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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 4.

Simulated time profiles for a level of density fluctuations ϵ = 0.8, an emission source located at θ0 = 10°, an emission frequency of f = 35.2 MHz, f/fpe(r0) = 1.10, and anisotropy α = 0.1 (left column), 0.2 (middle column), and 0.3 (right column). Top row: the radio flux (normalized by the maximum value) where the blue and red lines represent the signal with and without collisional absorption, respectively. Middle row: the apparent radio source position (distance from the solar disk center). Bottom row: the apparent radio source area (at half-maximum level). Error bars represent one standard deviation.

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