An analytical method similar to that used by (1) on Lorentz lines was applied to the problem of the growth of an isolated Doppler line for the case of nonisothermal paths. The results, given in terms of the total radiance (N) and equivalent width (W) of the line, are: W = ([pi]/ln 2)1/2[gamma]eg(xL) where is the function obtained by (4) for the isothermal case, [gamma]e is an effective spectral line half-width, N*v( g) is the Planck function of the local temperature in the emitting-absorbing gas, the nondimensional optical depth is defined by dx = (ln2/[pi])1/2[S(X)G(X)dX]/[gamma]e, where S(X) is the local value of the line strength, dX is the in crement of standard optical depth, and G(X) is a function characterizing the temperature depen...
Four styles of spectral line shape function and their transformation relation were investigated theo...
Methods are described for calculating the spectral absorption coefficient for lines with combined Do...
The similarity groups for multicomponent, reacting gas mixtures with radiative energy transport are ...
Analytical expressions for total radiances and equivalent widths of isolated spectral lines with com...
The relativistic Doppler broadening of the line emission from both thermal and power-law particle di...
The experimental determination of absolute intensities for isolated spectral lines or for entire vib...
Methods for the calculation of spectral absorption coefficients for combined Doppler and Lorentz bro...
Equations are developed for observable intensities in emission and absorption for spectral lines wit...
International audienceWe describe the theory and the numerical model used to simulate Doppler-broade...
The escape probability method introduced by Sobolev (1947) is used to derive the mean intensity of t...
The relativistic Doppler-broadened profile of an absorption line due to the thermal motion of light-...
Author Institution:Semiconductor diode laser (SDL) spectrometers, such as the Laser Analytics Model ...
We present an algorithm that allows the efficient determination of the dispersion and Doppler contri...
We present a list of 61 solar photospheric lines in the near-infrared H-band (1500 - 1800 nm), obtai...
A novel approach to Doppler-width thermodynamic thermometry based upon line-absorbance analysi
Four styles of spectral line shape function and their transformation relation were investigated theo...
Methods are described for calculating the spectral absorption coefficient for lines with combined Do...
The similarity groups for multicomponent, reacting gas mixtures with radiative energy transport are ...
Analytical expressions for total radiances and equivalent widths of isolated spectral lines with com...
The relativistic Doppler broadening of the line emission from both thermal and power-law particle di...
The experimental determination of absolute intensities for isolated spectral lines or for entire vib...
Methods for the calculation of spectral absorption coefficients for combined Doppler and Lorentz bro...
Equations are developed for observable intensities in emission and absorption for spectral lines wit...
International audienceWe describe the theory and the numerical model used to simulate Doppler-broade...
The escape probability method introduced by Sobolev (1947) is used to derive the mean intensity of t...
The relativistic Doppler-broadened profile of an absorption line due to the thermal motion of light-...
Author Institution:Semiconductor diode laser (SDL) spectrometers, such as the Laser Analytics Model ...
We present an algorithm that allows the efficient determination of the dispersion and Doppler contri...
We present a list of 61 solar photospheric lines in the near-infrared H-band (1500 - 1800 nm), obtai...
A novel approach to Doppler-width thermodynamic thermometry based upon line-absorbance analysi
Four styles of spectral line shape function and their transformation relation were investigated theo...
Methods are described for calculating the spectral absorption coefficient for lines with combined Do...
The similarity groups for multicomponent, reacting gas mixtures with radiative energy transport are ...