Update of the HITRAN collision-induced absorption sectionShow others and affiliations
2019 (English)In: Icarus, 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 N2
N2, N2
H2, N2-CH4, N2
H2O, N2
O2, O2
O2, O2-CO2, CO2-CO2, H2
H2, H2
He, H2-CH4, H2
H, H
He, CH4-CH4, CH4-CO2, CH4
He, and CH4
Ar 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)
2019-03-192019-03-192023-10-28Bibliographically approved