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dc.contributor.author Drazkowska, J.
dc.contributor.author Hanasz, M.
dc.contributor.author Kowalik, K.
dc.date.accessioned 2017-06-03T20:12:53Z
dc.date.available 2017-06-03T20:12:53Z
dc.date.issued 2011
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
dc.identifier.uri http://dspace.nbuv.gov.ua/handle/123456789/119090
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
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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