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3GM_IO_PLASMA_TORUS_OCCULTATION
3GM_IO_PLASMA_TORUS_OCCULTATION
The radio science experiment 3GM will use navigation data in X/X and X/Ka band to characterize the Io plasma torus. The data generated by the DST in 2-way dual-frequency radio links will be the primary observable to perform this investigation. Occultations occur throughout the jovian tour, but their phasing is not always synchronized with the timing of dedicated Jupiter observations by the other orbiter experiments. USO will stay MUTED and HAA in nominal SCIENCE.
Note that other observation strategy would be possible (2-way triple link, 1-way X and Ka link with USO UNMUTED).
3GM

Pointing

track
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Advanced

HAA should be in CONFIGURATION mode and scheduled in the background (TO BE SCHEDULED BY SOC AT PLANNING SET-UP). If HAA is OFF, HAA needs to be ON at least 48hours before measurement starts. Occultation observations are event-driven and defined by the Earth-SC line crossing the Io plasma torus. Note that the occultation event shall include a 1-hour margin at the beginning and at the end to serve as a baseline for radiometric measurements. This observation should be preceded by 3GM_HAA_SELF_CALIBRATION 1 hour before the start of the observation.
any rule that is used to schedule the observation: repetition rules, continuous (plasma instruments), one-off, every orbit, every day, etc
N/A
conditions that make the observation not possible (e.g. thruster firing)

Commanding