This report describes an algorithm for the accelerated computation of the convolution of a Lorentz line shape (pressure broadened) with spectral line data. A computational savings of approximately 10 has been achieved over conventional methods. The Lorentz function has been decomposed into three functions, each of which is convolved independently at optional sampling intervals. Criteria for the determination of the sampling interval of the Lorentz function for a resultant error of 0.1 percent is described. The report contains a listing of the computer program based on the algorithm and sample results in the spectral region 3550 to 3650/cm due to water and carbon dioxide."Optical Physics Division Project 2310.""ADA047515 (from http://www.dti...
To deduce accurate infrared molecular line parameters (positions at zero pressure, pressure-shiftin...
International audienceCoefficients of the broadening of ozone lines by nitrogen and oxygen pressure ...
Author Institution: Obukhov Institute of Atmospheric Physics, Siberian Branch, Russian Academy of Sc...
Methods are described for calculating the spectral absorption coefficient for lines with combined Do...
1. J. H. Pierluissi, P. C. Vanderwood, and R. B. Gomez, JQSRT, 18, 555 (1977).Author Institution:Pre...
Author Institution: Astronomy Research Facility, University of MassachusettsThe contour of isolated ...
Methods for the calculation of spectral absorption coefficients for combined Doppler and Lorentz bro...
Abstract-The most important sources of error incurred in the measurements of spectral-line parameter...
Author Institution: Astronomy Research Facility, University of MassachusettsThe combined equivalent ...
We present new models which provide satisfactory and low cost modeling of infrared absorption spectr...
A new method of retrieving quantitative information on the hard, soft, and diffraction collision’s f...
Fourier transform infrared (FTIR) spectroscopy has become a powerful tool for the detection and mea...
The standard description of molecular line shapes in spectral databases and radiative transfer codes...
An algorithm is constructed for solving the problem of diagnostics of an optically dense plasma from...
Author Institution: Université Libre de Bruxelles, Roosevelt ave, 50, B-1050, Brussels, Belgium.We h...
To deduce accurate infrared molecular line parameters (positions at zero pressure, pressure-shiftin...
International audienceCoefficients of the broadening of ozone lines by nitrogen and oxygen pressure ...
Author Institution: Obukhov Institute of Atmospheric Physics, Siberian Branch, Russian Academy of Sc...
Methods are described for calculating the spectral absorption coefficient for lines with combined Do...
1. J. H. Pierluissi, P. C. Vanderwood, and R. B. Gomez, JQSRT, 18, 555 (1977).Author Institution:Pre...
Author Institution: Astronomy Research Facility, University of MassachusettsThe contour of isolated ...
Methods for the calculation of spectral absorption coefficients for combined Doppler and Lorentz bro...
Abstract-The most important sources of error incurred in the measurements of spectral-line parameter...
Author Institution: Astronomy Research Facility, University of MassachusettsThe combined equivalent ...
We present new models which provide satisfactory and low cost modeling of infrared absorption spectr...
A new method of retrieving quantitative information on the hard, soft, and diffraction collision’s f...
Fourier transform infrared (FTIR) spectroscopy has become a powerful tool for the detection and mea...
The standard description of molecular line shapes in spectral databases and radiative transfer codes...
An algorithm is constructed for solving the problem of diagnostics of an optically dense plasma from...
Author Institution: Université Libre de Bruxelles, Roosevelt ave, 50, B-1050, Brussels, Belgium.We h...
To deduce accurate infrared molecular line parameters (positions at zero pressure, pressure-shiftin...
International audienceCoefficients of the broadening of ozone lines by nitrogen and oxygen pressure ...
Author Institution: Obukhov Institute of Atmospheric Physics, Siberian Branch, Russian Academy of Sc...