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

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• 作者：P. A. Konyaev ; A. V. Borovik ; A. A. Zhdanov
• 关键词：solar chromosphere ; spotless flares ; light curves
• 刊名：Atmospheric and Oceanic Optics
• 出版年：2016
• 出版时间：January 2016
• 年：2016
• 卷：29
• 期：1
• 页码：89-94
• 全文大小：2,893 KB
• 参考文献：1.L. Fletcher, B. R. Dennis, H. S. Hudson, S. Krucher, K. Phillips, A. Veronig, M. Battaglia, L. Bone, A. Caspi, Q. Chen, P. Gallagher, P. T. Grigis, H. Ji, W. Liu, R. O. Milligan, and M. Temmer, “An observational overview of solar flares,” Space Sci. Rev. 159, 19–106 (2011).ADS CrossRef
  2.A. V. Borovik, D. Yu. Myachin, and V. M. Tomozov, “Observations of spotless solar flares in Baikal astrophysical observatory of the ISTP SB RAS and their interpretation,” Izv. Irkutsk. Gos. Univ., Ser. Nauki Zemle, No. 7, 23–45 (2014).
  3.P. A. Konyaev and A. V. Borovik, “Studying the astroclimate at Baikal astrophysical observatory by optical methods,” Atmos. Ocean. Opt. 27 (2), 130–133 (2014).CrossRef
  4.A. V. Borovik and P. A. Konyaev, “The astronomical climate of the ISTP SB RAS Baikal Astrophysical Observatory,” Izv. Irkutsk. Gos. Univ., Ser. Nauki Zemle, No. 8, 25–34 (2014).
  5.T. S. Razmadze, “Photometry of chromospheric flares,” Bul. Abastumanskoi Astrofizich. Observatorii, No. 29, 3–27 (1962).
  
• 作者单位：P. A. Konyaev (1)
  A. V. Borovik (2)
  A. A. Zhdanov (2)
  
  1. V.E. Zuev Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences, pl. Akademika Zueva 1, Tomsk, 634055, Russia
  2. Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, ul. Lermontova 126a, Irkutsk, 664033, Russia
  
• 刊物类别：Physics and Astronomy
• 刊物主题：Physics
  Applied Optics, Optoelectronics and Optical Devices
  Russian Library of Science
  
• 出版者：MAIK Nauka/Interperiodica distributed exclusively by Springer Science+Business Media LLC.
• ISSN：2070-0393

文摘

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.