Theoretical modelling of the methane absorption spectrum for planetary applications

Details Theoretical modelling of the methane absorption spectrum for planetary applications Theoretical modelling of the methane absorption spectrum for planetary applications

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..115b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.115

Physics

Scientific paper

Methane is a key species in many planetary atmospheres, including Titan,
the giant planets and exoplanets. In this paper, we present the
state-of-theart of line-by-line (line positions, line intensities and
line broadening) modeling of the CH4 infrared absorption spectrum. We
also discuss the perspectives and future directions of this topic.

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