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SWI_5POINT_CROSS_FS
SWI 5POINT CROSS FS
Same as SWI 5POINT CROSS 12 PS, except a frequency-switch calibration mode is used instead of position-switch. It enables spending ~100% of the integration time on-source. For Jupiter, two CTS spectra are recorded every 60 seconds over 10000 channels (16 bits coding). For moon monitoring, two CTS spectra are recorded every 30 seconds over 210 channels (16 bits coding). For both cases, and in parallel, two CCH measurements (20 bits coding) are recorded every 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
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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. To be used when the target angular size is 1 to 2 x 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)
#update2021

Commanding