Real line strength distributions for random band models

Details Real line strength distributions for random band models Real line strength distributions for random band models

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jqsrt..29..151k&link_type=abstract

Journal of Quantitative Spectroscopy and Radioactive Transfer, vol. 29, Feb. 1983, p. 151-156.

Other

2

Infrared Spectra, Planetary Radiation, Spectral Bands, Spectral Line Width, Molecular Spectra, Radiative Transfer, Solar System, Spectral Energy Distribution

Scientific paper

An improved random band-model method, which makes allowance for the real line-strength distribution, is proposed. The model is shown to be useful for low-resolution, infrared observational data of the outer solar system. The method can be used as easily as conventional random band calculations. In the illustrative examples cited here, the variation of line width with J, the rotational quantum number, is small. Other effects which can, in principle, cause the model to deviate from laboratory observations are discussed. These include the assumption that line positions are random, ignoring the effects of the Lorentz wings of lines immediately outside the specific interval for which the mean transmission is calculated, and ignoring the effects of instrumental slit functions.

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