About the preparation and analysis of the RPW/SCM noise measurements, to be performed during spacecraft Earth magnetic lobes crossing.
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General
Purpose & Objectives
During the CP (TBC), Solar Orbiter will pass inside the Earth magnetic lobes, where the B field amplitude is very low. It is the occasion for RPW to measure the SCM sensitivity.
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Give here the overall timeline of the operation, including the expected instrument operating configurations.
Orbitography
Give here the orbitography (i.e., time versus S/C orbit/attitude)
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Give here the operation constraints at RPW and SOLO levels (e.g., TM rate, PW, SOOP, etc.)
Command/Control
Give here the list of flight procedures and IOR (PDOR?) required to execute this operation
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