Open Access
Issue
J. Space Weather Space Clim.
Volume 1, Number 1, 2011
Article Number A01
Number of page(s) 3
DOI https://doi.org/10.1051/swsc/2011110013
Published online 17 August 2011
  • Brajša, R., H. Wöhl, A. Hanslmeier, G. Verbanac, D. Ruždjak, E. Cliver, L. Svalgaard, and M. Roth, Prediction for the 24th Solar Cycle, Central European Astrophys. Bull., 33, 95–98, 2009.
  • Cameron, R., and M. Schüssler, Solar cycle prediction using precursors and flux transport models, The Astrophys. J., 659 (1), 801–811, 2007. [NASA ADS] [CrossRef]
  • Cameron, R., and M. Schüssler, A robust correlation between growth rate and amplitude of solar cycles: consequences for prediction methods, The Astrophys. J., 685, 1291–1296, 2008. [NASA ADS] [CrossRef]
  • Choudhuri, A. R., P. Chatterjee, and J. Jiang, Predicting solar cycle 24 with a solar dynamo model, Phys. Rev. Lett., 98, 131103, 2007. [NASA ADS] [CrossRef] [PubMed]
  • Feynman, J., Geomagnetic and solar wind cycles, 1900–1975, J. Geophys. Res., 87, 6153–6162, 1982. [CrossRef]
  • Gonzalez, G., and K. H. Schatten, Using geomagnetic indices to forecast the next sunspot maximum, Solar Phys., 114, 189–192, 1987.
  • HathawayD. H., Solar cycle forecasting, Space Sci. Rev., 144, 401–412, 2009. [NASA ADS] [CrossRef]
  • Hathaway, D. H., R. M. Wilson, E. J. Reichmann, A synthesis of solar cycle prediction techniques, J. Geophys. Res., 104 (A10), 22.375–22.388, 1999. [NASA ADS] [CrossRef]
  • Javaraiah J., North-south asymmetry in solar activity: predicting the amplitude of the next solar cycle, Mon. Not. R. Astron. Soc., 377, L34–L38, 2007. [NASA ADS] [CrossRef]
  • Kane, R. P., Prediction of solar cycle maximum using solar cycle lengths, Solar Phys., 248 (1), 203–209, 2008. [CrossRef]
  • Lantos, P., The skewness of a solar cycle as a precursor of the amplitude of the next, Solar Phys., 236, 199–205, 2006. [NASA ADS] [CrossRef]
  • Maris, G., M.D. Popescu, and D. Besliu, Solar cycle 23: forecasts and observations, Rom. Astron. J., 13 (2), 139–142, 2003.
  • Ohl, A. I., and G. I. Ohl, A new method of very long-term prediction of solar activity, NOAA Solar-Terr. Pred. Proc., 2, 268–263, 1979.
  • Podladchikova, T., B. Lefebvre, and R. Van der Linden, Integral activity of the declining phase of sunspot cycles as precursor of the next cycle, J. Atm. Solar-Terr. Phys., 70, 277–284, 2008. [CrossRef]
  • Ramaswamy G., Sunspot cycles and solar activity forecasting, Nature, 265, 713–715, 1977. [CrossRef]
  • Sargent H. H., A prediction for the next sunspot ctcle, 28th IEEE Vehicular Tech Conf. Proc., 490–496, 1978. [CrossRef]
  • Schatten, K., Fair space weather for solar cycle 24, Geophys. Res. Lett., 32, L21106, 2005. [NASA ADS] [CrossRef]
  • Schatten, K., and S. Sofia, Forecast of an exceptionally large even-numbered solar cycle, Geophys. Res. Lett., 14, 632–635, 1987. [CrossRef]
  • Schatten, K. H., and W. K. Tobiska, Solar activity heading for a Maunder minimum?, Bull. Am. Astro.Soc., 35, 817, 2003.
  • Schatten, K. H., P. H. Scherrer, L. Svalgaard, and J. M. Wilcox, Using dynamo theory to predict the sunspot number during solar cycle 21, Geophys. Res. Lett., 5, 411–414, 1978. [NASA ADS] [CrossRef]
  • Svalgaard, L., E. W. Cliver, and Y. Kamide, Cycle 24: the smallest sunspot cycle in 100 years?, Geophys. Res. Lett., 32 (1), L01104, 2005. [NASA ADS] [CrossRef]
  • Thomson, R. J., A technique for predicting the amplitude of the solar cycle, Solar phys., 148, 383–388, 1993. [NASA ADS] [CrossRef]
  • Wilson, R. M., D. H. Hathaway, and E. J. Reichmann,, An estimate for the size of cycle 23 based on near minimum conditions, J. Geophys. Res., 103, 6595–6603, 1998. [NASA ADS] [CrossRef]

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.