Update of the HITRAN collision-induced absorption section

By T. Karman, I. Gordon, A. van der Avoird, Y. Baranov, C. Boulet, B. Drouin, G. Groenenboom, M. Gustafsson, J. Hartmann, R. Kurucz and 10 more. Icarus (New York, N.Y. 1962), 2019

160 citations recorded by the source corpus.

Abstract 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.

Subfields: Atmospheric Science, Global and Planetary Change, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/e5968d09be22c169d3c3b4aa4ba13f387f7923ce

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In Atmospheric Science

1. Mercedes López-Morales
2. J. Lustig-Yaeger
3. D. Sing
4. Kevin B. Stevenson
5. H. Wakeford
6. Z. Rustamkulov

In Global and Planetary Change

1. J. Lustig-Yaeger
2. Z. Rustamkulov

In Spectroscopy

1. Mercedes López-Morales
2. J. Lustig-Yaeger
3. D. Sing
4. H. Wakeford
5. Z. Rustamkulov

Citations in the corpus

• High Tide or Riptide on the Cosmic Shoreline? A Water-rich Atmosphere or Stellar Contamination for the Warm Super-Earth GJ 486b from JWST Observations (2023, background): “The opacity contributions from these gases include line opacity (Tashkun & Perevalov 2011; Li et al. 2015; Yurchenko et al. 2017; Polyansky et al. 2018) and collision-induced absorption (CIA) from H2–H2, H2–N2, H2–CH4, H2–CO2, CO2–CO2, CO2–CH4, and N2–N2 (Karman et al. 2019).”