Abstract
The correlation between the characteristics (sunspot area and galactic cosmic ray intensity) at inflection points and at the solar cycle maximum is discussed. Probable characteristics in the forthcoming maximum of cycle 24 are considered.
Similar content being viewed by others
References
G. A. Bazilevskaya and A. K. Svirzhevskaya, Space Sci. Rev. 85, 431 (1998).
G. A. Bazilevskaya et al., Solar Phys. 197, 157 (2000).
M. B. Krainev, Kratkie Soobshcheniya po Fizike FIAN 39(4), 3 (2012) [Bulletin of the Lebedev Physics Institute 39, 95 (2012)].
Yu. A. Nagovitsyn, Astrofiz. Bull. 63, 45 (2008) [Astrophys. Bull. 63, 45 (2008)].
N. R. Sheeley, Jr., ASP Conf. Ser. 428, 3 (2010).
Yu. I. Stozhkov et al., Preprint No. 14 (Lebedev Physical Institute, Russian Academy of Sciences, 2007].
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © M.B. Krainev, 2013, published in Kratkie Soobshcheniya po Fizike, 2013, Vol. 40, No. 1, pp. 3–9.
About this article
Cite this article
Krainev, M.B. On the characteristics of solar activity and galactic cosmic ray intensity at the solar cycle maximum and inflection points. Bull. Lebedev Phys. Inst. 40, 1–5 (2013). https://doi.org/10.3103/S1068335613010016
Received:
Published:
Issue Date:
DOI: https://doi.org/10.3103/S1068335613010016