Abstract
Although the spectral method can be used on the spherical surface of general circulation models, it is difficult to extend to the vertical direction since various boundary conditions are applied at the top and bottom of the atmosphere. Thus, the grid method is normally used for vertical discretization of general circulation models. We have seen that the spectral method of shallow-water equations on a sphere naturally assures conservation of various physical quantities. It will be shown that conservation in the primitive equation model is achieved by proper vertical discretization. Here we use the flux-form finite volume method for vertical discretization. We require the domain integral conservation of energy and that of potential temperature. We will also find a discretization that minimizes an error in pressure gradient force when the atmosphere is everywhere isentropic.
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References and suggested reading
Arakawa, A. and Suarez, M. J., 1983: Vertical differencing of the primitive equations in sigma coordinates. Mon.Wea.Rev., 111, 34–45.
Arakawa, A. and Moorthi, S., 1988: Baroclinic instability in vertically discrete system. J.Atmos. Sci., 45, 1688–1707.
Arakawa, A. and Konor, C., 1996: Vertical differencing of the primitive equations based on the Charney-Phillips grid in hybrid sigma-p vertical coordinates. Mon.Wea.Rev., 124, 511–528.
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© 2014 Springer-Verlag Berlin Heidelberg
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Satoh, M. (2014). Vertical discretization of hydrostatic models. In: Atmospheric Circulation Dynamics and General Circulation Models. Springer Praxis Books(). Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-13574-3_22
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DOI: https://doi.org/10.1007/978-3-642-13574-3_22
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