Spatial discretization schemes commonly used in global meteorological applications are currently limited to spectral methods or low-order finite-difference/finiteelement methods. The spectral transform method, which yields high-order approximations, requires Legendre transforms, which have a computa
The Spectral Element Method for the Shallow Water Equations on the Sphere
โ Scribed by Mark Taylor; Joseph Tribbia; Mohamed Iskandarani
- Publisher
- Elsevier Science
- Year
- 1997
- Tongue
- English
- Weight
- 575 KB
- Volume
- 130
- Category
- Article
- ISSN
- 0021-9991
No coin nor oath required. For personal study only.
โฆ Synopsis
any potential climate model should perform well on these tests. In this paper we will present the results from these
The spectral element method is implemented for the shallow water equations in spherical geometry and its performance is com-test cases after first comparing and contrasting the spectral pared with other models. This is the first step in evaluating the element method with global spectral methods and desuitability of spectral elements for climate modeling. The potential scribing the details of the model specific to spherical geadvantages and disadvantages of spectral elements over more conometry.
ventional models used for climate studies are discussed. The method requires that the sphere be tiled with rectangles, for which we make use of the gnomonic projection to map the sphere onto the cube. To measure the performance of the method relative to
2. SPHERICAL HARMONICS AND
other models, results are presented from a standard suite of shallow
SPECTRAL ELEMENTS
water test cases for the sphere. These results confirm the spectral accuracy of the method. แฎ 1997 Academic Press Global atmospheric modeling is in one sense easier than ocean modeling. The geometrically complex ocean basins are replaced by the surface of a sphere. The sphere has
๐ SIMILAR VOLUMES
## Communicated by J. C. Nedelec A new solution of the two-dimensional shallow-water equations, using a finite element method is described. The formulation is based on the velocity and height variables and follows two step. In the first step, the convective terms are solved by a characteristic met
We describe the implementation of numerical models of shallow water flow on the surface of the sphere, models which include the nondivergent barotropic limit as a special case. All of these models are specified in terms of a new grid-point-based methodology which employs an heirarchy of tesselations