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JUPITER_ENA
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
CReMA 3.0, CReMA 3.1, CReMA 3.2, CREMA_5_0, CREMA_5_0b23_1, CREMA_5_1_150lb_23_1, CREMA_5_1_150lb_23_1_a3, CREMA_5_1_150lb_23_1_b2
False
Working Group 3

Pointing

-

Scheduler

None
-

Observation Definitions

PEP_JUPITER_IN_SITU_IMAGING_NOMINAL_1, PEP_JUPITER_IN_SITU_IMAGING_BURST_1, PEP_JUPITER_IN_SITU_IMAGING_LOW_1, PEP_JUPITER_IN_SITU_LOW_1

Advanced

Jupiter's rotational equator, or range from Jupiter barycentre of >=20Rj
Opportunity implementation in geopipeline:
- SC sub-spacecraft latitude at Jupiter (from rotational equator) > 0 deg
OR
- SC distance to Jupiter barycentre is > =20 RJ