | GENERIC |
|---|
| PERIJOVE_DAYSIDE | | Working Group 4 |
|---|
| PERIJOVE_NIGHTSIDE | | Working Group 4 |
|---|
| PERIJOVE_TERMINATOR | | Working Group 4 |
|---|
| PR | | WGX |
|---|
| RING_HP | Ring high phase | Working Group 2 |
|---|
| RING_LP | Ring low phase | Working Group 2 |
|---|
| RING_PHASECURV_10 | Opportunity 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 deg | Working Group 2 |
|---|
| RING_PHASECURV_100 | | Working Group 2 |
|---|