View segment definition

JUPITER_CB
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.
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_b2
False
Working Group 3

Pointing

-
corotation should be in the FoV of PEP/JDC or PEP/JEI. JDC is preferred for monitoring corotation, over JEI, when possible.

Scheduler

None
-

Observation Definitions

PEP_JUPITER_IN_SITU_NOMINAL_1, PEP_JUPITER_IN_SITU_IMAGING_NOMINAL_1, PEP_JUPITER_IN_SITU_IMAGING_LOW_1, PEP_JUPITER_IN_SITU_LOW_1

Advanced

Distance with respect to Jupiter barycentre 15 < range < 50 (RJ) AND when outside of Ganymede's magnetosphere. (Currently taking 2.25 RG from Ganymede is the value assumed for 'outside of Ganymede magnetosphere')
Opportunity implementation in geopipeline:
-Distance to Jupiter barycentre > 15 RJ
AND
-Distance to Jupiter barycentre < 50 RJ
AND
-Distance to Ganymede barycentre > 2.25 RG
NOTE: taking 2.25 RG from Ganymede is the value assumed for 'outside of Ganymede magnetosphere'
;; [from Nico's own estimate assuming Ganymede magnetosphere's having about
; 4-5 RG DIAMETER - from Wikipedia]