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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 7.

Parameters of drift-pair bursts versus emission frequency. (a) Time delay between the burst components. (b) Relative intensity of the second component. Black lines show the simulation results for an emission source located at longitude θ0 = 10°, ϵ = 0.8, α = 0.1, and initial emission to plasma frequency ratios ﹩f/{f}_{\mathrm{pe}}({r}_{0})=1.05﹩ and 1.10 (marked by ﹩\square ﹩ and ﹩\diamond ﹩ symbols, respectively). The observations are plotted as indicated by the legend. Error bars represent one standard deviation.

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