Heliospheric modulation of high-energy cosmic rays: I. Basic model of cosmic-ray modulation with solar cycle

被引：0
作者：
G. F. Krymsky
P. A. Krivoshapkin
V. P. Mamrukova
S. K. Gerasimova
机构：
[1] Russian Academy of Sciences,Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
来源：
Journal of Experimental and Theoretical Physics | 2007年 / 104卷
关键词：
96.50.S-; 96.50.Xy; 96.60.Q-;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We have constructed a greatly simplified theory for the heliospheric modulation of high-energy cosmic rays in which no adjustable parameters are used. The only parameter k, which characterizes the degree of regularity of the interplanetary magnetic field, varies in the model in a definite way with solar cycle phase. The approximations used lead to solutions expressed in terms of elementary functions. The role of the magnetic drift of particles has been revealed. Quantitative agreement with the observed cosmic-ray variations has been achieved.
引用
收藏
页码：189 / 195
页数：6
相关论文
共 33 条
  • [1] Charakhchyan A. N.(1973)undefined Izv. Akad. Nauk SSSR, Ser. Fiz. 33 1258-undefined
  • [2] Bazilevskaya G. A.(2005)undefined J. Geophys. Res. 110 A10106-undefined
  • [3] Svirzhevskaya A. K.(1991)undefined Planet. Space Sci. 39 1617-undefined
  • [4] Ahluwalia H. S.(1997)undefined Nuovo Cimento C 20 871-undefined
  • [5] Nagashima K.(1976)undefined J. Geophys. Res. 81 2082-undefined
  • [6] Fujimoto K.(1977)undefined Astrophys. J. 213 861-undefined
  • [7] Tatsuoka R.(1981)undefined Astrophys. J. 243 1115-undefined
  • [8] Storini M.(1983)undefined Astrophys. J. 265 573-undefined
  • [9] Levy E. H.(2001)undefined Space Sci. Rev. 98 327-undefined
  • [10] Jokipii J. R.(2001)undefined Space Sci. Rev. 97 295-undefined
1234