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Radio Echo in the Turbulent Corona and Simulations of Solar Drift-pair Radio Bursts

  • Authors: Alexey A. Kuznetsov, Nicolina Chrysaphi, Eduard P. Kontar, and Galina Motorina

2020 The Astrophysical Journal 898 94.

  • Provider: AAS Journals

Caption: Figure 5.

Same as in Figure 4, for ϵ = 0.8, α = 0.1, emission at f = 35.2 MHz, ﹩f/{f}_{\mathrm{pe}}({r}_{0})=1.10﹩, and emission sources located at θ0 = 30° (left column) and θ0 = 50° (right column).

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