Cycles of solar activity and the configurations of planets

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• 作者：V. P. Okhlopkov (1) okhlopkov@taspd.sinp.msu.ru
• 关键词：mean difference of heliocentric longitudes of planets – ; frequency spectra – ; center of mass of the Solar system – ; solar activity
• 刊名：Moscow University Physics Bulletin
• 出版年：2012
• 出版时间：July 2012
• 年：2012
• 卷：67
• 期：4
• 页码：377-383
• 全文大小：332.1 KB
• 参考文献：1. R. Wolf, Astr. Mitt. 8, 183 (1859).
  2. E. W. Brown, Mon. Not. Roy. Astron. Soc. 60, 599 (1900).
  3. V. B. Shostakovich, Tr. Irkutsk. Magn. Observ., Nos. 2–3 (1928).
  4. J. Malberet, L’Astronomie 39, 503 (1925).
  5. H. H. Clayton, Smith. Misc. Coll. 106, 3870 (1947).
  6. F. D. Jose, Astron. J. 70, 193 (1965).
  7. V. G. Surdin, in Dynamics of Star Systems (URSS, Moscow, 2001), p. 32 [in Russian].
  8. M. Trellis, Compt. Rend. Acad. Sci. Paris 262, 376 (1966).
  9. R. V. Fairbridge and J. N. Shirley, Solar Phys. 110, 191 (1987).
  10. I. Charvatova and J. Strejntik, Bull. Astron. Czech. 42, 90 (1991).
  11. B. C. Prokudina, Tr. Gos. Astron. Inst. P.K. Shternberga 64, 145 (1995).
  12. A. I. Khlystov, Vestn. Kiev. Univ., No. 24, 61 (1982).
  13. A. I. Khlystov, Tr. Gos. Astron. Inst. P.K. Shternberga 62, 111 (1991).
  14. A. I. Khlystov, V. P. Dolgachev, and L. M. Domozhilova, Biofizika 37, 547 (1992).
  15. A. I. Khlystov, V. P. Dolgachev, and L. M. Domozhilova, Tr. Gos. Astron. Inst. P.K. Shternberga 64, 91 (1995).
  16. V. P. Okhlopkov, Moscow Univ. Phys. Bull. 66, 634 (2011).
  17. I. F. Nikulin, in Proceedings of the Cycles of Activity on Sun and Stars, Moscow, Russia, 2009 (Glav. Astron. Observ. Ross. Akad. Nauk, Saint Petersburg, 2009).
  18. V. A. Sukharev, All Catastrophes of the Earth (Enio, Odessa, 2004) [in Russian].
• 作者单位：1. Skobeltsyn Nuclear Physics Research Institute, Moscow State University, Moscow, 119991 Russia
• ISSN：1934-8460

文摘

In this paper, using the parameter—the average difference between the heliocentric longitudes of the planets Venus, Earth and Jupiter—the strong link found 22-year and 11-year cycles of solar activity with the lowest values of the parameter. The envelope curve of the minimum values of this parameter is well described as the conjunctions of the three planets, when they are almost in a straight line from the sun, which causes the maximum of solar activity, and the conjunctions in the larger longitudinal sector (25–30 degrees), which occur much more frequently and are accompanied by different combinations of planets on the opposite side of the Sun, which also cause the maximum of solar activity. Location of these planets on opposite sides of the Sun in various combinations is very well compatible with the parameter used.