Time Integration of the Shallow Water Equations in Spherical Geometry
The shallow water equations in spherical geometry provide a prototype for developing and testing numerical algorithms for atmospheric circulation models. In a previous paper we have studied a spatial discretization of these equations based on an Osher-type finite-volume method on stereographic and l...
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Published in | Journal of computational physics Vol. 171; no. 1; pp. 373 - 393 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Elsevier Inc
20.07.2001
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Subjects | |
Online Access | Get full text |
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Summary: | The shallow water equations in spherical geometry provide a prototype for developing and testing numerical algorithms for atmospheric circulation models. In a previous paper we have studied a spatial discretization of these equations based on an Osher-type finite-volume method on stereographic and latitude–longitude grids. The current paper is a companion devoted to time integration. Our main aim is to discuss and demonstrate a third-order, A-stable, Runge–Kutta–Rosenbrock method. To reduce the costs related to the linear algebra operations, this linearly implicit method is combined with approximate matrix factorization. Its efficiency is demonstrated by comparison with a classical, third-order explicit, Runge–Kutta method. For that purpose we use a known test set from literature. The comparison shows that the Rosenbrock method is by far superior. |
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Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
ISSN: | 0021-9991 1090-2716 |
DOI: | 10.1006/jcph.2001.6802 |