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Update of the HITRAN collision-induced absorption section
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA. Radboud University, Nijmegen, the Netherlands. Durham University, United Kingdom.
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA.
Radboud University, Nijmegen, the Netherlands.
Institute of Experimental Meteorology, Obninsk, Russia.
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2019 (English)In: Icarus (New York, N.Y. 1962), ISSN 0019-1035, E-ISSN 1090-2643, Vol. 328, p. 160-175Article in journal (Refereed) Published
Abstract [en]

Correct parameterization of the Collision-induced Absorption (CIA) phenomena is essential for accurate modeling of planetary atmospheres. The HITRAN spectroscopic database provides these parameters in a dedicated section. Here, we significantly revise and extend the HITRAN CIA data with respect to the original effort described in Richard et al. [JQSRT 113, 1276 (2012)]. The extension concerns new collisional pairs as well as wider spectral and temperature ranges for the existing pairs. The database now contains CIA for N2N2, N2H2, N2-CH4, N2H2O, N2O2, O2O2, O2-CO2, CO2-CO2, H2H2, H2He, H2-CH4, H2H, HHe, CH4-CH4, CH4-CO2, CH4He, and CH4Ar collision pairs. The sources of data as well as their validation and selection are discussed. A wish list to eliminate remaining deficiencies or lack of data from the astrophysics perspective is also presented.

Place, publisher, year, edition, pages
Elsevier, 2019. Vol. 328, p. 160-175
National Category
Atom and Molecular Physics and Optics Other Physics Topics
Research subject
Applied Physics
Identifiers
URN: urn:nbn:se:ltu:diva-73252DOI: 10.1016/j.icarus.2019.02.034ISI: 000469159500014Scopus ID: 2-s2.0-85063527773OAI: oai:DiVA.org:ltu-73252DiVA, id: diva2:1297177
Funder
Knut and Alice Wallenberg Foundation
Note

Validerad;2019;Nivå 2;2019-04-08 (svasva)

Available from: 2019-03-19 Created: 2019-03-19 Last updated: 2019-06-19Bibliographically approved

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Gustafsson, Magnus

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