View segment definition

CAL
CAL
CReMA 3.0, CReMA 3.1, CReMA 3.2, CReMA 4.0B, 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
True
WGX

Pointing

-

Scheduler

None
-

Observation Definitions

MAG_CALROLL, 3GM_HAA_CALIBRATION, 3GM GRAVITY FOR EPHEMERIDES, HAA_STDBY, 3GM USO SWON, MAJ_BORESIGHT_ALIGNEMENT, MAJ internal calibration using ICU, MAJ SAFE, MAJ_SERVICE

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
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)
SWI monitoring of the moons no included for now. (as per spreadsheet)

From case #5/6 onward:
moniroting rate for in-situ 7.36 kbps
SWI monitoring 0.33 kbps