[MITgcm-devel] Re: odds and ends
Jean-Michel Campin
jmc at ocean.mit.edu
Fri Nov 18 08:05:35 EST 2005
Hi Daniel,
Others might be interested, so I cc to mitgcm-devel list.
On Thu, Nov 17, 2005 at 04:46:42PM -0500, Daniel Enderton wrote:
> Hey Jean -Michel!
>
> Hope your having a good time in Belgium.
>
> If you have time for a couple questions...
>
> (1) I am trying to get all your key cube sphere functions a bit
> cleaned up and user friendly to put in the cs_grid directory. I have
> banged out the heat transport script and the overturning script. I
> was working on the horizontal stream function script (calc_psiH_CS.m)
> and had a couple questions. Why is the output of the function of
> length 6146 = 192*32+2 rather than 6144 = 192*32. What are the two
> extra points for? Are there any particular two points that I can
> strip off and plot using merccube?
Psi is located at grid-cell corner (= vorticity point) and the CS grid
has 2 more corner points than cell-center points. To make a plot,
I usually interpolate to lat-lon (just need the list of longitude
& latitude corresponding to the Psi values) and then draw contour lines.
> (2) Is there anyway that I can generate u*phi and v*phi to get the
> heat transport in the atmosphere associates with potential energy?
I think Andrea checked-in 2 new diagnostics (UVELPHI & VVELPHI)
two days ago.
> Further, since we are using zstar in the atmosphere we need hu and hv
> to generate the overturning stream function. Would this not mean we
> should use hu*t and hv*t for the sensible heat transport. I looked,
> but saw not huttave (or similar) field in the output or in the
> diagnostics package.
With timeave pkg, the hfac is already accounted for in the
output files UTtave & VTtave. With the diagnostics pkg, both
diagnostics are available (with hfac: UTHMASS,VTHMASS
and without: UVELTH,VVELTH)
Cheers,
Jean-Michel
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