Monte Carlo ray-tracing shows quasilinear scattering coefficients for solar radio waves are accurate for weak scattering but deviate in strong scattering, requiring a speed-based correction in 3D.
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A Monte Carlo simulation on the scattering coefficients of solar radio wave propagation
Monte Carlo ray-tracing shows quasilinear scattering coefficients for solar radio waves are accurate for weak scattering but deviate in strong scattering, requiring a speed-based correction in 3D.