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

Document Type

Article

Publication Date

1-1-2005

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. © 2004 Elsevier B.V. All rights reserved.

Identifier

10444252659 (Scopus)

Publication Title

New Astronomy

External Full Text Location

https://doi.org/10.1016/j.newast.2004.10.003

ISSN

13841076

First Page

209

Last Page

218

Issue

3

Volume

10

Grant

10073019

Fund Ref

Chinese Academy of Sciences

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