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Mnemonic:
JUPITER_CB
Name:
JUPITER_CB
Description:
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.
Trajectories:
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
Prime Segment:
Group:
Working Group 3
Pointing
Pointing request file:
Slew Policy:
-
Pointing Target:
corotation should be in the FoV of PEP/JDC or PEP/JEI. JDC is preferred for monitoring corotation, over JEI, when possible.
Scheduler
Scheduler Flag:
Scheduling Priority:
-
Observation Definitions
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
Scheduling rules:
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')
Contextual Parameters:
Comments:
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]
Attachment file 1:
Attachment file 2:
Attachment file 3:
Attachment file 4:
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