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Estimates of Magnetic Field Strength in the Solar Corona Using Observations of Thermal Radio Emission at Low Frequencies

Authors: Sayuf Shaik, C. Kathiravan, R. Ramesh

Sayuf Shaik et al 2026 The Astrophysical Journal 1011 .

Provider: AAS Journals

Caption: Figure 4.

(a) Ray-tracing representation in the Sun–Earth plane. Solar north is perpendicular to the plane of the paper in the viewing direction. (b) Reflection levels of O- and E-modes near the location of maximum optical depth in the present case.

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