Zobrazeno 1 - 6
of 6
pro vyhledávání: '"S D Ustyugov"'
Publikováno v:
New Journal of Physics, Vol 19, Iss 6, p 065003 (2017)
We explore the structure and statistics of multiphase, magnetized ISM turbulence in the local Milky Way by means of driven periodic box numerical MHD simulations. Using the higher order-accurate piecewise-parabolic method on a local stencil (PPML), w
Externí odkaz:
https://doaj.org/article/15e8bd29b2324534a32ac84b840c7701
Autor:
D. O. Ustyugov, S. D. Ustyugov
Publikováno v:
Mathematical Models and Computer Simulations. 2:362-374
Radiation expansion of laser plasma in an external magnetic field is investigated in the paper. A two-dimensional system of ideal magneto-hydrodynamics with radiation transfer in a cylindrical system of coordinates was solved numerically using second
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3cff06d55772b7469665b3e6825ff2da
https://doi.org/10.1134/s2070048210030105
https://doi.org/10.1134/s2070048210030105
Autor:
D. O. Ustyugov, S. D. Ustyugov
Publikováno v:
Mathematical Models and Computer Simulations. 1:521-532
The evolution of laser-produced plasma in an external magnetic field was studied. Equations of ideal MHD in a cylindrical coordinate system were solved numerically by using the conservative TVD difference scheme of second order in time and space. At
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fa08f75d874f72fd6407137acc0a32d1
https://doi.org/10.1134/s2070048209040103
https://doi.org/10.1134/s2070048209040103
Autor:
S. D. Ustyugov, M. V. Popov
Publikováno v:
Computational Mathematics and Mathematical Physics. 48:477-499
A numerical scheme based on the piecewise parabolic method on a local stencil (PPML) is proposed for solving the ideal magnetohydrodynamic (MHD) equations. The method makes use of the conservation of Riemann invariants along the characteristics of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aae252762ac3e51af0a5a0689fc283e8
https://doi.org/10.1134/s0965542508030111
https://doi.org/10.1134/s0965542508030111
Publikováno v:
Journal of Experimental and Theoretical Physics. 86:629-635
This paper discusses the gravitational radiation that accompanies the formation of a rotating protoneutron star. Mainly large-scale entropy inhomogeneities develope inside the star. As a result, bubbles of hot nuclear substance are formed, and convec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::66de4c8a2732867d2d7734459483c9e9
https://doi.org/10.1134/1.558518
https://doi.org/10.1134/1.558518
Autor:
P. Padoan, A. G. Kritsuk, T. Lunttila, M. Juvela, A. Nordlund, M. L. Norman, S. D. Ustyugov, Giuseppe Bertin, Franca De Luca, Giuseppe Lodato, Roberto Pozzoli, Massimiliano Romé
Publikováno v:
AIP Conference Proceedings.
Supersonic magneto‐hydrodynamic (MHD) turbulence in molecular clouds (MCs) plays an important role in the process of star formation. The effect of the turbulence on the cloud fragmentation process depends on the magnetic field strength. In this wor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::860e7bba3579c440c160df6fc29a0168
https://doi.org/10.1063/1.3460128
https://doi.org/10.1063/1.3460128