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dc.contributor.author |
Drazkowska, J. |
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dc.contributor.author |
Hanasz, M. |
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dc.contributor.author |
Kowalik, K. |
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dc.date.accessioned |
2017-06-03T20:12:53Z |
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dc.date.available |
2017-06-03T20:12:53Z |
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dc.date.issued |
2011 |
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dc.identifier.citation |
Particle module of Piernik MHD code / J. Drazkowska, M. Hanasz, K. Kowalik // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 92-95. — Бібліогр.: 10 назв. — англ. |
uk_UA |
dc.identifier.isbn |
987-966-439-367-3 |
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dc.identifier.uri |
http://dspace.nbuv.gov.ua/handle/123456789/119090 |
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dc.description.abstract |
Piernik is a multi-fluid grid magnetohydrodynamic code based on the Relaxing Total Variation Diminishing conservative scheme. The original code has been extended by addition of the dust described within the particle approximation. The dust is now described as a system of interacting particles. The particles can interact with gas, which is described as a fluid. The comparison between the test problem results and the results coming from fluid simulations made with Piernik code shows the most important differences between fluid and particle approximations used to describe dynamical evolution of dust under astrophysical conditions. |
uk_UA |
dc.description.sponsorship |
This work was partially supported by Polish Ministry of Science and Higher Education through the grant 92/N-ASTROSIM/2008/0. The computations were performed on the HYDRA cluster at Torun Centre for Astronomy. |
uk_UA |
dc.language.iso |
en |
uk_UA |
dc.publisher |
Advances in astronomy and space physics |
uk_UA |
dc.relation.ispartof |
Advances in Astronomy and Space Physics |
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dc.title |
Particle module of Piernik MHD code |
uk_UA |
dc.type |
Article |
uk_UA |
dc.status |
published earlier |
uk_UA |
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