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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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
- solar chromosphere
- spotless flares
- light curves