Enviar artigo por via de e-mail Analysis of structure and development of spotless flares using digital images of the solar chromosphere
- Autores: Konyaev P.A.1, Borovik A.V.2, Zhdanov A.A.2
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Afiliações:
- V.E. Zuev Institute of Atmospheric Optics, Siberian Branch
- Institute of Solar-Terrestrial Physics, Siberian Branch
- Edição: Volume 29, Nº 1 (2016)
- Páginas: 89-94
- Seção: 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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Resumo
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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Sobre autores
P. Konyaev
V.E. Zuev Institute of Atmospheric Optics, Siberian Branch
Autor responsável pela correspondência
Email: peter@iao.ru
Rússia, pl. Akademika Zueva 1, Tomsk, 634055
A. Borovik
Institute of Solar-Terrestrial Physics, Siberian Branch
Email: peter@iao.ru
Rússia, ul. Lermontova 126a, Irkutsk, 664033
A. Zhdanov
Institute of Solar-Terrestrial Physics, Siberian Branch
Email: peter@iao.ru
Rússia, ul. Lermontova 126a, Irkutsk, 664033
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