Abstract
Statistical analysis of a large amount of data for three solar activity cycles (1975–2005) shows that the magnitude and other characteristics of Forbush effects are related to the intensity and longitude of previous solar flares.
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Iucci, N., Parisi, M., Storini, M., and Villoresi, G., Nuovo Cimento. C, 1984, vol. 7, p. 467.
Cane, H.V., Richardson, I.G., and von Rosenvinge, T.T., J. Geophys. Res., 1996, vol. 101, p. 21 561.
Cane, H.V., Space Sci. Rev., 2000, vol. 93, p. 41.
Belov, A.V., Garsia, G., Kurt, W., and Mavromichalaki, E., Kosm. Issled., 2005, vol. 43, p. 171.
Belov, A.V., Eroshenko, E.A., and Yanke, V.G., Abstracts of Papers, Proc. 27th ICRC, Hamburg, 1999, vol. 6, p. 431.
Sinno, K., Rep. Ionos. Space Res. Jpn., 1961, vol. 15, p. 276.
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Original Russian Text © A.V. Belov, E.A. Eroshenko, V.A. Oleneva, V.G. Yanke, 2007, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2007, Vol. 71, No. 7, pp. 1019–1021.
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Belov, A.V., Eroshenko, E.A., Oleneva, V.A. et al. Relationship between Forbush effects and X-ray flares. Bull. Russ. Acad. Sci. Phys. 71, 988–990 (2007). https://doi.org/10.3103/S1062873807070283
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DOI: https://doi.org/10.3103/S1062873807070283