期刊文献+

The prediction method of similar cycles 被引量:3

The prediction method of similar cycles
下载PDF
导出
摘要 The concept of degree of similarity (η), is proposed to quantitatively describe the similarity of a parameter (e.g. the maximum amplitude Rmax) of a solar cycle relative to a referenced one, and the prediction method of similar cycles is further developed. For two parameters, the solar minimum (Rmin) and rising rate (βa), which can be directly measured a few months after the minimum, a synthesis degree of similarity (ηs) is defined as the weighted-average of the η values around Rmin and βa, with the weights given by the coefficients of determination of Rmax with Rmin and βa, respectively. The monthly values of the whole referenced cycle can be predicted by averaging the corresponding values in the most similar cycles with the weights given by the ηs values. As an application, Cycle 24 is predicted to peak around January 2013 i8 (month) with a size of about Rmax = 84 ± 17 and to end around September 2019. The concept of degree of similarity (η), is proposed to quantitatively describe the similarity of a parameter (e.g. the maximum amplitude Rmax) of a solar cycle relative to a referenced one, and the prediction method of similar cycles is further developed. For two parameters, the solar minimum (Rmin) and rising rate (βa), which can be directly measured a few months after the minimum, a synthesis degree of similarity (ηs) is defined as the weighted-average of the η values around Rmin and βa, with the weights given by the coefficients of determination of Rmax with Rmin and βa, respectively. The monthly values of the whole referenced cycle can be predicted by averaging the corresponding values in the most similar cycles with the weights given by the ηs values. As an application, Cycle 24 is predicted to peak around January 2013 i8 (month) with a size of about Rmax = 84 ± 17 and to end around September 2019.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2011年第12期1482-1492,共11页 天文和天体物理学研究(英文版)
基金 supported by the National Natural Science Foundation of China(Grant Nos.10973020,40890161 and 10921303) the National Basic Research Program of China(973 Program Grant No.2011CB811406)
关键词 Sun: activity -- Sun: general -- sunspots Sun: activity -- Sun: general -- sunspots
  • 相关文献

参考文献35

  • 1Cameron, R., & Schussler, M. 2008, ApJ, 685, 1291.
  • 2Dikpati, M., de Toma, G., & Gilman, P. A. 2006, Geophys. Res. Lett., 330, L05102.
  • 3Du, Z. L. 2011a, Sol. Phys., 270, 407.
  • 4Du, Z. L. 2011b, Sol. Phys., 273, 231 (DOI: 10.1007/s11207-011-9849-8).
  • 5Du, Z. L., & Wang, H. 2011, Science in China G: Physics and Astronomy, 54, 172.
  • 6Du, Z. L. 2006, AJ, 132, 1485.
  • 7Du, Z. L., Li, R., & Wang, H. N. 2009a, AJ, 138, 1998.
  • 8Du, Z. L., Wang, H., & Zhang, L. 2009b, Sol. Phys., 255, 179.
  • 9Du, Z.-L., & Wang, H.-N. 2010, RAA (Research -in Astronomy and Astrophysics), 10, 950.
  • 10Du, Z.-L., Wang, H.-N., & Zhang, L.-Y. 2008, ChJAA (Chin. J. Astron. Astrophys.), 8, 477.

同被引文献39

引证文献3

二级引证文献18

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部