Zobrazeno 1 - 10
of 490
pro vyhledávání: '"V. S. Beskin"'
Autor:
V. I. Krauz, V. P. Vinogradov, A. M. Kharrasov, V. V. Myalton, K. N. Mitrofanov, V. S. Beskin, Yu. V. Vinogradova, I. V. Il’ichev
Publikováno v:
Astronomy Reports. 67:15-26
Autor:
V. S. Beskin
Publikováno v:
Astronomy Reports. 67:27-34
Autor:
D. B. Melrose
Publikováno v:
Science. 264:853-853
Publikováno v:
Astronomy Letters. 47:686-694
Autor:
V. S. Beskin, V. V. Myalton, S. S. Anan’ev, V. I. Krauz, I. V. Il’ichev, K. N. Mitrofanov, A. M. Kharrasov
Publikováno v:
Astronomy Reports. 65:26-44
The paper presents the results of experiments for studying the dynamics and internal structure of an axial plasma jet at the PF-3 facility. Measurements of the azimuthal distribution of the toroidal magnetic field $${{B}_{\varphi }}(\varphi )$$ were
Autor:
Mikhail A. Vasil’ev, M.O. Ptitsyn, V. S. Beskin, Gennadii A Mesyats, Nikolai N. Kolachevsky, Lev P. Pitaevskii, Kirill P. Zybin, Vladimir I. Ritus, Ya N. Istomin, Andrei V. Gaponov-Grekhov, Lev Zelenyi
Publikováno v:
Physics-Uspekhi. 63:1148-1150
Autor:
Leonid I. Gurvits, Masanori Nakamura, Keiichi Asada, V. S. Beskin, Kazuhiro Hada, E. E. Nokhrina
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 489(1)
We propose a new method of estimating a mass of a super massive black hole residing in the center of an active galaxy. The active galaxy M87 offers a convenient test case for the method due to the existence of a large amount of observational data on
Autor:
Ewa Zielinska, K. N. Mitrofanov, V. S. Beskin, K. Tomaszewski, M. Paduch, V. I. Pariev, Ya. N. Istomin, V. I. Krauz, A. Szymaszek
Publikováno v:
Journal of Plasma Physics. 86
This paper presents the results of studies of plasma flow parameters on the PF-1000U facility. A distinctive feature of this facility is the ability to create profiled initial gas distributions using gas puffs. In the experiments described, a combine
The recently constructed theory of radio wave propagation in the pulsar magnetosphere outlines the general aspects of the radio light curve and polarization formation. It allows us to describe general properties of mean profiles, such as the position
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::afb92d3727735bc9abfb2ef9a1854562
http://arxiv.org/abs/2008.13750
http://arxiv.org/abs/2008.13750
Autor:
V. S. Beskin, I. Yu. Kalashnikov
The laboratory simulations of jets from young stars that have been carried out for many years at plasma focus facilities allow the internal structure of the active regions emerging during the interaction of the jet with the surrounding plasma to be s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c230a2b79b73b2d9749aa05299726ad0