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SWI_5POINT_CROSS_FS_V1
SWI 5POINT CROSS FS V1
Same as SWI 5POINT CROSS PS, except a frequency-switch calibration
mode is used instead of position-switch. It enables spending  100% of the integration time onsource.
For Jupiter, two CTS spectra are recorded for 60 seconds over 10000 channels (16 bits
coding). For moon monitoring, two CTS spectra are recorded for 30 seconds over 210 channels
(16 bits coding). For both cases, and in parallel, two CCH measurements (20 bits coding) are
recorded for 0.1 second. If the purity of the spectral band is good enough, there is an option to
pre-compute ON-OFF for the CTS before downlink. Frequency-switch calibration method for
CTS data.
SWI

Pointing

nadir
-

Advanced

This mode is particularly meant for daily monitoring the moons during
the Jupiter Tour. It can also be used for rough mapping of Jupiter and calibration purposes from
long distances. Expected to be used when the target angular size is 1 to 2   the FWHM.
any rule that is used to schedule the observation: repetition rules, continuous (plasma instruments), one-off, every orbit, every day, etc
TBD
conditions that make the observation not possible (e.g. thruster firing)
#update2024Oct02

Commanding