Update of the HITRAN collision-induced absorption section

Tijs Karman; Iouli E. Gordon; Ad van der Avoird; Yury I. Baranov; Christian Boulet; Brian J. Drouin; Gerrit C. Groenenboom; Magnus Gustafsson; Jean Michel Hartmann; Robert L. Kurucz; Laurence S. Rothman; Kang Sun; Keeyoon Sung; Ryan Thalman; Ha Tran; Edward H. Wishnow; Robin Wordsworth; Andrey A. Vigasin; Rainer Volkamer; Wim J. van der Zande

doi:10.1016/j.icarus.2019.02.034

Update of the HITRAN collision-induced absorption section

Tijs Karman
, Iouli E. Gordon
, Ad van der Avoird
, Yury I. Baranov
, Christian Boulet
, Brian J. Drouin
, Gerrit C. Groenenboom
, Magnus Gustafsson
, Jean Michel Hartmann
, Robert L. Kurucz
, Laurence S. Rothman
, Kang Sun
, Keeyoon Sung
, Ryan Thalman
, Ha Tran
, Edward H. Wishnow
, Robin Wordsworth
, Andrey A. Vigasin
, Rainer Volkamer
, Wim J. van der Zande

Department of Civil, Structural & Environmental Engineering

Harvard-Smithsonian Center for Astrophysics
Radboud University Nijmegen
Durham University
Research and Production Association Typhoon
Institut des Sciences Moléculaires d'Orsay
Jet Propulsion Laboratory, California Institute of Technology
Luleå University of Technology
Sorbonne Université
University of Colorado Boulder
Snow College
University of California at Berkeley
Harvard University
Russian Academy of Sciences

Research output: Contribution to journal › Article › peer-review

186 Scopus citations

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 N ₂ -N ₂ , N ₂ -H ₂ , N ₂ -CH ₄ , N ₂ -H ₂ O, N ₂ -O ₂ , O ₂ -O ₂ , O ₂ -CO ₂ , CO ₂ -CO ₂ , H ₂ -H ₂ , H ₂ -He, H ₂ -CH ₄ , H ₂ -H, H-He, CH ₄ -CH ₄ , CH ₄ -CO ₂ , CH ₄ -He, and CH ₄ -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.

Original language	English
Pages (from-to)	160-175
Number of pages	16
Journal	Icarus
Volume	328
DOIs	https://doi.org/10.1016/j.icarus.2019.02.034
State	Published - Aug 2019

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10.1016/j.icarus.2019.02.034

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Karman, T., Gordon, I. E., van der Avoird, A., Baranov, Y. I., Boulet, C., Drouin, B. J., Groenenboom, G. C., Gustafsson, M., Hartmann, J. M., Kurucz, R. L., Rothman, L. S., Sun, K., Sung, K., Thalman, R., Tran, H., Wishnow, E. H., Wordsworth, R., Vigasin, A. A., Volkamer, R., & van der Zande, W. J. (2019). Update of the HITRAN collision-induced absorption section. Icarus, 328, 160-175. https://doi.org/10.1016/j.icarus.2019.02.034

@article{2620762c30f045ff977b32260c75562e,

title = "Update of the HITRAN collision-induced absorption section",

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 N 2 -N 2 , N 2 -H 2 , N 2 -CH 4 , N 2 -H 2 O, N 2 -O 2 , O 2 -O 2 , O 2 -CO 2 , CO 2 -CO 2 , H 2 -H 2 , H 2 -He, H 2 -CH 4 , H 2 -H, H-He, CH 4 -CH 4 , CH 4 -CO 2 , CH 4 -He, and CH 4 -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.",

author = "Tijs Karman and Gordon, \{Iouli E.\} and \{van der Avoird\}, Ad and Baranov, \{Yury I.\} and Christian Boulet and Drouin, \{Brian J.\} and Groenenboom, \{Gerrit C.\} and Magnus Gustafsson and Hartmann, \{Jean Michel\} and Kurucz, \{Robert L.\} and Rothman, \{Laurence S.\} and Kang Sun and Keeyoon Sung and Ryan Thalman and Ha Tran and Wishnow, \{Edward H.\} and Robin Wordsworth and Vigasin, \{Andrey A.\} and Rainer Volkamer and \{van der Zande\}, \{Wim J.\}",

note = "Publisher Copyright: {\textcopyright} 2019 Elsevier Inc.",

year = "2019",

month = aug,

doi = "10.1016/j.icarus.2019.02.034",

language = "English",

volume = "328",

pages = "160--175",

journal = "Icarus",

issn = "0019-1035",

publisher = "Academic Press Inc.",

}

Karman, T, Gordon, IE, van der Avoird, A, Baranov, YI, Boulet, C, Drouin, BJ, Groenenboom, GC, Gustafsson, M, Hartmann, JM, Kurucz, RL, Rothman, LS, Sun, K, Sung, K, Thalman, R, Tran, H, Wishnow, EH, Wordsworth, R, Vigasin, AA, Volkamer, R & van der Zande, WJ 2019, 'Update of the HITRAN collision-induced absorption section', Icarus, vol. 328, pp. 160-175. https://doi.org/10.1016/j.icarus.2019.02.034

TY - JOUR

T1 - Update of the HITRAN collision-induced absorption section

AU - Karman, Tijs

AU - Gordon, Iouli E.

AU - van der Avoird, Ad

AU - Baranov, Yury I.

AU - Boulet, Christian

AU - Drouin, Brian J.

AU - Groenenboom, Gerrit C.

AU - Gustafsson, Magnus

AU - Hartmann, Jean Michel

AU - Kurucz, Robert L.

AU - Rothman, Laurence S.

AU - Sun, Kang

AU - Sung, Keeyoon

AU - Thalman, Ryan

AU - Tran, Ha

AU - Wishnow, Edward H.

AU - Wordsworth, Robin

AU - Vigasin, Andrey A.

AU - Volkamer, Rainer

AU - van der Zande, Wim J.

PY - 2019/8

Y1 - 2019/8

N2 - 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 N 2 -N 2 , N 2 -H 2 , N 2 -CH 4 , N 2 -H 2 O, N 2 -O 2 , O 2 -O 2 , O 2 -CO 2 , CO 2 -CO 2 , H 2 -H 2 , H 2 -He, H 2 -CH 4 , H 2 -H, H-He, CH 4 -CH 4 , CH 4 -CO 2 , CH 4 -He, and CH 4 -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.

AB - 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 N 2 -N 2 , N 2 -H 2 , N 2 -CH 4 , N 2 -H 2 O, N 2 -O 2 , O 2 -O 2 , O 2 -CO 2 , CO 2 -CO 2 , H 2 -H 2 , H 2 -He, H 2 -CH 4 , H 2 -H, H-He, CH 4 -CH 4 , CH 4 -CO 2 , CH 4 -He, and CH 4 -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.

UR - https://www.scopus.com/pages/publications/85063527773

U2 - 10.1016/j.icarus.2019.02.034

DO - 10.1016/j.icarus.2019.02.034

M3 - Article

AN - SCOPUS:85063527773

SN - 0019-1035

VL - 328

SP - 160

EP - 175

JO - Icarus

JF - Icarus

ER -

Update of the HITRAN collision-induced absorption section

Abstract

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