TOWARDS AN ACCURATE INFRARED LINELIST FOR CO${_2}$ AND ISOTOPOLOGUES

Research Projects

Organizational Units

Journal Issue

Abstract

Following the "Best Theory + High-resolution Experimental Data" strategy, we have completed an initial CO2 infrared (IR) line list, denoted Ames-1. A procedure similar to the one used for ammonia nderline{\textbf129}, 214304 (2008); \textit{J. Chem. Phys.} nderline{\textbf134}, 044320/044321 (2011).} is adopted to generate a global potential energy surface (PES), including various small corrections such as scalar relativity, extrapolation to the one-particle basis-set limit, and a higher-order correlation correction, followed by refinement using accurate high-resolution laboratory data. We will discuss limitations in the use of HITRAN data for the refinement step. The current PES yields uncertainties of 0.01-0.02 cm−1for \textit{J}=0-117 12C16O2 energy levels up to 13,845 cm−1 above the zero-point level. Comparisons between Ames-1, HITRAN, and CDSD will be presented for room temperature as well as selected higher temperatures. Results for 13C, 14C, 17O, and 18O isotopologues will be presented, and the accuracy for isotopologues will be discussed. Limitations of the current PES and the Ames-1 line list together with strategies to improve these will be discussed.

Description

Author Institution: MS 245-1, NASA Ames Research Center, Moffett Field, CA, 94035; SETI Institute, 189 Bernardo Ave, Suite 100, Mountain View, CA, 94043; MS T27B-1, NASA Ames Research Center, Moffett Field, CA, 94035; Laboratory of Theoretical Spectroscopy, V.E. Zuev Institute of Atmospheric Optics, SB, Russian Academy of Science, 634055, Tomsk, Russia

Keywords

Citation