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SWI_JUP_LIMB_RASTER_FS_V1
SWI JUP LIMB RASTER FS V1
Same as SWI JUP LIMB RASTER PS, except a frequency-switch calibration
mode is used instead of position-switch. It enables spending  100% of the integration time
on-source. If the purity of the spectral band is good enough, there is an option to pre-compute
ON-OFF for the CTS before downlink.
SWI

Pointing

nadir
Jupiter atmosphere

Advanced

Scheduling: d1 for winds/temperature, d1/d2 for composition. Repetition:
This mode is the baseline mode for SWI when the distance to Jupiter is < d1 (in order to
cover all latitudes and longitudes with goal resolutions), except when other observation modes
are used.
any rule that is used to schedule the observation: repetition rules, continuous (plasma instruments), one-off, every orbit, every day, etc
none
conditions that make the observation not possible (e.g. thruster firing)
#update2024Oct02

Commanding