New blog post: Analysis of the CAMRAS Venus radar experiment. A deep dive into the Earth-Venus-Earth L-band radar experiment done in March by @radiotelescoop, Astropeiler Stockert, the Deep Space Exploration Society, and @OpenResearchIns.
I show how to compute the radar Doppler with SPICE and come up with a Doppler spread model based on an S-band scattering model from Arecibo. I explain why the maximum surface Doppler offset is 8.6 Hz even though the rotational velocity predicts 15.7 Hz.