Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Yu. L. Kolesnyk"'
Publikováno v:
Kinematics and Physics of Celestial Bodies. 38:181-189
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ec999050ed2a3beba08e412071fe9a77
https://doi.org/10.3103/s0884591322040043
https://doi.org/10.3103/s0884591322040043
Publikováno v:
Kinematics and Physics of Celestial Bodies. 35:153-163
—The propagation of high-energy charged particles in the magnetic field, which is a superposition of the mean homogeneous magnetic field and magnetic inhomogenieties of various scales, is considered on the basis of the Fokker-Planck kinetic equatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::12f2a6c3159a49c00197206842033607
https://doi.org/10.3103/s0884591319040056
https://doi.org/10.3103/s0884591319040056
Publikováno v:
Kinematics and Physics of Celestial Bodies. 33:1-12
The process of heliospheric modulation of intensity of galactic cosmic rays is investigated by solving the transport equation. The spatial-energetic distribution of cosmic rays in the present epoch and in the past is analyzed. It is demonstrated that
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ef03dadba37cb49fae4ce266e59816a4
https://doi.org/10.3103/s0884591317010032
https://doi.org/10.3103/s0884591317010032
Publikováno v:
Kinematics and Physics of Celestial Bodies. 32:265-275
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 o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e33b6105a97ca46e6b5bdfbb791d72c1
https://doi.org/10.3103/s0884591316060039
https://doi.org/10.3103/s0884591316060039
Publikováno v:
Kinematics and Physics of Celestial Bodies. 32:105-119
Ultrahigh energy cosmic rays (UHECRs, E > 1018 eV) from extragalactic sources deviate in the galactic and intergalactic magnetic fields, which explains the diffusive character of their propagation, the isotropization of their total flux, and the abse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6c0a9ca9ae4594103f4b8a6af8a53add
https://doi.org/10.3103/s088459131603003x
https://doi.org/10.3103/s088459131603003x
Publikováno v:
Kinematics and Physics of Celestial Bodies. 31:161-171
Propagation of cosmic rays in the interplanetary space that accelerated during the solar flare on January 20, 2005 is investigated based on the kinetic equation. The cases of instantaneous and continuous particle injection into the interplanetary med
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::90ffcb139ff1b2b5fcf2ad5d8b868423
https://doi.org/10.3103/s0884591315040042
https://doi.org/10.3103/s0884591315040042
Autor:
Yu. L. Kolesnyk, B. A. Shakhov
Publikováno v:
Kinematics and Physics of Celestial Bodies. 31:19-24
Two problems of the stationary galactic cosmic ray (GCR) modulation in the closed heliospheric model are considered. It is assumed that the heliosphere is a spherically symmetric medium, which is limited by the heliopause, and GCRs propagate from it
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::06be8a08c1a31bcd760360b13635f4e7
https://doi.org/10.3103/s0884591315010055
https://doi.org/10.3103/s0884591315010055
Autor:
B. A. Shakhov, Yu. L. Kolesnyk
Publikováno v:
Kinematics and Physics of Celestial Bodies. 25:213-219
The termination shock at the heliospheric boundary is simulated in terms of a two-layer turbulent medium for which the average radial component of solar wind velocity is nonzero inside the heliosphere and zero for external magnetic inhomogeneities. G
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6c85977a087ca3f1a840da29c46513c1
https://doi.org/10.3103/s0884591309040072
https://doi.org/10.3103/s0884591309040072
Autor:
Yu L Kolesnyk, B. A. Shakhov
Publikováno v:
Journal of Physics: Conference Series. 409:012154
Standard model of galactic cosmic rays (GCR) propagation in heliosphere and adjacent interstellar space is considered. Here heliosphere is considered as a two-layered medium consisting of two spherical regions symmetrical about the Sun and adjacent t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b9c057bf7b5dd11250801c78989ca266
https://doi.org/10.1088/1742-6596/409/1/012154
https://doi.org/10.1088/1742-6596/409/1/012154