Infrared radiative transfer in planetary atmospheres. I - Effects of computational and spectroscopic economies on thermal heating/cooling rates

Details Infrared radiative transfer in planetary atmospheres. I - Effects of computational and spectroscopic economies on thermal heating/cooling rates Infrared radiative transfer in planetary atmospheres. I - Effects of computational and spectroscopic economies on thermal heating/cooling rates

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jqsrt..16..505h&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 16, June 1976, p. 505-520.

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Computation

8

Atmospheric Heating, Infrared Radiation, Infrared Spectroscopy, Planetary Atmospheres, Radiant Cooling, Radiative Transfer, Atmospheric Radiation, Carbon Dioxide, Graphs (Charts), Line Shape, Mathematical Models, Ozone, Radiation Absorption, Water Vapor

Scientific paper

The availability of accurate spectroscopic data and improved knowledge of continuum absorption characteristics has required a further detailed study of IR radiative transfer. A sophisticated radiative transfer scheme based upon the Mayer-Goody random band model is developed and the derived transmissivities for H2O, CO2 and O3 are calibrated against laboratory measurements. This calibrated scheme is used to assess the effects on calculated heating/cooling rate profiles of introducing computational and spectroscopic economies.

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