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Documentation for gridalt

1 molod 1.1 \section{Gridalt - Alternate Grid Package}
2    
3     \subsection {Introduction}
4     To take advantage of a `high end' turbulence parameterization
5     (and convection parameterization), the vertical resolution near the surface
6     must be increased substantially as compared to the vertical resolution needed
7     aloft. This cannot be accomplished if the high end physics is computed using
8     the $p^*$ coordinate currently in use in the MIT gcm.
9    
10     The gridalt package was developed to allow the high end atmospheric physics
11     (fizhi) physics to be run on a separate grid from the hydrodynamics. The package
12     could (with some user modification) be used in conjunction with other packages
13     or for other calculations within the GCM. For the case of the atmospheric
14     physics, a modified $p^*$ coordinate, which adds additional levels between
15     the lower levels of the existing $p^*$ grid (and perhaps between the levels near
16     the tropopause as well), is implemented. The vertical discretization is
17     different for each grid point, although it consist of the same number of
18     levels. This is illustrated as follows:
19     \begin{figure}[htbp]
20     \vspace*{-0.4in}
21     \begin{center}
22     \includegraphics[height=2.4in]{vertical.eps}
23     \end{center}
24     \end{figure}
25    
26     \vspace*{-0.5in}
27     In addition to computing the physical forcing terms of the momentum,
28     thermodynamic and humidity equations on the modified (higher resolution)
29     grid, the higher resolution structure of the atmosphere (the boundary
30     layer) is retained between calculations. This neccessitates a second
31     set of evolution equations for the atmospheric state variables on the
32     modified grid. If the equations for the evolution of the state
33     on $p^*$ can be expressed as:
34     \[
35     \left . {\partial U \over {\partial t}} \right |_{p^*}^{total} =
36     \left . {\partial U \over {\partial t}} \right |_{p^*}^{dynamics} +
37     \left . {\partial U \over {\partial t}} \right |_{p^*}^{physics}
38     \]
39     where the physics forcing terms on $p^*$ have been computed from a
40     mapping from the modified grid, then an additional set of equations
41     to govern the evolution of $U$ on the modified grid are written:
42     \[
43     \left . {\partial U \over {\partial t}} \right |_{p^{*m}}^{total} =
44     \left . {\partial U \over {\partial t}} \right |_{p^{*m}}^{dynamics} +
45     \left . {\partial U \over {\partial t}} \right |_{p^{*m}}^{physics} +
46     \gamma ({\left . U \right |_{p^*}} - {\left . U \right |_{p^{*m}}})
47     \]
48     where $p^{*m}$ refers to the modified higher resolution grid, and
49     the dynamics forcing terms have been mapped from the $p^*$ space.
50     The last term on the RHS is a relaxation term, meant to constrain
51     the state variables on the modified vertical grid to `track' the
52     state variables on the $p^*$ grid on some time scale, $\gamma$.
53    
54     \subsection {Key subroutines, parameters and files }
55    
56     \subsection {Dos and donts}
57    
58     In the context of a Held-Suarez type of model experiment (located
59     in the fizhi-hs.cs-32x32x10 verification experiment) with
60     topography, the forcing terms which represent the physics are computed on
61     the modified grid. The forcing terms are computed as functions of the
62     state variables on the modified grid. The tendencies are then interpolated
63     to the standard grid
64    
65     \subsection {Gridalt Reference}

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