Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Babkovskaia, N."'
Autor:
Brandenburg, A., Johansen, A., Bourdin, P. A., Dobler, W., Lyra, W., Rheinhardt, M., Bingert, S., Haugen, N. E. L., Mee, A., Gent, F., Babkovskaia, N., Yang, C. -C., Heinemann, T., Dintrans, B., Mitra, D., Candelaresi, S., Warnecke, J., Käpylä, P. J., Schreiber, A., Chatterjee, P., Käpylä, M. J., Li, X. -Y., Krüger, J., Aarnes, J. R., Sarson, G. R., Oishi, J. S., Schober, J., Plasson, R., Sandin, C., Karchniwy, E., Rodrigues, L. F. S., Hubbard, A., Guerrero, G., Snodin, A., Losada, I. R., Pekkilä, J., Qian, C.
Publikováno v:
Journal of Open Source Software 6, 2807 (2021)
The Pencil Code is a highly modular physics-oriented simulation code that can be adapted to a wide range of applications. It is primarily designed to solve partial differential equations (PDEs) of compressible hydrodynamics and has lots of add-ons ra
Externí odkaz:
http://arxiv.org/abs/2009.08231
Publikováno v:
Phys. Rev. E 83, 016304 (2011)
Direct numerical simulations and mean-field theory are used to model reactive front propagation in a turbulent medium. In the mean-field approach, memory effects of turbulent diffusion are taken into account to estimate the front speed in cases when
Externí odkaz:
http://arxiv.org/abs/1008.5145
Publikováno v:
J. Comp. Phys., 230, 1-12 (2011)
A high-order scheme for direct numerical simulations of turbulent combustion is discussed. Its implementation in the massively parallel and publicly available Pencil Code is validated with the focus on hydrogen combustion. Ignition delay times (0D) a
Externí odkaz:
http://arxiv.org/abs/1005.5301
In an attempt to model the accretion onto a neutron star in low-mass X-ray binaries, we present two-dimensional hydrodynamical models of the gas flow in close vicinity of the stellar surface. First we consider a gas pressure dominated case, assuming
Externí odkaz:
http://arxiv.org/abs/0802.1663
Autor:
Szczerba, R., Szymczak, M., Babkovskaia, N., Poutanen, J., Richards, A. M. S., Groenewegen, M. A. T.
Various scenarios have been proposed to explain the presence of silicate features associated with carbon stars, such as V778 Cyg. We have attempted to constrain these theories by means of mapping water maser mission from V778 Cyg. The 22 GHz water ma
Externí odkaz:
http://arxiv.org/abs/astro-ph/0504354
Publikováno v:
In Journal of Computational Physics 2011 230(1):1-12
Akademický článek
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Autor:
Szczerba, R., Szymczak, M., Babkovskaia, N., Poutanen, J., Richards, A. M. S., Groenewegen, M. A. T., Szczerba, R., Szymczak, M., Babkovskaia, N., Poutanen, J., Richards, A. M. S., Groenewegen, M. A. T.
Publikováno v:
Astronomy and Astrophysics; June 2006, Vol. 452 Issue: 2 p561-565, 5p
Publikováno v:
Astronomy and Astrophysics; March 2006, Vol. 447 Issue: 3 p949-962, 14p
Publikováno v:
Astronomy and Astrophysics; April 2004, Vol. 418 Issue: 1 p117-129, 13p