title: Theoretical far-wing line shape and absorption for high-temperature CO2.
abstract: Theoretical results for the far-wing line shapes and corresponding absorption coefficients in the high-frequency wing of the nu(3) fundamental band of self-broadened CO(2) are presented for a number of temperatures between 218 and 751 K. These first-principles calculations are made assuming binary collisions within the framework of a quasi-static theory with a more accurate interaction potential than in previous calculations. The theoretical results are compared with existing laboratory data and are in good agreement for all the temperatures considered.
authors.affiliation: Department of Applied Physics, Columbia University, and the Institute for Space Studies, Goddard Space Flight Center, 2880 Broadway, New York, New York 10025, USA. qma@giss.nasa.gov
authors.forename: Q
authors.initials: Q
authors.lastname: Ma
authors.forename: R H
authors.initials: RH
authors.lastname: Tipping
authors.forename: C
authors.initials: C
authors.lastname: Boulet
authors.forename: J P
authors.initials: JP
authors.lastname: Bouanich