Abstract
Professor Roe’s beautiful expository article in this volume can be easily read and used by a novice to the field of shock capturing. Our purpose here is to demonstrate that we can go beyond the second order accurate TVD barrier [7] and still suppress spurious numerical oscillations near discontinuities and other steep gradients.
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References
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H. Yang, Ph.D. Thesis, UCLA Math. Dept., 1988.
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© 1990 Kluwer Academic Publishers
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Osher, S., Shu, CW. (1990). High Order Accurate Modern Numerical Methods Applicable to Stellar Pulsations. In: Buchler, J.R. (eds) The Numerical Modelling of Nonlinear Stellar Pulsations. NATO ASI Series, vol 302. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0519-1_15
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DOI: https://doi.org/10.1007/978-94-009-0519-1_15
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