Ustyugov Sergey Dmitrievich

Publications in Math-Net.Ru

1. A quasi-gas dynamic algorithm for the numerical solution of shallow water equations for magnetic hydrodynamics
   
   Keldysh Institute preprints, 2012, 064, 24 pp.
2. Quasi-gas dynamic algorithm of solution of magnetohydrodynamic equations. Multidimensional case
   
   Keldysh Institute preprints, 2011, 030, 24 pp.
3. Quasi-gas dynamic algorithm of solution of magnetohydrodynamic equations. One dimensional case.
   
   Keldysh Institute preprints, 2011, 001, 20 pp.
4. Laser plasma simulation in external magnetic field of the various configuration
   
   Matem. Mod., 23:3 (2011),  49–59
5. Simulation of radiation expansion of laser plasma in external magnetic field
   
   Matem. Mod., 21:11 (2009),  33–46
6. The laser plasma in external magnetic field
   
   Matem. Mod., 20:8 (2008),  74–86
7. Piecewise parabolic method on a local stencil for ideal magnetohydrodynamics
   
   Zh. Vychisl. Mat. Mat. Fiz., 48:3 (2008),  505–528
8. Piecewise parabolic method on local stencil. V. 3D Isothermal turbulence
   
   Keldysh Institute preprints, 2007, 081, 24 pp.
9. Piecewise parabolic method on local stencil. IV. Multidimensional ideal MHD
   
   Keldysh Institute preprints, 2007, 011, 30 pp.
10. Piecewise parabolic method on local stencil for gasdynamic simulations
    
    Zh. Vychisl. Mat. Mat. Fiz., 47:12 (2007),  2055–2075
11. Piecewise parabolic method on local stencil. III. 1D ideal MGD
    
    Keldysh Institute preprints, 2006, 078, 27 pp.
12. Piecewise parabolic method on local stencil. II. Gasdynamics equations
    
    Keldysh Institute preprints, 2006, 071, 22 pp.
13. Piecewise parabolic method on local stencil. I. Advection equation and Burgers' equation
    
    Keldysh Institute preprints, 2006, 065, 21 pp.
14. Mathematical modeling of a supernova explosion on a parallel computer
    
    Zh. Vychisl. Mat. Mat. Fiz., 44:5 (2004),  953–960
15. The Simulation of the Evolution of the Neutrino Distribution in a Region with Varying Parameters. (Homogeneous, isotropic approximation.)
    
    Keldysh Institute preprints, 1999, 070
16. The Modelling of the Evolution of the Neutrino Distribution in the Expanding Area . (Homogeneous, isotropic approximation.)
    
    Keldysh Institute preprints, 1998, 070