Interference of spectral lines in thermal radiation from the lower atmosphere of Venus

Details Interference of spectral lines in thermal radiation from the lower atmosphere of Venus Interference of spectral lines in thermal radiation from the lower atmosphere of Venus

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007astl...33..203a&link_type=abstract

Astronomy Letters, Volume 33, Issue 3, pp.203-210

Astronomy and Astrophysics

Astronomy

3

Scientific paper

The absorption spectrum and thermal radiation fluxes in the lower atmosphere of Venus are calculated using the theory of molecular state interference in the strong collision approximation. Comparison is made with the absorption and radiative transfer calculations in terms of the statistical theory of collisional line broadening and based on an empirical form factor. The calculations show that the line broadening mechanism does not affect the thermal regime of the atmosphere at heights above 60 km, but affects significantly the behavior of the greenhouse effect below the cloud layer.

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