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Table of Contents - The Atmospheric Studies Group at TRC

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Section 10: POSTPROCESSORS<br />

10.5 Input Files<br />

10.5.1 User Control File (CALPOST.INP)<br />

User-specified inputs to CALPOST are read from a control file whose default name is CALPOST.INP. A<br />

description <strong>of</strong> each input variable is shown in <strong>Table</strong> 10-14, and a sample input file is presented in<br />

<strong>Table</strong> 10-15. This control file uses the same self-documenting control file form<strong>at</strong> as CALPUFF. See<br />

Section 9.1 for a description <strong>of</strong> the control file input conventions. Selections may be made by either<br />

editing an existing control file, or by using the CALPOST GUI. Note th<strong>at</strong> you can gener<strong>at</strong>e a new control<br />

file with all <strong>of</strong> the standard options and comments by saving the NEW.INP file from the GUI to disk.<br />

10.5.2 CALPUFF Output Files (MODEL.DAT and VISB.DAT)<br />

<strong>The</strong> program reads the concentr<strong>at</strong>ion/deposition flux d<strong>at</strong>a from an unform<strong>at</strong>ted d<strong>at</strong>a file (default name:<br />

MODEL.DAT) th<strong>at</strong> is gener<strong>at</strong>ed by the CALPUFF model (or CALGRID). CALPUFF also gener<strong>at</strong>es a<br />

file containing rel<strong>at</strong>ive humidity d<strong>at</strong>a (default name: VISB.DAT), which is read by CALPOST if needed<br />

for the visibility option selected. <strong>The</strong> structure <strong>of</strong> these files is described in Section 9-13.<br />

10.5.3 Background Concentr<strong>at</strong>ions/Deposition Fluxes (BACK.DAT)<br />

As an option, a sp<strong>at</strong>ially uniform, hourly background concentr<strong>at</strong>ion/deposition flux can be added to<br />

modeled concentr<strong>at</strong>ions/deposition fluxes before averages are processed in CALPOST. <strong>The</strong>se values are<br />

provided in a form<strong>at</strong>ted ASCII file (default name: BACK.DAT) prepared by the user. <strong>Table</strong> 10-16 lists<br />

the record structure for this file, and a partial listing <strong>of</strong> a sample file is presented in <strong>Table</strong> 10-17.<br />

Units for the background values may be different from those requested from CALPOST. <strong>The</strong>refore, the<br />

scaling factor placed in the header record is an important fe<strong>at</strong>ure. It converts the n<strong>at</strong>ive units for the<br />

background concentr<strong>at</strong>ions to g/m 3 , or it converts the n<strong>at</strong>ive units for background deposition fluxes to<br />

g/m 2 /s. <strong>The</strong>se are the internal units used in the CALPUFF output file. Any units conversion specified in<br />

the control file (parameter IPRTU) can then be applied uniformly to both the CALPUFF and background<br />

values. Note th<strong>at</strong> the multiplic<strong>at</strong>ive and additive scaling factors (A, B) are not applied to the background<br />

values.<br />

10.5.4 Visibility Measurements (VSRN.DAT)<br />

CALPOST allows the use <strong>of</strong> visibility measurements to establish hourly background extinction for use in<br />

assessing the change in visibility resulting from modeled emissions. Two form<strong>at</strong>s are supported for these<br />

d<strong>at</strong>a, and both are taken from the d<strong>at</strong>a files available on CD-ROM from the Interagency Monitoring <strong>of</strong><br />

Protected Visual Environments (IMPROVE) program. When background extinction method number 4 is<br />

selected in the control file (MVISBK = 4), transmissometer measurements must be provided in the<br />

10-46

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