Zobrazeno 1 - 10
of 17
pro vyhledávání: '"R. Zemskov"'
Autor:
Alexis Kudryashov, R. Zemskov, A. A. Soloviev, Vadim Samarkin, Ilya Galaktionov, M. V. Starodubtsev, S. E. Perevalov, A. V. Kotov, A. Alexandrov
Publikováno v:
Quantum Electronics. 51:593-596
We present the results of the aberration correction of laser radiation wavefront using a dynamic method for determining the reference wavefront. The method, which is based on the processing of synchronously obtained data on the near- and far-field zo
Autor:
R. Zemskov, A. A. Shaikin, A. A. Kochetkov, A. A. Soloviev, A. G. Luchinin, M. Yu. Glyavin, M. V. Starodubtsev, Ivan V. Yakovlev, S. E. Perevalov, K. F. Burdonov, A. V. Kotov, A. A. Kuzmin, Vladislav Ginzburg, Mikhail V. Morozkin, Efim A. Khazanov, Julien Fuchs, M. D. Proyavin, I. A. Shaikin
Publikováno v:
Izvestiya vysshikh uchebnykh zavedenii. Radiofizika. 63:973-984
We present the results of studying experimentally the expansion of laser plasma in a strong external magnetic field (with a magnetic flux density of 13.5 T) at various sizes of the region of plasma formation on the surface of a solid-state target. It
Autor:
Alexander Soloviev, Andrea Ciardi, R. Bonito, A. Korzhimanov, K. F. Burdonov, M. Romanova, M. V. Starodubtsev, W. P. Yao, A. Sladkov, Julien Fuchs, S. N. Chen, R. Zemskov, Salvatore Orlando
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 657, pp.A112. ⟨10.1051/0004-6361/202140997⟩
Astronomy and Astrophysics-A&A, 2022, 657, pp.A112. ⟨10.1051/0004-6361/202140997⟩
This work was granted access to the HPC resources of MesoPSL financed by the Region Ile de France and the project EquipMeso (reference ANR-10-EQPX29-01) of the programme Investissements d’Avenir supervised by the Agence Nationale pour la Recherche.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa2edcc83491364cdedcb09dc9b5cbb6
https://hal-cea.archives-ouvertes.fr/cea-03538274
https://hal-cea.archives-ouvertes.fr/cea-03538274
Autor:
Mikhail Gushchin, Rosaria Bonito, K. Gubskiy, Efim A. Khazanov, Julien Fuchs, A. V. Strikovskiy, V. I. Gundorin, A. Kuznetsov, S. N. Ryazantsev, S. A. Pikuz, Salvatore Orlando, Alexander Soloviev, W. P. Yao, I. Shaykin, Teresa Giannini, R. Zemskov, Ivan V. Yakovlev, Shihua Chen, N. A. Aidakina, I. Zudin, Andrey Shaykin, M. V. Starodubtsev, Vladislav Ginzburg, K. Burdonov, A. A. Kuzmin, J. Béard, G. Revet, A. A. Kochetkov, Andrea Ciardi, S. V. Korobkov, Costanza Argiroffi
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 648, pp.A81. ⟨10.1051/0004-6361/202040036⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 648, pp.A81. ⟨10.1051/0004-6361/202040036⟩
Astronomy and Astrophysics-A&A, 2021, 648, pp.A81. ⟨10.1051/0004-6361/202040036⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 648, pp.A81. ⟨10.1051/0004-6361/202040036⟩
Aims. EXor-type objects are protostars that display powerful UV-optical outbursts caused by intermittent and powerful events of magnetospheric accretion. These objects are not yet well investigated and are quite difficult to characterize. Several par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4dddea2c8020464a94ec5b5f509805a5
https://hal.science/hal-03164400
https://hal.science/hal-03164400
Akademický článek
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Autor:
V. R. Zemskov
Publikováno v:
Plasma Physics Reports. 29:675-682
A study is made of the propagation of a long-wavelength fast magnetosonic wave in a space plasma with a low particle density and high temperature (βe≈βi≈1) in a direction perpendicular to the magnetic field, along which the structures originati
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Akademický článek
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Autor:
V. R. Zemskov
Publikováno v:
Plasma Physics Reports. 28:183-189
The question of the existence of a steady-state shock front of a fast magnetosonic wave propagating across the magnetic field against the background of turbulent Alfven waves is considered. It is shown that the steady-state shock front can form as a
Autor:
V. R. Zemskov
Publikováno v:
Russian Physics Journal. 40:821-827
The interaction of fast magnetoacoustic (FMA) waves in a plasma with particle concentration nt∼ni∼1 cm−3 is studied with allowance for Alfven modes, which simulates turbulence. Equations that describe three-wave interaction of FMAs are derived