On the formation of spot and magnetic cycles in the galactic cosmic ray intensity in the minima of solar activity

被引:0
作者
M. B. Krainev
M. S. Kalinin
机构
[1] Russian Academy of Sciences,Lebedev Physical Institute
来源
Bulletin of the Lebedev Physics Institute | 2012年 / 39卷
关键词
Sun; heliosphere; galactic cosmic rays; spot-forming activity cycle; magnetic cycle; solar cycle minimum;
D O I
暂无
中图分类号
学科分类号
摘要
The problems of the determination and separation of variations in the galactic cosmic ray intensity, caused by the spot-forming activity and polarity of high-latitude solar magnetic fields, are discussed. Based on the solution of the boundary-value problem, some features in the intensity formation at solar cycle minima are formulated.
引用
收藏
页码:175 / 180
页数:5
相关论文
共 12 条
  • [1] Bazilevskaya G. A.(2011)undefined Izv. RAN. Ser. Fiz. 75 849-undefined
  • [2] Jokipii J. R.(1977)undefined Astrophys. J. 213 861-undefined
  • [3] Levy E. H.(2011)undefined Izv. RAN. Ser. Fiz. 75 853-undefined
  • [4] Hubbard W. B.(1964)undefined Geomagnetizm i Aeronomiya 4 977-undefined
  • [5] Krainev M. B.(1958)undefined Phys. Rev. 110 1445-undefined
  • [6] Kalinin M. S.(2001)undefined Space Sci. Rev. 97 295-undefined
  • [7] Krymskii G. F.(2011)undefined Astrophys. Space Sci. Trans. 7 379-undefined
  • [8] Parker E. N.(2003)undefined Izv. RAN. Ser. Fiz. 67 1435-undefined
  • [9] Potgieter M. S.(undefined)undefined undefined undefined undefined-undefined
  • [10] Stozhkov Y. I.(undefined)undefined undefined undefined undefined-undefined