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Table of Contents - The Atmospheric Studies Group at TRC

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Section 7: Prognostic Meteorological Interfaces<br />

<strong>The</strong> vertical coordin<strong>at</strong>e is the terrain-following height Z* system, with Z* is defined as<br />

Zagl<br />

Z* <br />

7-4<br />

Zterr<br />

1<br />

Ztop<br />

where Z agl is the height above the ground, the Z terr is the topographical height <strong>at</strong> grid, and Z top is the height<br />

<strong>of</strong> model top. In this coordin<strong>at</strong>e system, each level is a given fraction <strong>of</strong> the distance between the surface<br />

and the model top. <strong>The</strong> variables are staggered in vertical. <strong>The</strong> horizontal momentum <strong>of</strong> U and V<br />

components and all thermodynamic variables are defined <strong>at</strong> the full Z* levels, while the vertical velocity<br />

(W) is defined <strong>at</strong> half-Z* levels. <strong>The</strong> model top height is usually about 15-20 km above the ground.<br />

<strong>The</strong> 3D.DAT file for CALMET needs a uniform coordin<strong>at</strong>e system in both horizontal and vertical<br />

directions. Since most variables are <strong>at</strong> thermodynamic points, a two-grid averaging is used to interpol<strong>at</strong>e<br />

momentum variables <strong>of</strong> U, V, and W in the staggered Arakawa-C coordin<strong>at</strong>e system to its thermodynamic<br />

point. <strong>The</strong> set <strong>of</strong> thermodynamic point coordin<strong>at</strong>es is used in the 3D.DAT file.<br />

<strong>The</strong> CALRAMS processor runs on a UNIX pl<strong>at</strong>form and includes a host program called CALRAMS.F90<br />

and a set <strong>of</strong> subroutines th<strong>at</strong> perform various functions.<br />

CALRAMS Input Files<br />

RAMS Output file<br />

CALRAMS was designed for a particular applic<strong>at</strong>ion <strong>of</strong> RAMS, with specific file names. Each RAMS<br />

file consists <strong>of</strong> one hour <strong>of</strong> model output for one nest. <strong>The</strong> naming convention is:<br />

iw-A-YYYY-MM-DD-HH0000-g1.vfm<br />

iw-A-YYYY-MM-DD-HH0000-g2.vfm<br />

iw-A-YYYY-MM-DD-HH0000-g3.vfm<br />

iw-A-YYYY-MM-DD-HH0000-g4.vfm<br />

iw-A-YYYY-MM-DD-HH0000-head.txt<br />

where YYYY is the 4-digit year, MM is the 2-digit month, DD is the 2-digit day, and HH is the 2-digit<br />

hour. <strong>The</strong> file with “head.txt” is the header file providing the RAMS configur<strong>at</strong>ion and output variables.<br />

<strong>The</strong> part “-g1 –g2 –g3 –g4” represents the nesting levels for the output. Because many hours are typically<br />

processed in one simul<strong>at</strong>ion, cre<strong>at</strong>ing a 3D.DAT file requires many RAMS files. <strong>The</strong>se file names are<br />

constructed by CALRAMS for the processing period, so all RAMS files for the period must reside in a<br />

single directory. Applic<strong>at</strong>ions th<strong>at</strong> use different file names will require changes to the CALRAMS code.<br />

7-52

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