Gallery / Simulation with regional domain using SCALE-DG (This page is under construction)
Planetary boundary layer turbulence
This page shows a result of large eddy simulation of idealized planetary boundary layer turbulence using the discontinuous Galerkin method (DGM). An example of the setting files is given in rootdir/model/atmosphere3d/test/case/pbl_turbulence/.
1. Description of dynamical core
Please see XX.
2. Experimental setup
The experiment setup is based on Nishizawa et al. (2015). To drive thermal convection, a constant heat flux with 200 W/m2 is injected at the surface. To parametrize the sub-grid scale effect of turbulence, a Smagorinsky-Lilly type turbulent model (Smagorinsky, 1963; Lilly, 1962; Brown et al., 1994) is used.
In next section, we show results in the case of using the following model parameters
- Spatial resolution: NeX=48, NeY=48, NeZ=10, p=7 (LGL nodes)
- Element-wise 16th-order exponential filter is applied for all modes and the factor of filter strength, $\alpha$, is 0.05; for example, the highest mode is dumped by $\exp{(-\alpha)}$.
- $\Delta t=0.003$ [sec] (with a full explicit ten-stage and fourth-order RK scheme)
3. Result
4. Reference
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Brown, A. R., S. H. Derbyshire, and P. J. Mason, 1994: Large-eddy simulation of stable atmo- spheric boundary layers with a revised stochastic subgrid model. Quarterly Journal of the Royal Meteorological Society, 120 (520), 1485–1512.
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Hesthaven, J. S., and T. Warburton, 2007: Nodal discontinuous Galerkin methods: algorithms, analysis, and applications, Springer Science & Business Media
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Nishizawa, S., H. Yashiro, Y. Sato, Y. Miyamoto, and H. Tomita, 2015: Influence of grid aspect ratio on planetary boundary layer turbulence in large-eddy simulations. Geoscientific Model Development, 8 (10), 3393–3419.
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Smagorinsky, J., 1963: GENERAL CIRCULATION EXPERIMENTS WITH THE PRIMITIVE EQUATIONS: I. THE BASIC EXPERIMENT. Monthly Weather Review, 91 (3), 99–164.
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Lilly, D. K., 1962: On the numerical simulation of buoyant convection. Tellus, 14 (2), 148–172.