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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 6.

Simulated radio images for emission at f = 35.2 MHz, ﹩f/{f}_{\mathrm{pe}}({r}_{0})=1.10﹩, a density fluctuation level ϵ = 0.8, a level of anisotropy α = 0.1, and an emission source located at longitudes θ0 = 10°, 30°, and 50°. Each dot represents one photon. The projected position of the true radio source and the apparent source centroid are shown by the red (×) and black (+) crosses, respectively. The black ellipse shows the source area at the half-maximum level. The orange circle denotes the solar limb, and the dashed circle denotes the level where the true source is located.

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