Hostname: page-component-848d4c4894-ttngx Total loading time: 0 Render date: 2024-05-01T22:55:18.092Z Has data issue: false hasContentIssue false
  • English
  • Français

SO2 and CO2 IR line lists for atmospheric modeling on Venus and Exoplanets

Published online by Cambridge University Press:  18 July 2017

Xinchuan Huang ,
David W. Schwenke  and
Timothy J. Lee
Xinchuan Huang
Affiliation:
SETI Institute, 189 Bernardo Ave, Suite 100, Mountain View, CA 94043, USA email: Xinchuan.Huang-1@nasa.gov
David W. Schwenke
Affiliation:
NASA Ames Research Center emails: David.W.Schwenke@nasa.gov, Timothy.J.Lee@nasa.gov
Timothy J. Lee
Affiliation:
NASA Ames Research Center emails: David.W.Schwenke@nasa.gov, Timothy.J.Lee@nasa.gov
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Highly accurate IR line lists are ready for 13 CO2 isotopologues and 7 SO2 isotopologues. Ames-296K IR lists carry 0.01 - 0.03 cm−1 accuracy up to 13,000 cm−1 for CO2 and 5500 cm−1 for SO2, and 90–95% intensity agreement for most observable bands. Good for atmospheric modeling on Venus and Exoplanets.

Keywords

CO2SO2isotopologueInfraredline listab initiohighly accuratemodeling
Type
Addendum
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , E16
Copyright
Copyright © International Astronomical Union 2017