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Methods for the Forecasting of Solar Flares

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  • First Online:
Solar-Terrestrial Physics/1970

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 29))

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Abstract

Flares appear only in regions on the sun with strong magnetic fields, mostly in sunspot groups. Two circumstances are of great importance for the forecasting of flares:

  1. (a)

    the character of the regions producing flares of a certain importance,

  2. (b)

    the characteristic features of the evolution of active regions.

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Author information

Authors and Affiliations

  1. Crimean Astrophysical Observatory, Russia

    A. B. Severny & N. V. Steshenko

Authors
  1. A. B. Severny
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  2. N. V. Steshenko
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Editor information

E. R. Dyer

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© 1972 Springer Science+Business Media Dordrecht

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Severny, A.B., Steshenko, N.V. (1972). Methods for the Forecasting of Solar Flares. In: Dyer, E.R. (eds) Solar-Terrestrial Physics/1970. Astrophysics and Space Science Library, vol 29. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3693-5_13

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  • DOI: https://doi.org/10.1007/978-94-009-3693-5_13

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  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8154-2

  • Online ISBN: 978-94-009-3693-5

  • eBook Packages: Springer Book Archive

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