Computational method for low-Mach-number compressible flows with moving particles and large temperature variations
Author:
Affiliation:
1. Academic Center for Computing and Media studies, Kyoto University
Publisher
Japan Society for Simulation Technology
Subject
General Engineering
Link
https://www.jstage.jst.go.jp/article/jasse/9/1/9_170/_pdf
Reference15 articles.
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2. [2] M. Rempel: Solar differential rotation and meridional flow: the role of a subadiabatic tachocline for the Taylor-Proudman balance, The Astrophysical Journal, 622 (2005), 1320-1332.
3. [3] H. Hotta, M. Rempel, T. Yokoyama, Y. Iida, Y. Fan: Numerical calculation of convection with reduced speed of sound technique, Astronomy & Astrophysics, 539 (2012), A30.
4. [4] H. Iijima, H. Hotta, S. Imada: Semiconservative reduced speed of sound technique for low Mach number flows with large density variations, Astronomy & Astrophysics, 622 (2019), A157.
5. [5] D. Toriu, S. Ushijima: Computation of non-isothermal and compressible low Mach number gas flows by fully explicit scheme using control method for speed of sound, Journal of Advanced Simulation in Science and Engineering, 6:1 (2019), 11-20.
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