MD simulations of the RT CIA of CO2 for the atmosphere of Venus

Details MD simulations of the RT CIA of CO2 for the atmosphere of Venus MD simulations of the RT CIA of CO2 for the atmosphere of Venus

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..386..429g&link_type=abstract

The 13th international conference on spectral line shapes. AIP Conference Proceedings, Volume 386, pp. 429-430 (1997).

Computer Science

2

Line And Band Widths, Shapes, And Shifts, Venus

Scientific paper

The Roto-Translational (RT) collision-induced absorption (CIA) spectra of gaseous CO2 were computed using molecular dynamics (MD) simulations. By adjusting an overlap contribution to the multipolar induction, a good agreement between MD simulations and existing experiments (233 K to 400 K) was achieved. Based on these results an analytical model of the CIA spectral profile from 200 K to 800 K for modeling of Venus' atmosphere is proposed.

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