Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Yu. I. Fedorov"'
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
Autor:
Yu. I. Fedorov, I. M. Mingazov
Publikováno v:
Herald Of Technological University. 25:46-50
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b0a39e3e99328c94945143a293c34fb7
https://doi.org/10.55421/1998-7072_2022_25_10_46
https://doi.org/10.55421/1998-7072_2022_25_10_46
Autor:
Yu. I. Fedorov
Publikováno v:
Kinematics and Physics of Celestial Bodies. 37:107-120
The propagation of cosmic rays in the interplanetary medium is considered based on the kinetic Fokker–Planck equation. The analytical expression for the anisotropic part of the cosmic ray distribution function is derived in the approximation of sma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7d249d21882c1c5b39fd563a4eb5ea4b
https://doi.org/10.3103/s088459132103003x
https://doi.org/10.3103/s088459132103003x
Publikováno v:
Chemical and Petroleum Engineering. 56:761-769
An alternative method for determining the empirical coefficients of the Kunin-Yurchenko equation of pressing is proposed. This method consists in constructing a polynomial regression tertiary model of the dependence of the density on the pressing pre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::96a5c00905c04a70a122daa6dcbb425b
https://doi.org/10.1007/s10556-021-00839-7
https://doi.org/10.1007/s10556-021-00839-7
Autor:
Yu. I. Fedorov
Publikováno v:
Kinematics and Physics of Celestial Bodies. 36:103-113
The propagation of solar cosmic rays in the interplanetary medium is considered on the basis of the kinetic equation describing the small-angle multiple scattering of charged particles. Energetic particles are assumed to be injected into the interpla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::da27e42ec937374cd4af2774cd31052a
https://doi.org/10.3103/s0884591320030034
https://doi.org/10.3103/s0884591320030034
Autor:
Yu. I. Fedorov
Publikováno v:
Kinematics and Physics of Celestial Bodies. 35:203-216
—The propagation of solar cosmic rays (SCR) in the interplanetary medium is considered on the basis of the Fokker–Planck kinetic equation. It is known that the SCR distribution function averaged over a solar proton event contains valuable data on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::028ed2afc30081dc218f84603b891c11
https://doi.org/10.3103/s0884591319050039
https://doi.org/10.3103/s0884591319050039
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
Autor:
Yu. I. Fedorov
Publikováno v:
Kinematics and Physics of Celestial Bodies. 35:1-16
The acceleration of energetic particles and their propagation in magnetic fields of the solar wind and the Galaxy is a topical astrophysical problem. Cosmic rays (CR) affect communications and the operation of on-board spacecraft electronics and dist
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3f08f2a5260ddff1f0af7488f672caaa
https://doi.org/10.3103/s0884591319010021
https://doi.org/10.3103/s0884591319010021
Autor:
B. A. Shakhov, Yu. I. Fedorov
Publikováno v:
Kinematics and Physics of Celestial Bodies. 34:107-122
The propagation of solar cosmic rays in interplanetary space is considered based on the kinetic equation. The expression for cosmic ray density under instantaneous particle injection by a point-like source is obtained. The set of a differential equat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d2707ea8771b86d516836ac287e13d66
https://doi.org/10.3103/s0884591318030042
https://doi.org/10.3103/s0884591318030042
Autor:
Yu. I. Fedorov
Publikováno v:
Kinematics and Physics of Celestial Bodies. 34:1-12
The propagation of solar cosmic rays in the interplanetary space is analyzed by solving the Fokker–Planck equation in the small-angle approximation. The particle source is assumed to be instantaneous and point-like. The spatiotemporal distribution
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4275ae3fe12e2107e2fff2a0f3c6401c
https://doi.org/10.3103/s0884591318010038
https://doi.org/10.3103/s0884591318010038