Difference between revisions of "One way nesting"

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The need for grid nesting is greatly reduced with unstructured grid models.  
 
The need for grid nesting is greatly reduced with unstructured grid models.  
  
Occasionally, 1 way nesting may be useful; e.g., you don't usually have velocity b.c. at an open boundary. You can effectively use SELFE's 1-way nesting capability to get around this issue.  
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Occasionally, 1 way nesting may be useful; e.g., you don't usually have velocity b.c. at an open boundary. You can effectively use SCHISM's 1-way nesting capability to get around this issue.  
  
You can first run the efficient SELFE 2D in a larger or same grid, and then use the 1-way nesting scripts in the source code bundle (v3.2 and up) to extract results from this run and prepare uv3D.th (if you first run a coarse-grid SELFE 3D baroclinic simulation, you can also prepare salt3D.th and temp3D.th). Then simple use *3D.th to drive the small-domain 3D runs. Note that this approach only works if the b.c. does not significantly affect the internal dynamics.
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You can first run the efficient SCHISM 2D in a larger or same grid, and then use the 1-way nesting scripts in the source code bundle (v4.1 and up) to extract results from this run and prepare elev2D.th, uv3D.th (if you first run a coarse-grid SCHISM 3D baroclinic simulation, you can also prepare salt3D.th and temp3D.th). See: .../src/Utility/OneWayNestScripts/README. Then simply use *[23]D.th to drive the small-domain 3D runs. Note that this approach only works if the b.c. does not significantly affect the internal dynamics.

Latest revision as of 07:58, 30 March 2015

The need for grid nesting is greatly reduced with unstructured grid models.

Occasionally, 1 way nesting may be useful; e.g., you don't usually have velocity b.c. at an open boundary. You can effectively use SCHISM's 1-way nesting capability to get around this issue.

You can first run the efficient SCHISM 2D in a larger or same grid, and then use the 1-way nesting scripts in the source code bundle (v4.1 and up) to extract results from this run and prepare elev2D.th, uv3D.th (if you first run a coarse-grid SCHISM 3D baroclinic simulation, you can also prepare salt3D.th and temp3D.th). See: .../src/Utility/OneWayNestScripts/README. Then simply use *[23]D.th to drive the small-domain 3D runs. Note that this approach only works if the b.c. does not significantly affect the internal dynamics.