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


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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.

作者简介

P. Konyaev

V.E. Zuev Institute of Atmospheric Optics, Siberian Branch

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Email: peter@iao.ru
俄罗斯联邦, pl. Akademika Zueva 1, Tomsk, 634055

A. Borovik

Institute of Solar-Terrestrial Physics, Siberian Branch

Email: peter@iao.ru
俄罗斯联邦, ul. Lermontova 126a, Irkutsk, 664033

A. Zhdanov

Institute of Solar-Terrestrial Physics, Siberian Branch

Email: peter@iao.ru
俄罗斯联邦, ul. Lermontova 126a, Irkutsk, 664033

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