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New Evidence for Spatio-temporal Fragmentation in the Solar Flare Energy Release

  • Authors: R. Ramesh, V. Mugundhan, and K. Prabhu

2020 The Astrophysical Journal Letters 889 L25.

  • Provider: AAS Journals

Caption: Figure 3.

GRIP observations (at 80 MHz) of the Stokes I and V time profiles of the type III burst group in Figure 1, and the scaled light curve of the flare observed with the KSO Hα telescope during the same time interval. Shape preserving spline interpolation was used for the Hα light curve. The profiles (black color) in solid and dotted lines correspond to Stokes I and V emission, respectively.

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