Analysis of structure and development of spotless flares using digital images of the solar chromosphere

Abstract

The technique and algorithms for plotting the light curves of spotless solar flares are proposed for the study of chromosphere activity in the H-alpha line. Software for the hardware system of the Baikal astrophysical observatory is developed for computer analysis of flare development from digital images of the solar chromosphere.

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Correspondence to P. A. Konyaev.

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Original Russian Text © P.A. Konyaev, A.V. Borovik, A.A. Zhdanov, 2015, published in Optika Atmosfery i Okeana.

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Konyaev, P.A., Borovik, A.V. & Zhdanov, A.A. Analysis of structure and development of spotless flares using digital images of the solar chromosphere. Atmos Ocean Opt 29, 89–94 (2016). https://doi.org/10.1134/S1024856016010103

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Keywords

  • solar chromosphere
  • spotless flares
  • light curves