Turbulent density fluctuations and proton heating rate in the solar wind from 9-20~R_{\odot} (1710.06295v1)

Abstract: 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 modulation index (\delta N_e/N_e) caused by turbulent density fluctuations in the solar wind ranges from 1.9 \times 10^{-3} to 7.7 \times 10^{-3} between 9-20 R_{\odot}. We also find that the heating rate of solar wind protons at these distances ranges from 2.2 \times 10^{-13} to 1.0 \times 10^{-11} ~erg~cm^{-3}~s^{-1}. On two occasions, the line of sight intercepted a coronal streamer. We find that the presence of the streamer approximately doubles the thickness of the scattering screen.