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- Title
The effect of solar wind high-speed streams on the galactic cosmic rays intensity.
- Authors
Kolesnyk, Yu.; Klyuyeva, A.; Shakhov, B.; Fedorov, Yu.
- Abstract
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.
- Subjects
GALACTIC cosmic rays; TRANSPORT theory; SPATIAL distribution (Quantum optics); NEUTRON transport theory; SOLAR wind
- Publication
Kinematics & Physics of Celestial Bodies, 2016, Vol 32, Issue 6, p265
- ISSN
0884-5913
- Publication type
Article
- DOI
10.3103/S0884591316060039