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

P. A. Konyaev; A. V. Borovik; A. A. Zhdanov

doi:10.1134/S1024856016010103

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

Authors: Konyaev P.A.¹, Borovik A.V.², Zhdanov A.A.²
Affiliations:
1. V.E. Zuev Institute of Atmospheric Optics, Siberian Branch
2. Institute of Solar-Terrestrial Physics, Siberian Branch
Issue: Vol 29, No 1 (2016)
Pages: 89-94
Section: Optical Instrumentation
URL: https://journals.rcsi.science/1024-8560/article/view/187719
DOI: https://doi.org/10.1134/S1024856016010103
ID: 187719

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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.