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Turbulent Density Fluctuations and Proton Heating Rate in the Solar Wind from 9–20<i>R</i><sub>⊙</sub>
We obtain scatter broadened images of the Crab Nebula at 80 MHz as it transits through the inner solar wind in June 2016 and 2017. These images are anisotropic, with the major axis oriented perpendicular to the radially outward coronal magnetic field. Using these data, we deduce that the density …