[MITgcm-support] 2D boundary conditions at the poles
Jean-Michel Campin
jmc at ocean.mit.edu
Sat Nov 12 11:14:52 EST 2011
Hi Angela,
Could you send the complete parameter file "data" ? might be useful
to figure out what is the problem. Also, a plot of Eta function
of latitude would be nice.
Cheers,
Jean-Michel
On Thu, Nov 10, 2011 at 06:34:34PM -0500, Angela Marie Zalucha wrote:
> Hi,
>
> I am running the MIT GCM in 2D for the atmosphere (latitue and r*
> coordinates). When I look at eta vs. latitue, I get a very huge
> spike in the second to last gridpoint from the poles. I believe it
> is numerical and not physical. I was wondering what the boundary
> conditions are at the poles and how to explain it.
>
> Here's what I have for the horizontal grid:
> usingSphericalPolarGrid=.TRUE.,
> delX=1*2.8125,
> delY=64*2.8125,
> ygOrigin=-90.,
>
> The pressure is extremely low because this is Pluto!
> Ro_SeaLevel=1.6,
> rSphere=1180.E3,
>
> I have seen that the Shapiro filter can affect numerical spikes in
> eta in other 2D planets, but haven't been able to modify it
> successfully here. Here's my data.shap :
> &SHAP_PARM01
> shap_filt_uvStar=.FALSE.,
> shap_filt_TrStagg=.TRUE.,
> Shap_funct=4,
> nShapT=4,
> nShapUV=4,
>
> Does anybody have any ideas?
>
> Angela
>
>
>
> _-_-_-_-_-_-_-_-_-_-_-_-_-_-_-_-_-_-_-_-_-_-_-
> Angela Zalucha, Ph.D.
> Postdoctoral Associate
> Department of Earth, Atmospheric,
> and Planetary Sciences
> Massachusetts Institute of Technology
>
> Office located at Southwest Research Institute
> 1050 Walnut Street, Suite 300
> Boulder, CO 80302
> USA
> (720) 208-7211
>
>
> http://web.mit.edu/azalucha/www/index.html
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>
>
>
>
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