Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10704652 | New Astronomy | 2005 | 10 Pages |
Abstract
A modified method is developed to evaluate the level of solar activity at the remainder of a progressing solar cycle based on a method previously proposed by [Li, K.J., Zhan, L.S., Wang, J.X., et al., 2002a. A&A 392, 301]. The behavior of sunspot numbers at the remainder of cycle 23 is studied. A comparison of different methods that predict sunspot numbers of a whole cycle is also given in this paper.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
K.J. Li, J. Qiu, F.Y. Xiang, P.X. Gao, T.W. Su,