Abstract
The well known Waldmeier rule and its modifications applied to forecasting of the solar activity are discussed. The maximum annual mean rate of the increase in the magnetic flux observed on the growth branch of the cycle is proposed as a predicting (diagnosing) parameter for the amplitude of the cycle currently in progress. The maximum Wolf number of the current (24th) cycle is estimated to reach 104 (±12) or more, and to occur in 2013 or later. The yearly average Wolf numbers observed during the 24th cycle are presented.
Similar content being viewed by others
References
M. Waldmeier, Results and Problems of Solar Studies (Geest and Portig, Leipzig, 1955; Inostr. Liter., Moscow, 1950).
Yu. I. Vitinskii, Cyclicity and Solar-activity Forecasting (Nauka, Moscow, 1973) [in Russian].
V. I. Makarov, A. G. Tlatov, D. K. Callebaut, et al., Solar Phys. 198, 409 (2001).
Yu. A. Nagovitsyn, Astron. Lett. 32, 344 (2006).
A. G. Tlatov, Solar Phys. 260, 465 (2009).
I. S. Veselovsky and M. V. Tarsina, Adv. Space Res. 29, 417 (2002).
Yu. A. Nagovitsyn, Astron. Lett. 23, 735 (1997).
M. Schussler, Astron. Nachr. 328, 1087 (2007).
K. Petrovay, Living Rev. Solar Phys. 7, 1 (2010).
D. V. Hoyt and K. H. Schatten, Solar Phys. 181, 491 (1998).
Yu. A. Nagovitsyn, Astron. Lett. 31, 557 (2005).
Yu. A. Nagovitsyn, Astron. Lett. 33, 340 (2007).
L. A. Aguirre, C. Letellier, and J. Maquet, Solar Phys. 249, 103 (2008).
I. Kitiashvili and A. G. Kosovichev, Astrophys. J. 688, L49 (2008).
A. Kilcik, C. N. K. Anderson, J. P. Rozelot, et al., Astrophys. J. 693, 1173 (2009).
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © Yu.A. Nagovitsyn, A.I. Kuleshova, 2012, published in Astronomicheskii Zhurnal, 2012, Vol. 89, No. 10, pp. 883–887.
Rights and permissions
About this article
Cite this article
Nagovitsyn, Y.A., Kuleshova, A.I. The Waldmeier rule and early diagnostics of the maximum of the current solar cycle. Astron. Rep. 56, 800–804 (2012). https://doi.org/10.1134/S1063772912090065
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1063772912090065