A method to evaluate the level of solar activity at the remainder of a progressing solar cycle

Details A method to evaluate the level of solar activity at the remainder of a progressing solar cycle A method to evaluate the level of solar activity at the remainder of a progressing solar cycle

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005newa...10..209l&link_type=abstract

New Astronomy, Volume 10, Issue 3, p. 209-218.

Astronomy and Astrophysics

Astronomy

1

96.60.-J, 96.60.Qc

Scientific paper

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.

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