Across Chandrayaan-2/3, Venus Express, and Akatsuki data, interplanetary plasma adds mHz-level Doppler noise to S-band signals and smaller X-band noise, while lunar ionosphere and coronal paths show much larger fluctuations.
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A study on the contribution of the interplanetary medium in radio occultation experiments
Across Chandrayaan-2/3, Venus Express, and Akatsuki data, interplanetary plasma adds mHz-level Doppler noise to S-band signals and smaller X-band noise, while lunar ionosphere and coronal paths show much larger fluctuations.