intermediate formats (metgrid/src/read_met_module.F90 andmetgrid/src/write_met_module.F90, respectively).When writing data to the WPS intermediate format, 2-dimensional fields are written as arectangular array of real values. 3-dimensional arrays must be split across the verticaldimension into 2-dimensional arrays, which are written independently. It should also benoted that, for global data sets, either a Gaussian or cylindrical equidistant projectionmust be used, and for regional data sets, either a Mercator, Lambert conformal, polarstereographic, or cylindrical equidistant may be used. The sequence of writes used towrite a single 2-dimensional array in the WPS intermediate format is as follows (note thatnot all of the variables declared below are used for a given projection of the data).integer :: version! Format version (must =5 for WPS format)integer :: nx, ny! x- and y-dimensions of 2-d arrayinteger :: iproj! Code for projection of data in array:! 0 = cylindrical equidistant! 1 = Mercator!!3 = Lambert conformal conic4 = Gaussian (global only!)! 5 = Polar stereographicreal :: nlats! Number of latitudes north of equator! (for Gaussian grids)real :: xfcst! Forecast hour of datareal :: xlvlreal :: startlat, startlon! Vertical level of data in 2-d array! Lat/lon of point in array indicated by! startloc stringreal :: deltalat, deltalonreal :: dx, dy! Grid spacing, degrees! Grid spacing, kmreal :: xlonc! Standard longitude of projectionreal :: truelat1, truelat2real :: earth_radius! True latitudes of projection! Earth radius, kmreal, dimension(nx,ny) :: slab ! The 2-d array holding the datalogical :: is_wind_grid_rel ! Flag indicating whether winds are! relative to source grid (TRUE) or! relative to earth (FALSE)character (len=8) :: startloc ! Which point in array is given by! startlat/startlon; set either! to 'SWCORNER' or 'CENTER 'character (len=9) :: fieldcharacter (len=24) :: hdate! Name of the field! Valid date for data YYYY:MM:DD_HH:00:00character (len=25) :: units ! Units of datacharacter (len=32) :: map_source ! Source model / originating centercharacter (len=46) :: desc ! Short description of data! 1) WRITE FORMAT VERSIONwrite(unit=ounit) version! 2) WRITE METADATA! Cylindrical equidistantif (iproj == 0) thenwrite(unit=ounit) hdate, xfcst, map_source, field, &units, desc, xlvl, nx, ny, iprojwrite(unit=ounit) startloc, startlat, startlon, &deltalat, deltalon, earth_radius! Mercatorelse if (iproj == 1) thenwrite(unit=ounit) hdate, xfcst, map_source, field, &units, desc, xlvl, nx, ny, iproj<strong>WRF</strong>-NMM V3: User’s Guide 3-25
write(unit=ounit) startloc, startlat, startlon, dx, dy, &truelat1, earth_radius! Lambert conformalelse if (iproj == 3) thenwrite(unit=ounit) hdate, xfcst, map_source, field, &units, desc, xlvl, nx, ny, iprojwrite(unit=ounit) startloc, startlat, startlon, dx, dy, &xlonc, truelat1, truelat2, earth_radius! Gaussianelse if (iproj == 4) thenwrite(unit=ounit) hdate, xfcst, map_source, field, &units, desc, xlvl, nx, ny, iprojwrite(unit=ounit) startloc, startlat, startlon, &nlats, deltalon, earth_radius! Polar stereographicelse if (iproj == 5) thenwrite(unit=ounit) hdate, xfcst, map_source, field, &units, desc, xlvl, nx, ny, iprojwrite(unit=ounit) startloc, startlat, startlon, dx, dy, &xlonc, truelat1, earth_radiusend if! 3) WRITE WIND ROTATION FLAGwrite(unit=ounit) is_wind_grid_rel! 4) WRITE 2-D ARRAY OF DATAwrite(unit=ounit) slabCreating and Editing VtablesAlthough Vtables are provided for many common data sets, it would be impossible forungrib to anticipate every possible source of meteorological data in GRIB format. Whena new source of data is to be processed by ungrib.exe, the user may create a new Vtableeither from scratch, or by using an existing Vtable as an example. In either case, a basicknowledge of the meaning and use of the various fields of the Vtable will be helpful.Each Vtable contains either seven or eleven fields, depending on whether the Vtable isfor a GRIB Edition 1 data source or a GRIB Edition 2 data source, respectively. Thefields of a Vtable fall into one of three categories: fields that describe how the data areidentified within the GRIB file, fields that describe how the data are identified by theungrib and metgrid programs, and fields specific to GRIB Edition 2. Each variable to beextracted by ungrib.exe will have one or more lines in the Vtable, with multiple lines fordata that are split among different level types – for example, a surface level and upper-airlevels. The fields that must be specified for a line, or entry, in the Vtable depends on thespecifics of the field and level.The first group of fields – those that describe how the data are identified within the GRIBfile – are given under the column headings of the Vtable shown below.<strong>WRF</strong>-NMM V3: User’s Guide 3-26
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ForewordUser's Guide for the NMM Co
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• WPP Directory Structure 7-3•
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The WRF modeling system software is
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WRF-NMM FLOW CHARTTerrestrialDataMo
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Vendor Hardware OS CompilerCray X1
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If all of these executables are def
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Once the tar file is obtained, gunz
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HWRF is set, then (3) will be autom
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In addition to these three links, a
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• Real-data simulations• Non-hy
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k. Morrison double-moment scheme (1
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g. GFDL surface layer (88): (This s
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Other physics optionsa. gwd_opt: Gr
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to the convergence of meridians app
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Variable NamesValue(Example)Descrip
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Variable NamesValue(Example)Descrip
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Variable NamesValue(Example)Descrip
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Variable NamesValue(Example)Descrip
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Variable NamesValue(Example)Descrip
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mpirun.lsf wrf.exeand for interacti
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The boundary conditions for the nes
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Examples:1. One nest and one level
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ottom_top_stag = 28 ;soil_layers_st
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float HLENSW(Time, south_north, wes
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float HBOTS(Time, south_north, west
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operational mesoscale Eta model. J.
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Mlawer, E. J., S. J. Taubman, P. D.
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NCEP WRF Postprocessor (WPP)WPP Int
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./configureYou will be given a list
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equested output field. If the pre-r
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RAINCV SNOW HBOTRAINNCVSNOWCNote: F
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Running WPPFour scripts for running
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i. As the grid id of a pre-defined
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The GrADS package is available from
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Height on pressure surface HEIGHT O
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MELTPrecipitation type (4 types) -
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Press at tropopause PRESS AT TROPOP
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RIP4RIP IntroductionRIP (which stan
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A successful compilation will resul
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iinterp = 0v v v v vH V H V h h h h
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espectively, of the centered domain
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- Page 90 and 91: Creating Vis5D Dataset with RIPVis5
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- Page 94 and 95: Configuration: The configure script
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- Page 136 and 137: GRIB1| Level| From | To |Param| Typ
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