A forward-modeling framework combining refractive ray tracing in a 3D coronal model with radiative transfer produces synthetic 40-800 MHz radio maps that reproduce the quiet-Sun spectrum for Carrington rotation 2298.
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The quiet-Sun temperature ratio R≈2.4 equals the KL-divergence difference between a κ=2.5 distribution and its EUV and radio Maxwellian projections, satisfying ΔD_KL = (3/2)[R0 − ln R0 − 1] = (3/2) d_IS(T_eff, T_core).
Radio wave distortion effects serve as established probes of solar corona and wind turbulence parameters, with SKA expected to expand observational capabilities.
citing papers explorer
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Modeling the Thermal Low-Frequency Radio Sun with Ray Tracing
A forward-modeling framework combining refractive ray tracing in a 3D coronal model with radiative transfer produces synthetic 40-800 MHz radio maps that reproduce the quiet-Sun spectrum for Carrington rotation 2298.
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Diagnostic Disagreement as an Information-Projection Divergence: An Information-Theoretic Reading of the Quiet-Sun Temperature Ratio
The quiet-Sun temperature ratio R≈2.4 equals the KL-divergence difference between a κ=2.5 distribution and its EUV and radio Maxwellian projections, satisfying ΔD_KL = (3/2)[R0 − ln R0 − 1] = (3/2) d_IS(T_eff, T_core).
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Radio Wave Propagation as a Probe of the Solar Corona and Solar Wind
Radio wave distortion effects serve as established probes of solar corona and wind turbulence parameters, with SKA expected to expand observational capabilities.