USF Hitran-PC Version 4 Demo
Download a free Hitran-PC 4 Demo version and user manual.
Hitran-PC Version 4: Bug list, fixes and update history list.
- Hitran-PC Version 4.1 (Released October 28, 2009)
- Hitran-PC Version 4.0 (Released September 10, 2009)
- Hitran-PC Beta version (Released June 11, 2009)
Hitran-PC is a PC software program that can calculate or model the high-resolution
( < 0.01 cm-1 ) optical transmission spectrum of the atmosphere and of selected
gases using primarily the HITRAN Line-by-Line molecular absorption database.
Hitran-PC has been developed over the past 20 years with application toward
the modeling of the transmission and absorption of a laser beam propagating through the atmosphere.
Hitran-PC has been developed with various levels of improvements and capability, starting with Version
1.0 in 1991 through Version 4.0 in 2009. The latest version uses the 2008 HITRAN Line-by-Line
database, but also uses the HITRAN UV and IR Cross Section files, the experimental PNNL IR database,
aerosol extinction using the BACKSCAT program, and the water vapor, CO2 and N2 Continuum. The following
figure is a transmission of the atmosphere from 3.3 to 5 micron in wavelength for a path of 1000 meters. |
The transmission (and absorption) spectrum of the atmosphere can be calculated over a spectral wavelength
range for a given path length, using supplied models of the atmosphere (i.e. US Standard Atmosphere) or
user specified pressure, temperature, lineshape (pressure, Doppler, Voigt), and partial pressures of a
variety of gases as a function of altitude, and for horizontal paths and slant path geometries.
In addition, the user can select one or more specific gases or isotopes in order to study the individual
spectrum for those particular gases. The irradiance of a gas plume or a hot target through the atmosphere
can also be displayed. The user can smooth the resultant optical spectrum to simulate the finite
resolution of an optical instrument, or overlay known laser lines to help decide which to use for
atmospheric laser remote sensing. |
The overall operation of Hitran-PC 4.0 is shown in the following figure. As can be seen, the user can specify
the path length, temperature, concentration, line shape (Pressure, Voigt, etc.), and other parameters
pertaining to the transmission of the atmosphere. These startup parameters can also be stored in a
configuration file for easy use at a later time. The startup parameters are then used along with
atmospheric models of pressure/temperature/altitude to model the geometry of the optical transmission
path through the gas or atmosphere. Both horizontal and slant path spectral calculations can be made.
In the figure, the Main Program screen is shown, along with the Info Panel which contains the Working
Parameters for the input parameters and databases, for easy modification and control by the user. |
As can be seen in the figure, the top screen of the Main Program is shown for a typical Horizontal Path
calculation showing the color coded absorption spectrum of individual gases. Another option is shown
in the middle screen which displays the slant path calculation of the transmission as a function of wavelength. |
In this mode, the user can easily insert a gas plume or cloud of a specified gas (i.e, from the PNNL
database) into the optical path at a specified range. Finally, the program can also calculate the
radiance for a hot target or a gas plume as shown in the lower example.
The databases and spectral calculations used by Hitran-PC 4.0 consist of:
(1) the main HITRAN Line-by-Line (LBL) database consisting of about several million individual
absorption lines of gases in the atmosphere (modeled with a spectral resolution greater than 0.001 cm-1),
(2) the experimental infrared PNNL database of environmental and chemical gases for about 400 gases (with a spectral
resolution on the order of 0.1 cm-1),
(3) the Continuum models for the far-wings of water vapor, CO2, and N2 that add up to a few percent attenuation
over a wide spectral range,
(4) the HITRAN cross section models that give the attenuation for UV and IR gases, and
(5) the BACKSCAT (Version 4.0) attenuation due to aerosols (clouds, fogs, dust) which is the same as the
US Air Force LOWTRAN7 model.
Hitran-PC 4.0 uses the HITRAN LBL as the main calculation for atmospheric
attenuation, but allows the user to add in the other spectral contributions also. For example, the user
can specify the HITRAN LBL for the transmission of the atmosphere, add in the attenuation due to fog or urban
haze, and then use the PNNL database to add the attenuation of a 10 m plume of a particular gas at a specified
range. The calculated spectrums can be stored in data files, for further use by the user.
Hitran-PC 4.0 program improvements
The main improvements to the Hitran-PC 4.0 program compared to version 3.0 include: |
→   Hitran-PC 4.0 competely rewritten in Visual Basic.NET to operate under the NET Framework
→   HITRAN 2008-2004 format database usage on CD/DVD, or a harddrive, etc.
→   Ability to carry out calculations for individual isotopes
→   Addition of Aerosols (BACKSCAT 4.0 model, BACKSCAT 4.0 manual is available here)
→   Addition of HITRAN Cross-sections into calculations
→   Introduction of PNNL IR database into calculations
→   Combined use of HITRAN line-by-line, HITRAN Cross-sections, PNNL IR and aerosols data
→   Temperature recalculation routine updated
→   Hitran-PC is now supplied with a new version of the Betaspec 2.0 program
Some of the major interface improvements include:
→   Addition of the "Info Panel" for easy access to parameters and their manipulation
→   Ability to zoom in and zoom out a selected portion of a spectrum
→   Ability to view separate lines or total spectra for separate isotopes or separate molecules
→   Improved "Slant path layer editor"
→   Option to save calculations to multicolumn TXT files for easy export to other programs
Hitran-PC uses the HITRAN database for transmission simulations. The HITRAN database is maintained and distributed
by the Harvard-Smithsonian Center for Astrophysics. If you would like to learn more about the HITRAN
database please visit www.hitran.com. |
To download the HITRAN database free of charge from the Harvard-Smithsonian Center for Astrophysics,
you need to fill out the following request form
at their website.
The PNNL IR database was developed and distributed by the Pacific Northwest National Laboratory. If you would
like to learn more about the PNNL Infrared database please visit
PNNL IR database website. The PNNL database is released on the
following conditions. |
Technical questions about Hitran-PC
For technical questions please contact: |
Prof. Dennis Killinger
University of South Florida
Tampa, FL, 33620
Hitran-PC is distributed by Ontar Corporation: |
9 Village Way
North Andover MA 01845-2000
FAX: (508) 681-4585