Table of Contents - The Atmospheric Studies Group at TRC

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Section 10: POSTPROCESSORS CALPOST generates an output list file (default name: CALPOST.LST) and a set of optional files. The names for the optional files follow a fixed template, with one or more characters reserved for the user to specify in order to distinguish output from multiple applications. For example, a plot-file in GRID format containing the highest second-high 24-hour average concentration of species ASPEC at each receptor would be called: RANK(02)_ASPEC_24HR_CONC_TEST1.grd where "TEST1" is the user-specified run identifier. If the user does not enter a run identifier, the file would be called: RANK(02)_ASPEC_24HR_CONC.grd A plot-file in DATA format containing the number of exceedances of a 3-hour concentration threshold specified by the user for species ASPEC with a run identifier "TEST2" would be called: EXCEED_ASPEC_03HR_CONC_TEST2.dat Plot-files in GRID format containing 8-hour average concentrations of species ASPEC for Julian Day 112 in 1995 (April 22) in base time zone 5 (EST in the USA) would be called 1995_M04_D22_0000(UTC-0500)_L00_ASPEC_08HR_CONC.GRD 1995_M04_D22_0800(UTC-0500)_L00_ASPEC_08HR_CONC.GRD 1995_M04_D22_1600(UTC-0500)_L00_ASPEC_08HR_CONC.GRD A visibility analysis with a run identifier "TOTAL" would generate the plot-file: DAILY_VISIB_TOTAL.DAT As with CALPUFF and CALMET, CALPOST is configured by means of a parameter file, called PARAMS.PST, in which all of the array dimensions related to the number of gridded, discrete, and complex terrain receptors, the number of "top N" tables allowed, and the Fortran unit numbers associated with each input and output file are specified. If for a particular application, the user needs to increase the number of discrete receptors, for example, beyond the current maximum, a change to the value of the discrete receptor parameter in PARAMS.PST will automatically re-size all arrays related to this parameter upon recompilation of the CALPOST code. 10-45
Section 10: POSTPROCESSORS 10.5 Input Files 10.5.1 User Control File (CALPOST.INP) User-specified inputs to CALPOST are read from a control file whose default name is CALPOST.INP. A description of each input variable is shown in Table 10-14, and a sample input file is presented in Table 10-15. This control file uses the same self-documenting control file format as CALPUFF. See Section 9.1 for a description of the control file input conventions. Selections may be made by either editing an existing control file, or by using the CALPOST GUI. Note that you can generate a new control file with all of the standard options and comments by saving the NEW.INP file from the GUI to disk. 10.5.2 CALPUFF Output Files (MODEL.DAT and VISB.DAT) The program reads the concentration/deposition flux data from an unformatted data file (default name: MODEL.DAT) that is generated by the CALPUFF model (or CALGRID). CALPUFF also generates a file containing relative humidity data (default name: VISB.DAT), which is read by CALPOST if needed for the visibility option selected. The structure of these files is described in Section 9-13. 10.5.3 Background Concentrations/Deposition Fluxes (BACK.DAT) As an option, a spatially uniform, hourly background concentration/deposition flux can be added to modeled concentrations/deposition fluxes before averages are processed in CALPOST. These values are provided in a formatted ASCII file (default name: BACK.DAT) prepared by the user. Table 10-16 lists the record structure for this file, and a partial listing of a sample file is presented in Table 10-17. Units for the background values may be different from those requested from CALPOST. Therefore, the scaling factor placed in the header record is an important feature. It converts the native units for the background concentrations to g/m 3 , or it converts the native units for background deposition fluxes to g/m 2 /s. These are the internal units used in the CALPUFF output file. Any units conversion specified in the control file (parameter IPRTU) can then be applied uniformly to both the CALPUFF and background values. Note that the multiplicative and additive scaling factors (A, B) are not applied to the background values. 10.5.4 Visibility Measurements (VSRN.DAT) CALPOST allows the use of visibility measurements to establish hourly background extinction for use in assessing the change in visibility resulting from modeled emissions. Two formats are supported for these data, and both are taken from the data files available on CD-ROM from the Interagency Monitoring of Protected Visual Environments (IMPROVE) program. When background extinction method number 4 is selected in the control file (MVISBK = 4), transmissometer measurements must be provided in the 10-46
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CALPUFF Modeling System Version 6 U
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Section 1: Introduction 7.5 CALWRF
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Section 1: Introduction List of Fig
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Section 1: Introduction Table 3-1:
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Section 1: Introduction introductio
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Section 1: Introduction released a
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Section 1: Introduction CALMET Upd
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Section 1: Introduction To enhance
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Section 1: Introduction Meteorologi
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Section 1: Introduction READ62 is a
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Section 1: Introduction contained i
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Section 1: Introduction OPTHILL uti
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Section 1: Introduction From CALPUF
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Section 1: Introduction Observation
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Section 1: Introduction Slope Flows
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Section 1: Introduction CALPUFF con
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Section 1: Introduction 1.5 Summary
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Section 1: Introduction If the uppe
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Section 1: Introduction Table 1-5 (
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Section 1: Introduction 1-44
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Section 1: Introduction technical o
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Section 2: Geophysical Data Process
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Section 3: READ62 Upper Air Preproc
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Section 5: PMERGE Precipitation Dat
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Section 6: SMERGE Surface Data Mete
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Section 7: Prognostic Meteorologica
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Section 8: CALMET Model Files (e.g.
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Section 8: CALMET Model Files Table
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Section 8: CALMET Model Files descr
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Section 8: CALMET Model Files range
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Section 8: CALMET Model Files recor
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Section 8: CALMET Model Files 8.10
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Section 8: CALMET Model Files 4 NUS
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Section 8: CALMET Model Files CALME
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Section 8: CALMET Model Files 8.1.1
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Section 8: CALMET Model Files ┌
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Section 8: CALMET Model Files 8.2 P
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Section 8: CALMET Model Files -----
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Section 8: CALMET Model Files 6 0 0
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Section 8: CALMET Model Files 3 1 1
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Section 8: CALMET Model Files IBHR
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Section 8: CALMET Model Files Multi
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Section 9: CALPUFF 9. CALPUFF The C
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Section 9: CALPUFF The control file
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Section 9: CALPUFF Table 9-1: Input
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Section 9: CALPUFF 17a,b Non-gridde
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Section 9: CALPUFF MASSBAL.DAT outp
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Section 9: CALPUFF d The filenames
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Section 9: CALPUFF >0 = File update
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Section 9: CALPUFF 0 = chemical tra
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Section 9: CALPUFF [DIAGNOSTIC FEAT
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Section 9: CALPUFF ! CSPEC = SO2 !
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Section 9: CALPUFF WGS-84 NAS-C NAR
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Section 9: CALPUFF for selected spe
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Section 9: CALPUFF ---------------
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Section 9: CALPUFF --------- ------
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Section 9: CALPUFF Input Group 11 O
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Section 9: CALPUFF (XLAIIN) Default
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Section 9: CALPUFF Minimum mixing h
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Section 9: CALPUFF Near-Surface dep
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Section 9: CALPUFF Sample CALPUFF C
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Section 9: CALPUFF -------- a Data
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Section 9: CALPUFF Number of buoyan
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Section 9: CALPUFF -------- a Data
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Section 9: CALPUFF Number of non-gr
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Section 9: CALPUFF 9-47
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Section 9: CALPUFF Table 9-3 (Conti
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Section 9: CALPUFF IOUTU IOVERS int
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Section 9: CALPUFF MSHEAR integer V
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Section 9: CALPUFF MDISP integer Me
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Section 9: CALPUFF MPDF integer Pro
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Section 9: CALPUFF IMFLX integer Co
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Section 9: CALPUFF IPRTU integer Co
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Section 9: CALPUFF BCKNH3(12) real
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Section 9: CALPUFF CDIV(2) real Div
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Section 9: CALPUFF *MDEPBC integer
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Section 9: CALPUFF BDOWN real Build
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Section 9: CALPUFF source is treate
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Section 9: CALPUFF (i.e., !END!). I
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Section 9: CALPUFF (i.e., !END!). I
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Section 9: CALPUFF terminator (i.e.
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Section 9: CALPUFF Table 9-3 (Concl
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Section 9: CALPUFF 9.2 Meteorologic
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Section 9: CALPUFF if(nssta.ge.1)th
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Section 9: CALPUFF Table 9-4: CALME
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Section 9: CALPUFF Table 9-4 (Concl
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Section 9: CALPUFF 4 b 6 ZTEMP real
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Section 9: CALPUFF 9 6 WSTAR real a
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Section 9: CALPUFF 14 6 IRH integer
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Section 9: CALPUFF variable dispers
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Section 9: CALPUFF Table 9-6: Sampl
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Section 9: CALPUFF NCOMM+6 * intege
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Section 9: CALPUFF Table 9-8 (conti
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Section 9: CALPUFF table. A descrip
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Section 9: CALPUFF Table 9-10: PLMM
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Section 9: CALPUFF 9.2.4 SURFACE.DA
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Section 9: CALPUFF Table 9-12: Samp
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Section 9: CALPUFF Table 9-13 (cont
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Section 9: CALPUFF Table 9-14: SURF
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Section 9: CALPUFF Table 9-14 (conc
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Section 9: CALPUFF Table 9-15 (cont
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Section 9: CALPUFF 9.3 Point Source
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Section 9: CALPUFF Table 9-17: PTEM
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Section 9: CALPUFF Table 9-17 (Cont
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Section 9: CALPUFF 9.4 Buoyant Area
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Section 9: CALPUFF Table 9-21: BAEM
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Section 9: CALPUFF . . . . . . . .
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Section 9: CALPUFF Table 9-23 (Conc
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Section 9: CALPUFF NCOMM+8 or 9 IEJ
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Section 9: CALPUFF Table 9-26: LNEM
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Section 9: CALPUFF a C*16 = Charact
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Section 9: CALPUFF * "NSE" elements
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Section 9: CALPUFF 9.7 Boundary Con
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Section 9: CALPUFF Table 9-32: Boun
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Section 9: CALPUFF The model checks
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Section 9: CALPUFF 9.11 Site-Specif
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Section 9: CALPUFF Table 9-43: HILL
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Section 9: CALPUFF where the follow
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Section 9: CALPUFF 9.14 Mass Flux B
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Section 9: CALPUFF Table 9-49: FLUX
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Section 9: CALPUFF 9.15 CALPUFF Out
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Section 9: CALPUFF 1 XRCT real arra
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Section 9: CALPUFF C*16 = Character
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Section 9: CALPUFF C*16 = Character
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Section 9: CALPUFF CONC.DAT File -
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Section 9: CALPUFF 9.15.4 Dry Flux
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Section 9: CALPUFF 24 IBSAMP intege
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Section 9: CALPUFF nxg = IESAMP - I
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Section 9: CALPUFF 5 SYKM real Sour
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Section 9: CALPUFF 9.15.6 Relative
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Section 9: CALPUFF a C*15 = Charact
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Section 9: CALPUFF 16 Length Emitte
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Section 9: CALPUFF Figure 9-1: Prof
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Section 10: POSTPROCESSORS Table 10
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