The effect of solar wind high-speed streams on the galactic cosmic rays intensity
| Autor: | A. I. Klyuyeva, B. A. Shakhov, Yu. I. Fedorov, Yu. L. Kolesnyk |
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| Rok vydání: | 2016 |
| Předmět: |
Physics
010504 meteorology & atmospheric sciences Mean free path Astrophysics::High Energy Astrophysical Phenomena Astronomy Coronal hole Astronomy and Astrophysics Cosmic ray Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics 01 natural sciences Solar wind Space and Planetary Science 0103 physical sciences Neutron Forbush decrease Ultra-high-energy cosmic ray 010303 astronomy & astrophysics Intensity (heat transfer) 0105 earth and related environmental sciences |
| Zdroj: | Kinematics and Physics of Celestial Bodies. 32:265-275 |
| ISSN: | 1934-8401 0884-5913 |
| DOI: | 10.3103/s0884591316060039 |
| Popis: | The effect of high-speed recurrent solar wind streams from coronal holes on the galactic cosmic rays intensity is investigated. The distribution of galactic cosmic rays for different solar cycles is considered based on the data of the world network of neutron monitors. Within the inhomogeneous model, which includes a homogeneous background and regions of high-speed streams (HSS’s), the transport equation has been solved and the effect of HSS’s on the spatial distribution of galactic cosmic rays is estimated. It is shown that theoretical calculations are agreed with the experimental results obtained for 2000–2014 under different assumptions about the mean free path of cosmic rays in the corresponding period of HSS’s. |
| Databáze: | OpenAIRE |
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