JA_PE20 | | Working Group 4 |
JM_PE19 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JA_PE18 | | Working Group 4 |
JM_PE17 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JA_PE16 | | Working Group 4 |
JM_PE15 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JA_PE14 | | Working Group 4 |
JM_PE13 | share prime high lat PJ between WG3 and WG4 | Working Group 3 |
JA_PE12 | | Working Group 4 |
JA_PE11 | | Working Group 4 |
JA_PE10 | | Working Group 4 |
JA_PE9 | | Working Group 4 |
JA_PE8 | | Working Group 4 |
JA_PE7 | | Working Group 4 |
JA_PE6 | | Working Group 4 |
JA_PE5 | | Working Group 4 |
JA_PE4 | | Working Group 4 |
JA_PE3 | | Working Group 4 |
JA_PE2 | | Working Group 4 |
G_RS_4G4 | | Working Group 2 |
G_RS_3G3 | HAA as per 3GM UM
IS considering NIM | Working Group 2 |
G_RS_2G2 | | Working Group 2 |
ASTRO_INNER | Astrometry inner moons | Working Group 2 |
CHAR_IRR1 | Characterization irregular moons group 1 (see list below) | Working Group 2 |
J_AURORA | | Working Group 4 |
IO_RS | | Working Group 2 |
TOR_RS | | Working Group 3 |
J_RING | | Working Group 2 |
PR | | WGX |
EUROPA_FB_RS | Europa Flyby remote sensing | Working Group 2 |
CALLISTO_FB_RS | Callisto Flyby remote sensing | Working Group 2 |
GANYMEDE_FB_RS | Ganymede flyby remote sensing | Working Group 2 |
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 |
JM_INCL | | Working Group 3 |
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 |
DL_ | assuming:
JMAG: 2.31 kbps
RPWI: 1.7*2.167 kbps (Ballparks numbers from the team)
PEP: 2 kpbs (ball park number; discussion with Gabriella at WG3 F2F meeting in Sept 2018) | GENERIC |
CAL | | WGX |
JM_CB | | Working Group 3 |
JM_ENA | | Working Group 3 |
JM_GM | | Working Group 3 |
JA_PH | | Working Group 4 |
JA_M | | Working Group 4 |
JA_INCL | | Working Group 4 |
G_IS | | Working Group 3 |
G_distant | | Working Group 2 |
E_RS | | Working Group 2 |
E_IS | | Working Group 3 |
E_GPH | | Working Group 1 |
E_distant | | Working Group 2 |
C_IS | | Working Group 3 |
C_distant | | Working Group 2 |
GAN_EUR_TRANSIT_PR | Double transit in front of Jupiter (Europa, Ganymede) | WGX |
CALLISTO_FLYBY | | Working Group 1 |
CALLISTO_FLYBY_3GM | | Working Group 1 |
CALLISTO_FLYBY_GALA | | Working Group 1 |
CALLISTO_FLYBY_JANUS | | Working Group 1 |
CALLISTO_FLYBY_MAJIS | | Working Group 1 |
CALLISTO_FLYBY_RIME_AJS | Callisto active radar opportunity, anti-jovian side | Working Group 1 |
CALLISTO_FLYBY_RIME_JS | Callisto active radar opportunity, jovian side | Working Group 1 |
CALLISTO_RPWI_PASSIVRAD | Callisto passive radar opportunity for RPWI | Working Group 1 |
EUROPA_FLYBY | | Working Group 1 |
EUROPA_FLYBY_3GM | | Working Group 1 |
EUROPA_FLYBY_GALA | | Working Group 1 |
EUROPA_FLYBY_JANUS | | Working Group 1 |
EUROPA_FLYBY_MAJIS | | Working Group 1 |
EUROPA_FLYBY_RIME_JS | Europa active radar opportunity, jovian side | Working Group 1 |
EUROPA_RPWI_PASSIVRAD | Europa passive radar opportunity for RPWI | Working Group 1 |
GANYMEDE_FLYBY | | Working Group 1 |
GANYMEDE_FLYBY_3GM | | Working Group 1 |
GANYMEDE_FLYBY_GALA | | Working Group 1 |
GANYMEDE_FLYBY_JANUS | | Working Group 1 |
GANYMEDE_FLYBY_MAJIS | | Working Group 1 |
GANYMEDE_FLYBY_RIME_AJS | Ganymede active radar opportunity, anti-jovian side | Working Group 1 |
GANYMEDE_FLYBY_RIME_JS | Ganymede active radar opportunity, jovian side | Working Group 1 |
GANYMEDE_RPWI_PASSIVRAD | Ganymede passive radar opportunity for RPWI | Working Group 1 |
ASTRO_IRR2_PASIPHAE | astrometry measurement with inertial pointing to moon Pasiphae | Working Group 2 |
ASTRO_IRR2_SINOPE | | Working Group 2 |
ASTRO_IRR_ELARA | | Working Group 2 |
CALLISTO_DISTANT | | Working Group 2 |
CHARACTERIZATION_IRR2_CARME | | Working Group 2 |
CHARACTERIZATION_IRR2_PASIPHAE | characterization irregular moon Pasiphae | Working Group 2 |
CHARACTERIZATION_IRR2_SINOPE | Characterization irregular moon Sinope | Working Group 2 |
CHARACTERIZATION_IRR_ELARA | Characterization irregular moon Elara | Working Group 2 |
GANYMEDE_DISTANT | | 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_DUST | Io torus dust | Working Group 2 |
CALLISTO_ENA | Far approach energetic neutral atom imaging of Callisto | Working Group 3 |
CALLISTO_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
CALLISTO_WAKE | In situ Callisto wake observation | Working Group 3 |
EUROPA_ENA | Far approach energetic neutral atom imaging of Europa | Working Group 3 |
EUROPA_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
EUROPA_TOR_IS | In situ Europa torus observation | Working Group 3 |
EUROPA_WAKE | In situ Europa wake observation | Working Group 3 |
GANYMEDE_ENA | Far approach energetic neutral atom imaging of Ganymede | Working Group 3 |
GANYMEDE_GM | In situ mapping of global configuration and monitoring dynamics of Ganymede's magnetospheric environment | Working Group 3 |
GANYMEDE_FLYBY_RPWI_IONO_AJS | | Working Group 3 |
GANYMEDE_WAKE | In situ Ganymede wake observation | 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 |