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:
-
(a)
the character of the regions producing flares of a certain importance,
-
(b)
the characteristic features of the evolution of active regions.
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Severny, A.B., Steshenko, N.V. (1972). Methods for the Forecasting of Solar Flares. In: de Jager, C., Dyer, E.R. (eds) Solar-Terrestrial Physics/1970. Astrophysics and Space Science Library, vol 29. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3126-4_13
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DOI: https://doi.org/10.1007/978-94-010-3126-4_13
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