Abstract:
The article contains results of modeling a meteor entering dense atmosphere layers using Galerkin’s method and smoother particle hydrodynamics. Numerical simulations were run using experimental data gathered for the Chelyabinsk meteor while varying the meteor material characteristics and its orientation when entering the atmosphere.
Citation:
I. B. Petrov, V. A. Miryaha, A. V. Sannikov, A. V. Shevtsov, “Computational modeling of a meteor entering atmosphere dense layersusing elastoplastic approximation”, Computer Research and Modeling, 5:6 (2013), 957–967
\Bibitem{PetMirSan13}
\by I.~B.~Petrov, V.~A.~Miryaha, A.~V.~Sannikov, A.~V.~Shevtsov
\paper Computational modeling of a meteor entering atmosphere dense layersusing elastoplastic approximation
\jour Computer Research and Modeling
\yr 2013
\vol 5
\issue 6
\pages 957--967
\mathnet{http://mi.mathnet.ru/crm448}
\crossref{https://doi.org/10.20537/2076-7633-2013-5-6-957-967}
Linking options:
https://www.mathnet.ru/eng/crm448
https://www.mathnet.ru/eng/crm/v5/i6/p957
This publication is cited in the following 2 articles:
A. V. Astanin, A. D. Dashkevich, I. B. Petrov, M. N. Petrov, S. V. Utyuzhnikov, N. I. Khokhlov, “Modeling the influence of the Chelyabinsk meteorite's bow shock wave on the Earth surface”, Math. Models Comput. Simul., 9:2 (2017), 133–141
A. S. Kholodov, “Ob evolyutsii vozmuschenii, vyzvannykh dvizheniem meteoroidov v atmosfere Zemli”, Kompyuternye issledovaniya i modelirovanie, 5:6 (2013), 993–1030
Citation in format AMSBIB
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