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JMAG_CALROLL
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
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
WGX

Pointing

-

Scheduler

None
-

Observation Definitions

PEL_JUPITER_IN_SITU_NOMINAL_1, PEL_JUPITER_IN_SITU_IMAGING_NOMINAL_1, PEL_JUPITER_IN_SITU_IMAGING_BURST_1, PEL_JUPITER_IN_SITU_IMAGING_LOW_1, PEL_GANYMEDE_IN_SITU_LOW_1, PEL_JUPITER_IN_SITU_BURST_1, PEL_JUPITER_IN_SITU_LOW_1, PEL_GANYMEDE_IN_SITU_LOW_5, PEL_GANYMEDE_IN_SITU_NOMINAL_3, PEL_GANYMEDE_IN_SITU_LOW_6, PEL_GANYMEDE_IN_SITU_LOW_7, PEH_JUPITER_IN_SITU_IMAGING_NOMINAL_1, PEH_JUPITER_IN_SITU_NOMINAL_1, PEH_JUPITER_IN_SITU_IMAGING_BURST_1

Advanced

The opportunity windows for JMAG calibration rolls are defined as:
Interval |B|> 100 nT for more than 12 hours (Use Khurana model or/and latest B model from Juno (Jupiter intrinsic) )
the local magnetic field strength is not varying by more than 10 nT over each of the six 2 hour-windows (within the 12 hours).
At least one of those 2hour windows is not varying by more than 5 nT.
5 rolls in total should be scheduled during the tour: 2 as soon as possible after JOI, 2 right before GOI and one in the middle
Opportunity computation in geopipeline
-Waiting for discussion with Adam Master
- Currently, any window longer than 12h with at least 100 nT - plot attached

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