Отправить статью по E-mail Construction of the light curves for solar flares in the Hα line
- Авторы: Borovik A.V.1, Konyaev P.A.2, Zhdanov A.A.1
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Учреждения:
- Institute of Solar–Terrestrial Physics, Siberian Branch
- V.E. Zuev Institute of Atmospheric Optics, Siberian Branch
- Выпуск: Том 56, № 5 (2016)
- Страницы: 513-523
- Раздел: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/155746
- DOI: https://doi.org/10.1134/S0016793216050029
- ID: 155746
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Аннотация
The results of an investigation of some factors affecting the construction of the light curves for solar flares in the Hα line are presented. It is determined that the type of the light curve depends on the method of measuring the intensity, the size of the measurement window, and the brightness fluctuations of the quiet chromosphere areas (the reference areas). The light curves constructed on the basis of the flare’s peak intensity show a real picture of the flare development process. A method for the selection of the “reference areas” is suggested.
Об авторах
A. Borovik
Institute of Solar–Terrestrial Physics, Siberian Branch
Автор, ответственный за переписку.
Email: aborovik@iszf.irk.ru
Россия, Irkutsk
P. Konyaev
V.E. Zuev Institute of Atmospheric Optics, Siberian Branch
Email: aborovik@iszf.irk.ru
Россия, Tomsk
A. Zhdanov
Institute of Solar–Terrestrial Physics, Siberian Branch
Email: aborovik@iszf.irk.ru
Россия, Irkutsk
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