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Model equations

In a generic pressure-based terrain following vertical coordinate ¦Ç, the governing equations of the atmosphere under the hydrostatic assumption can be derived following Kasahara (1974). This equation set, also known as the primitive equations, reads

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(1)
(2)
(3)
(4)

Here v is the  horizontal velocity vector (on the sphere)k is the  unit vector in the radial outward directionf  is the Coriolis parameter; is the vertical component of the relative vorticity; is the kinetic energy per unit mass.  p and T denote pressure and temperature, respectively. is geopotential, R is the gas constant and Cp  the specific heat capacity of dry air under constant pressure. Note that the momentum equation is written in the vector invariant form.

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The hybrid vertical coordinate

The generalized p-sigma hybrid vertical coordinate used in ICOHDC is the same as in ECHAM5 and many other global hydrostatic models. It was first introduced by Simmons and Str¨¹fing (1981) for the grid-point forecast model of the ECMWF. The vertical domain of the model atmosphere is divided into NLEV layers. Pressure values of the interfaces between layers are given by

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(5)

and are parameters independent of the horizontal location.  Near the earth¡¯s surface equals zero and the interfaces are pure sigma levels; near the model top equals zero and the interfaces coincide with isobaric surfaces. The levels in between provide a smooth transition. Pressure of the "full levels" on which the horizontal wind and temperature are predicted is defined as

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(6)

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Last modified: 2008-10-20 by Hui Wan