Zobrazeno 1 - 10
of 66
pro vyhledávání: '"A. V. Koldoba"'
Autor:
Ahmed K. Abu-Nab, Alexander V. Koldoba, Elena V. Koldoba, Yury A. Poveshchenko, Viktoriia O. Podryga, Parvin I. Rahimly, Ahmed E. Bakeer
Publikováno v:
Mathematics, Vol 11, Iss 2, p 341 (2023)
The purpose of this paper is to present a one-dimensional model that simulates the thermo-physical processes for methane hydrate decomposition in porous media. The mathematical model consists of equations for the conservation of energy, gas, and liqu
Externí odkaz:
https://doaj.org/article/253781ca03a24b7fad4502b9a13b3339
Autor:
A. V. Koldoba, Galina V. Ustyugova
Publikováno v:
Mathematical Models and Computer Simulations. 13:674-683
The paper proposes a computational algorithm for the numerical simulation of two-dimensional magnetohydrodynamic (MHD) flows, using a symmetry analyzer as an element of the numerical method. The algorithm is based on a finite-volume Godunov-type sche
Autor:
G. V. Ustyugova, A. V. Koldoba
Publikováno v:
Mathematical Models and Computer Simulations. 12:125-132
The paper proposes a symmetry analyzer as an element of the computational algorithm for the numerical integration of two-dimensional equations of ideal gas dynamics. A symmetry analyzer is an algorithm that allows using grid data to give a preference
Autor:
A. V. Koldoba, Galina V. Ustyugova, A. A. Blinova, P. S. Lii, Lisa Kaltenegger, Richard V. E. Lovelace, Marina M. Romanova
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 485:2666-2680
Inward migration of low-mass planets and embryos of giant planets can be stopped at the disc-cavity boundaries due to co-orbital corotation torque. We performed the first global three-dimensional (3D) simulations of planet migration at the disc-cavit
Publikováno v:
Mathematical Models and Computer Simulations. 11:86-96
We consider numerical aspects of the mathematical modeling of composite flows (relativistic and nonrelativistic) on adaptive computational grids applied to a double pulsar–optical star system. The pulsar is the source of an ultrarelativistic wind o
Autor:
Galina V. Ustyugova, A. V. Koldoba
Publikováno v:
Smart Modelling for Engineering Systems ISBN: 9789813346185
The chapter describes an approach using Godunov-type difference schemes to construct numerical algorithms for numerically integrating equations of ideal gas dynamics and magnetohydrodynamics. This approach allows calculating the flows of conservative
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::463033ce761e6d1fcc5692aeb552503e
https://doi.org/10.1007/978-981-33-4619-2_10
https://doi.org/10.1007/978-981-33-4619-2_10
Autor:
Galina V. Ustyugova, Dong Lai, Richard V. E. Lovelace, Marina M. Romanova, A. A. Blinova, A. V. Koldoba
We present results of global three-dimensional (3D) magnetohydrodynamic (MHD) simulations of accretion onto magnetized stars where both the magnetic and rotational axes of the star are tilted about the rotational axis of the disc. We observed that in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::76ab0fc56809e293fad254bce7fe16e2
http://arxiv.org/abs/2012.10826
http://arxiv.org/abs/2012.10826
Autor:
Marina M. Romanova, A. A. Blinova, Galina V. Ustyugova, A. V. Koldoba, Richard V. E. Lovelace
Publikováno v:
New Astronomy. 62:94-114
We investigate the properties of magnetized stars in the propeller regime using axisymmetric numerical simulations. We modelled the propeller regime for stars with realistically large magnetospheres (5-7 stellar radii), so that our results could be a
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 477:127-138
We numerically investigate the generation of a magnetic field in a protostellar disc via an $\alpha \Omega$-dynamo and the resulting magnetohydrodynamic (MHD) driven outflows. We find that for small values of the dimensionless dynamo parameter $\alph
Publikováno v:
Mathematical Models and Computer Simulations. 10:111-119
An algorithm is presented, which enables us to use the iterative Richardson method for solving a system of linear algebraic equations with the matrix corresponding to a sign-definite selfadjoint operator, in the absence of information about the lower