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3.14.1 Overview

This example demonstrates using the MITgcm to simulate the planetary atmospheric circulation, with flat orography and simplified forcing. In particular, only dry air processes are considered and radiation effects are represented by a simple newtownien cooling, Thus this example does not rely on any particular atmospheric physics package. This kind of simplified atmospheric simulation has been widely used in GFD-type experiments and in intercomparison projects of AGCM dynamical cores [Held and Suarez, 1994].

The horizontal grid is obtain from the projection of a uniform gridded cube to the sphere. Each of the 6 faces has the same resolution, with $ 32 \times 32$ grid points. The equator line coincide with a grid line and crosses, right in the midle, 4 of the 6 faces, leaving 2 faces for the Northern and Southern polar regions. This curvilinear grid requires the use of the 2nd generation exchange topology (pkg/exch2) to connect tile and face edges, but without any limitation on the number of processors.

The use of the $ p^*$ coordinate with 20 equally spaced levels ( $ 20 \times 50\,{\rm mb}$ , from $ p^*=1000,{\rm mb}$ to 0 at the top of the atmosphere) follows the choice of Held and Suarez [1994]. Note that without topography, the $ p^*$ coordinate and the normalized pressure coordinate ($ \sigma_p$ ) coincide exactly. No viscosity and zero diffusion are used here, but a $ 8^th$ order Shapiro [1970] filter is applied to both momentum and potential temperature, to remove selectively grid scale noise. Apart from the horizontal grid, this experiment is made very similar to the grid-point model case used in Held and Suarez [1994] study.

At this resolution, the configuration can be integrated forward for many years on a single processor desktop computer.


next up previous contents
Next: 3.14.2 Forcing Up: 3.14 Held-Suarez Atmosphere MITgcm Previous: 3.14 Held-Suarez Atmosphere MITgcm   Contents
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