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Sunspot changes following proton flares
Published online by Cambridge University Press: 14 August 2015
Abstract
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Although the area of some sunspot groups declines suddenly after a flare that produces energetic protons, other groups show a delayed or gradual decline, or continue to grow for several days after the flare. The mean area of sunspot groups that produced flares with polar-cap absorption declines gradually and continuously, beginning within a day after the flare.
- Type
- Part VII: Proton Flare Project (PFP)
- Information
- Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 543 - 550
- Copyright
- Copyright © Reidel 1968
References
Gopasyuk, S.I., Ogir, M.B., Severny, A.B., Shaposhnikova, E.F. (1963) Izv. Krym. astrofiz. Obs., 29, 15.Google Scholar
Greenwich Photoheliographic Results 1942 and 1946, Her Majesty's Stationery Office, London.Google Scholar
Severny, A.B. (1967) Preliminary communication of results presented at IQSY Meeting, London, July.Google Scholar
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