Art
J-GLOBAL ID:201002261153103551   Reference number:10A0928569

The influence of the sidereal cosmic-ray anisotropies originated on the tail- and nose-boundaries of the heliomagnetosphere (HMS) upon the solar cosmic-ray anisotropy produced inside the HMS

HMS内部で作られる太陽宇宙線の異方性についてのへりコン磁気圏(HMS)の末端及びノーズ境界に発生する恒星宇宙線異方性の影響
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Material:
Volume: 62  Issue:Page: 525-544  Publication year: 2010 
JST Material Number: G0106B  ISSN: 1343-8832  Document type: Article
Article type: 原著論文  Country of issue: Japan (JPN)  Language: ENGLISH (EN)
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Category name(code) classified by JST.
Geomagnetic variation and pulsation 
Reference (31):
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  • DORMAN, L. I. Galactic cosmic ray distribution in interplanetary space expected on the basis of anisotropic diffusion theory including the actual distribution of solar activity over solar disc. Proc. 13th Int. Cosmic Ray Conf. (Denver), 1973. 1973, 2, 713
  • EARL, J. A. The effect of adiavatic focusing upon charged particle propagation in random magnetic field. Astrophys. J. 1976, 205, 900
  • FISK, L. A. Solar modulation of galactic cosmic rays, 2. J. Geophys. Res. 1971, 76, 221
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