Methane heating rates in outer planet atmospheres.

Details Methane heating rates in outer planet atmospheres. Methane heating rates in outer planet atmospheres.

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jqsrt..54..819w&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 54, issue 5, pp. 819-826

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Planetary Atmospheres: Heating, Planetary Atmospheres: Methane

Scientific paper

The authors have reviewed and expanded the techniques for calculating the heating rates of CH4 near-IR bands (3.3, 2.3, and 1.7 μm) for conditions relevant to the atmospheres of the outer planets. They consider all pressures below 100 mbar and temperatures from 77 to 300 K. The authors find that using the correlated-k method, the heating rates of the stronger band, 3.3 μm band, at all pressures and the heating rates for the other two bands at pressures below 0.1 mbar can be accurately calculated. The authors also find that the application of the general random band models which depend on the line listings is not appropriate to these three bands.

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