Abstract
Instantaneous predictions of the maximum monthly smoothed sunspot number in solar cycle 23 have been made with a linear regressive model, which gives the predicted maximum value as a function of the smoothed sunspot numbers corresponding to a given month from the minimum in all preceding cycles. These predictions indicate that the intensity of solar activity in the current cycle will be at an average level.
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References
Denkmayr, K. and rCugnon, P.: 1997, in R. Heckman et al.(eds), Proceedings of the 5th Solar-Terrestrial Predictions Workshop, CRL, Japan, p. 103.
Hanslmeier, A., Denkmayr, K., and Weiss, P.: 1999, Solar Phys. 184: 213.
Mugellesi, R. and Kerridge, D., J.: 1991, EAS J. 15, 132.
Wang, H.-N.: 1995, Solar Phys. 157, 199.
Wang, H.-N.: 1997, Solar Phys. 174, 265.
Wang, H.-N. and Wang J.-X.: 1996, Astron. Astrophys. 313, 285.
Wilson, R.: 1988, Solar Phys. 117, 179.
Zhang, G.: 1990, in R. Thompson et al.(eds), Proceedings of the 3rd Solar-Terrestrial Predictions Workshop, Vol. 1, Leura, Australia, p. 670.
Zhang, G.: 1994, Solar Phys. 154, 41.
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Guiqing, Z., Huaning, W. Prediction of maximum sunspot number in solar cycle 23. Solar Physics 188, 397–400 (1999). https://doi.org/10.1023/A:1005282419046
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DOI: https://doi.org/10.1023/A:1005282419046