The HITRAN2020 molecular spectroscopic database

I. E. Gordon; L. S. Rothman; R.J.  Hargreaves; R. Hashemi; E.V. Karlovets; F.M. Skinner; E.K. Conway; C. Hill; R.V.  Kochanov; Y. Tan; Piotr Wcislo; A.A. Finenko; K. Nelson; P.F. Bernath; M. Birk; Vincent Boudon; A. Campargue; K.V. Chance; A. Coustenis; B.J. Drouin; Jean-Marie Flaud; Robert Gamache; J.T. Hodges; D. Jacquemart; E.J. Mlawer; Andrei Nikitin; Valery I. Perevalov; M. Rotger; Jonathan Tennyson; G.C. Toon; Ha Tran; Vladimir G. Tyuterev; E.M. Adkins; A. Baker; Alain Barbe; E. Canè; Attila G. Császár; A. Dudaryonok; Oleg Egorov; A.J. Fleisher; M. Fleurbaey; A. Foltynowicz; T. Furtenbacher; J.J. Harrison; J.M. Hartmann; V. M. Horneman; X. Huang; T. Karman; J. Karns; S. Kassi; I. Kleiner; V. Kofman; F. Kwabia–Tchana; N.N. Lavrentieva; T.J. Lee; D.A. Long; A.A. Lukashevskaya; O.M. Lyulin; V.Yu Makhnev; W. Matt; S.T. Massie; M. Melosso; S.N. Mikhailenko; Didier Mondelain; H.S.P. Müller; O.V. Naumenko; A. Perrin; Oleg L. Polyansky; E. Raddaoui; P.L. Raston; Z.D. Reed; Michaël Rey; C. Richard; R. Tóbiás; I. Sadiek; D.W. Schwenke; E. Starikova; K. Sung; F. Tamassia; Sergei A. Tashkun; Jean Vander Auwera; I.A. Vasilenko; A.A. Vigasin; G.L. Villanueva; Bastien Vispoel; G. Wagner; A. Yachmenev; Sergei N. Yurchenko

doi:10.1016/j.jqsrt.2021.107949

The HITRAN2020 molecular spectroscopic database

I. E. Gordon, L. S. Rothman, R.J. Hargreaves, R. Hashemi, E.V. Karlovets, F.M. Skinner, E.K. Conway, C. Hill, R.V. Kochanov, Y. Tan, Piotr Wcislo, A.A. Finenko, K. Nelson, P.F. Bernath, M. Birk, Vincent Boudon, A. Campargue, K.V. Chance, A. Coustenis, B.J. DrouinJean-Marie Flaud, Robert Gamache, J.T. Hodges, D. Jacquemart, E.J. Mlawer, Andrei Nikitin, Valery I. Perevalov, M. Rotger, Jonathan Tennyson, G.C. Toon, Ha Tran, Vladimir G. Tyuterev, E.M. Adkins, A. Baker, Alain Barbe, E. Canè, Attila G. Császár, A. Dudaryonok, Oleg Egorov, A.J. Fleisher, M. Fleurbaey, A. Foltynowicz, T. Furtenbacher, J.J. Harrison, J.M. Hartmann, V. M. Horneman, X. Huang, T. Karman, J. Karns, S. Kassi, I. Kleiner, V. Kofman, F. Kwabia–Tchana, N.N. Lavrentieva, T.J. Lee, D.A. Long, A.A. Lukashevskaya, O.M. Lyulin, V.Yu Makhnev, W. Matt, S.T. Massie, M. Melosso, S.N. Mikhailenko, Didier Mondelain, H.S.P. Müller, O.V. Naumenko, A. Perrin, Oleg L. Polyansky, E. Raddaoui, P.L. Raston, Z.D. Reed, Michaël Rey, C. Richard, R. Tóbiás, I. Sadiek, D.W. Schwenke, E. Starikova, K. Sung, F. Tamassia, Sergei A. Tashkun, Jean Vander Auwera, I.A. Vasilenko, A.A. Vigasin, G.L. Villanueva, Bastien Vispoel, G. Wagner, A. Yachmenev, Sergei N. Yurchenko

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Abstract

The HITRAN database is a compilation of molecular spectroscopic parameters. It was established in the early 1970s and is used by various computer codes to predict and simulate the transmission and emission of light in gaseous media (with an emphasis on terrestrial and planetary atmospheres). The HITRAN compilation is composed of five major components: the line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, experimental infrared absorption cross-sections (for molecules where it is not yet feasible for representation in a line-by-line form), collision-induced absorption data, aerosol indices of refraction, and general tables (including partition sums) that apply globally to the data. This paper describes the contents of the 2020 quadrennial edition of HITRAN. The HITRAN2020 edition takes advantage of recent experimental and theoretical data that were meticulously validated, in particular, against laboratory and atmospheric spectra. The new edition replaces the previous HITRAN edition of 2016 (including its updates during the intervening years).
All five components of HITRAN have undergone major updates. In particular, the extent of the updates in the HITRAN2020 edition range from updating a few lines of specific molecules to complete replacements of the lists, and also the introduction of additional isotopologues and new (to HITRAN) molecules: SO, CH3F, GeH4, CS2, CH3I and NF3. Many new vibrational bands were added, extending the spectral coverage and completeness of the line lists. Also, the accuracy of the parameters for major atmospheric absorbers has been increased substantially, often featuring sub-percent uncertainties. Broadening parameters associated with the ambient pressure of water vapor were introduced to HITRAN for the first time and are now available for several molecules.
The HITRAN2020 edition continues to take advantage of the relational structure and efficient interface available at www.hitran.org and the HITRAN Application Programming Interface (HAPI). The functionality of both tools has been extended for the new edition.

Original language	English
Article number	107949
Journal	Journal of Quantitative Spectroscopy and Radiative Transfer
Volume	277
DOIs	https://doi.org/10.1016/j.jqsrt.2021.107949
Publication status	Published - Jan 2022

Keywords

Absorption cross-sections
Aerosols
Collision-induced absorption
HITRAN
Molecular opacities
Molecular spectroscopy
Spectroscopic database
Spectroscopic line parameters

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10.1016/j.jqsrt.2021.107949

VispoelB_article_2022Final published version, 13 MBLicence: CC BY

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Gordon, I. E., Rothman, L. S., Hargreaves, R. J., Hashemi, R., Karlovets, E. V., Skinner, F. M., Conway, E. K., Hill, C., Kochanov, R. V., Tan, Y., Wcislo, P., Finenko, A. A., Nelson, K., Bernath, P. F., Birk, M., Boudon, V., Campargue, A., Chance, K. V., Coustenis, A., ... Yurchenko, S. N. (2022). The HITRAN2020 molecular spectroscopic database. Journal of Quantitative Spectroscopy and Radiative Transfer, 277, Article 107949. https://doi.org/10.1016/j.jqsrt.2021.107949

@article{f917877dab5348b89a0921b40f4dd293,

title = "The HITRAN2020 molecular spectroscopic database",

abstract = "The HITRAN database is a compilation of molecular spectroscopic parameters. It was established in the early 1970s and is used by various computer codes to predict and simulate the transmission and emission of light in gaseous media (with an emphasis on terrestrial and planetary atmospheres). The HITRAN compilation is composed of five major components: the line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, experimental infrared absorption cross-sections (for molecules where it is not yet feasible for representation in a line-by-line form), collision-induced absorption data, aerosol indices of refraction, and general tables (including partition sums) that apply globally to the data. This paper describes the contents of the 2020 quadrennial edition of HITRAN. The HITRAN2020 edition takes advantage of recent experimental and theoretical data that were meticulously validated, in particular, against laboratory and atmospheric spectra. The new edition replaces the previous HITRAN edition of 2016 (including its updates during the intervening years).All five components of HITRAN have undergone major updates. In particular, the extent of the updates in the HITRAN2020 edition range from updating a few lines of specific molecules to complete replacements of the lists, and also the introduction of additional isotopologues and new (to HITRAN) molecules: SO, CH3F, GeH4, CS2, CH3I and NF3. Many new vibrational bands were added, extending the spectral coverage and completeness of the line lists. Also, the accuracy of the parameters for major atmospheric absorbers has been increased substantially, often featuring sub-percent uncertainties. Broadening parameters associated with the ambient pressure of water vapor were introduced to HITRAN for the first time and are now available for several molecules.The HITRAN2020 edition continues to take advantage of the relational structure and efficient interface available at www.hitran.org and the HITRAN Application Programming Interface (HAPI). The functionality of both tools has been extended for the new edition.",

keywords = "Absorption cross-sections, Aerosols, Collision-induced absorption, HITRAN, Molecular opacities, Molecular spectroscopy, Spectroscopic database, Spectroscopic line parameters",

author = "Gordon, {I. E.} and Rothman, {L. S.} and R.J. Hargreaves and R. Hashemi and E.V. Karlovets and F.M. Skinner and E.K. Conway and C. Hill and R.V. Kochanov and Y. Tan and Piotr Wcislo and A.A. Finenko and K. Nelson and P.F. Bernath and M. Birk and Vincent Boudon and A. Campargue and K.V. Chance and A. Coustenis and B.J. Drouin and Jean-Marie Flaud and Robert Gamache and J.T. Hodges and D. Jacquemart and E.J. Mlawer and Andrei Nikitin and Perevalov, {Valery I.} and M. Rotger and Jonathan Tennyson and G.C. Toon and Ha Tran and Tyuterev, {Vladimir G.} and E.M. Adkins and A. Baker and Alain Barbe and E. Can{\`e} and Cs{\'a}sz{\'a}r, {Attila G.} and A. Dudaryonok and Oleg Egorov and A.J. Fleisher and M. Fleurbaey and A. Foltynowicz and T. Furtenbacher and J.J. Harrison and J.M. Hartmann and Horneman, {V. M.} and X. Huang and T. Karman and J. Karns and S. Kassi and I. Kleiner and V. Kofman and F. Kwabia–Tchana and N.N. Lavrentieva and T.J. Lee and D.A. Long and A.A. Lukashevskaya and O.M. Lyulin and V.Yu Makhnev and W. Matt and S.T. Massie and M. Melosso and S.N. Mikhailenko and Didier Mondelain and H.S.P. M{\"u}ller and O.V. Naumenko and A. Perrin and Polyansky, {Oleg L.} and E. Raddaoui and P.L. Raston and Z.D. Reed and Micha{\"e}l Rey and C. Richard and R. T{\'o}bi{\'a}s and I. Sadiek and D.W. Schwenke and E. Starikova and K. Sung and F. Tamassia and Tashkun, {Sergei A.} and {Vander Auwera}, Jean and I.A. Vasilenko and A.A. Vigasin and G.L. Villanueva and Bastien Vispoel and G. Wagner and A. Yachmenev and Yurchenko, {Sergei N.}",

note = "Funding Information: Development of the HITRAN2020 database and associated tools was supported through the NASA grants NNX17AI78G, NNX16AG51G, 80NSSC20K0962, 80NSSC20K1059. Funding Information: Portions of the research described in this paper were performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. The research from the V.E. Zuev Institute of Atmospheric Optics of Siberian Branch of Russian Academy of Sciences were supported by the Ministry of Science and Higher Education of the Russian Federation. The work of the Tomsk group on ozone spectroscopy was supported by the Russian Science Foundation RNF grant no. 19-12-00171. GSMA Reims and LiPhy Grenoble acknowledge support from the French-Russian collaboration program LIA CNRS “SAMIA”. AGC, TF, and RT received support from the ELTE Institutional Excellence Program (TKP2020-IKA-05) and from NKFIH (K119658). OLP and JT received support from the UK Natural Environment Research Council under grants NE/N001508/1 and the European Research Council under ERC Advanced Investigator grant 8838302 Publisher Copyright: {\textcopyright} 2021 The Author(s)",

year = "2022",

month = jan,

doi = "10.1016/j.jqsrt.2021.107949",

language = "English",

volume = "277",

journal = "Journal of Quantitative Spectroscopy and Radiative Transfer",

issn = "0022-4073",

publisher = "Elsevier",

}

Gordon, IE, Rothman, LS, Hargreaves, RJ, Hashemi, R, Karlovets, EV, Skinner, FM, Conway, EK, Hill, C, Kochanov, RV, Tan, Y, Wcislo, P, Finenko, AA, Nelson, K, Bernath, PF, Birk, M, Boudon, V, Campargue, A, Chance, KV, Coustenis, A, Drouin, BJ, Flaud, J-M, Gamache, R, Hodges, JT, Jacquemart, D, Mlawer, EJ, Nikitin, A, Perevalov, VI, Rotger, M, Tennyson, J, Toon, GC, Tran, H, Tyuterev, VG, Adkins, EM, Baker, A, Barbe, A, Canè, E, Császár, AG, Dudaryonok, A, Egorov, O, Fleisher, AJ, Fleurbaey, M, Foltynowicz, A, Furtenbacher, T, Harrison, JJ, Hartmann, JM, Horneman, VM, Huang, X, Karman, T, Karns, J, Kassi, S, Kleiner, I, Kofman, V, Kwabia–Tchana, F, Lavrentieva, NN, Lee, TJ, Long, DA, Lukashevskaya, AA, Lyulin, OM, Makhnev, VY, Matt, W, Massie, ST, Melosso, M, Mikhailenko, SN, Mondelain, D, Müller, HSP, Naumenko, OV, Perrin, A, Polyansky, OL, Raddaoui, E, Raston, PL, Reed, ZD, Rey, M, Richard, C, Tóbiás, R, Sadiek, I, Schwenke, DW, Starikova, E, Sung, K, Tamassia, F, Tashkun, SA, Vander Auwera, J, Vasilenko, IA, Vigasin, AA, Villanueva, GL, Vispoel, B, Wagner, G, Yachmenev, A & Yurchenko, SN 2022, 'The HITRAN2020 molecular spectroscopic database', Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 277, 107949. https://doi.org/10.1016/j.jqsrt.2021.107949

TY - JOUR

T1 - The HITRAN2020 molecular spectroscopic database

AU - Gordon, I. E.

AU - Rothman, L. S.

AU - Hargreaves, R.J.

AU - Hashemi, R.

AU - Karlovets, E.V.

AU - Skinner, F.M.

AU - Conway, E.K.

AU - Hill, C.

AU - Kochanov, R.V.

AU - Tan, Y.

AU - Wcislo, Piotr

AU - Finenko, A.A.

AU - Nelson, K.

AU - Bernath, P.F.

AU - Birk, M.

AU - Boudon, Vincent

AU - Campargue, A.

AU - Chance, K.V.

AU - Coustenis, A.

AU - Drouin, B.J.

AU - Flaud, Jean-Marie

AU - Gamache, Robert

AU - Hodges, J.T.

AU - Jacquemart, D.

AU - Mlawer, E.J.

AU - Nikitin, Andrei

AU - Perevalov, Valery I.

AU - Rotger, M.

AU - Tennyson, Jonathan

AU - Toon, G.C.

AU - Tran, Ha

AU - Tyuterev, Vladimir G.

AU - Adkins, E.M.

AU - Baker, A.

AU - Barbe, Alain

AU - Canè, E.

AU - Császár, Attila G.

AU - Dudaryonok, A.

AU - Egorov, Oleg

AU - Fleisher, A.J.

AU - Fleurbaey, M.

AU - Foltynowicz, A.

AU - Furtenbacher, T.

AU - Harrison, J.J.

AU - Hartmann, J.M.

AU - Horneman, V. M.

AU - Huang, X.

AU - Karman, T.

AU - Karns, J.

AU - Kassi, S.

AU - Kleiner, I.

AU - Kofman, V.

AU - Kwabia–Tchana, F.

AU - Lavrentieva, N.N.

AU - Lee, T.J.

AU - Long, D.A.

AU - Lukashevskaya, A.A.

AU - Lyulin, O.M.

AU - Makhnev, V.Yu

AU - Matt, W.

AU - Massie, S.T.

AU - Melosso, M.

AU - Mikhailenko, S.N.

AU - Mondelain, Didier

AU - Müller, H.S.P.

AU - Naumenko, O.V.

AU - Perrin, A.

AU - Polyansky, Oleg L.

AU - Raddaoui, E.

AU - Raston, P.L.

AU - Reed, Z.D.

AU - Rey, Michaël

AU - Richard, C.

AU - Tóbiás, R.

AU - Sadiek, I.

AU - Schwenke, D.W.

AU - Starikova, E.

AU - Sung, K.

AU - Tamassia, F.

AU - Tashkun, Sergei A.

AU - Vander Auwera, Jean

AU - Vasilenko, I.A.

AU - Vigasin, A.A.

AU - Villanueva, G.L.

AU - Vispoel, Bastien

AU - Wagner, G.

AU - Yachmenev, A.

AU - Yurchenko, Sergei N.

N1 - Funding Information: Development of the HITRAN2020 database and associated tools was supported through the NASA grants NNX17AI78G, NNX16AG51G, 80NSSC20K0962, 80NSSC20K1059. Funding Information: Portions of the research described in this paper were performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. The research from the V.E. Zuev Institute of Atmospheric Optics of Siberian Branch of Russian Academy of Sciences were supported by the Ministry of Science and Higher Education of the Russian Federation. The work of the Tomsk group on ozone spectroscopy was supported by the Russian Science Foundation RNF grant no. 19-12-00171. GSMA Reims and LiPhy Grenoble acknowledge support from the French-Russian collaboration program LIA CNRS “SAMIA”. AGC, TF, and RT received support from the ELTE Institutional Excellence Program (TKP2020-IKA-05) and from NKFIH (K119658). OLP and JT received support from the UK Natural Environment Research Council under grants NE/N001508/1 and the European Research Council under ERC Advanced Investigator grant 8838302 Publisher Copyright: © 2021 The Author(s)

PY - 2022/1

Y1 - 2022/1

N2 - The HITRAN database is a compilation of molecular spectroscopic parameters. It was established in the early 1970s and is used by various computer codes to predict and simulate the transmission and emission of light in gaseous media (with an emphasis on terrestrial and planetary atmospheres). The HITRAN compilation is composed of five major components: the line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, experimental infrared absorption cross-sections (for molecules where it is not yet feasible for representation in a line-by-line form), collision-induced absorption data, aerosol indices of refraction, and general tables (including partition sums) that apply globally to the data. This paper describes the contents of the 2020 quadrennial edition of HITRAN. The HITRAN2020 edition takes advantage of recent experimental and theoretical data that were meticulously validated, in particular, against laboratory and atmospheric spectra. The new edition replaces the previous HITRAN edition of 2016 (including its updates during the intervening years).All five components of HITRAN have undergone major updates. In particular, the extent of the updates in the HITRAN2020 edition range from updating a few lines of specific molecules to complete replacements of the lists, and also the introduction of additional isotopologues and new (to HITRAN) molecules: SO, CH3F, GeH4, CS2, CH3I and NF3. Many new vibrational bands were added, extending the spectral coverage and completeness of the line lists. Also, the accuracy of the parameters for major atmospheric absorbers has been increased substantially, often featuring sub-percent uncertainties. Broadening parameters associated with the ambient pressure of water vapor were introduced to HITRAN for the first time and are now available for several molecules.The HITRAN2020 edition continues to take advantage of the relational structure and efficient interface available at www.hitran.org and the HITRAN Application Programming Interface (HAPI). The functionality of both tools has been extended for the new edition.

AB - The HITRAN database is a compilation of molecular spectroscopic parameters. It was established in the early 1970s and is used by various computer codes to predict and simulate the transmission and emission of light in gaseous media (with an emphasis on terrestrial and planetary atmospheres). The HITRAN compilation is composed of five major components: the line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, experimental infrared absorption cross-sections (for molecules where it is not yet feasible for representation in a line-by-line form), collision-induced absorption data, aerosol indices of refraction, and general tables (including partition sums) that apply globally to the data. This paper describes the contents of the 2020 quadrennial edition of HITRAN. The HITRAN2020 edition takes advantage of recent experimental and theoretical data that were meticulously validated, in particular, against laboratory and atmospheric spectra. The new edition replaces the previous HITRAN edition of 2016 (including its updates during the intervening years).All five components of HITRAN have undergone major updates. In particular, the extent of the updates in the HITRAN2020 edition range from updating a few lines of specific molecules to complete replacements of the lists, and also the introduction of additional isotopologues and new (to HITRAN) molecules: SO, CH3F, GeH4, CS2, CH3I and NF3. Many new vibrational bands were added, extending the spectral coverage and completeness of the line lists. Also, the accuracy of the parameters for major atmospheric absorbers has been increased substantially, often featuring sub-percent uncertainties. Broadening parameters associated with the ambient pressure of water vapor were introduced to HITRAN for the first time and are now available for several molecules.The HITRAN2020 edition continues to take advantage of the relational structure and efficient interface available at www.hitran.org and the HITRAN Application Programming Interface (HAPI). The functionality of both tools has been extended for the new edition.

KW - Absorption cross-sections

KW - Aerosols

KW - Collision-induced absorption

KW - HITRAN

KW - Molecular opacities

KW - Molecular spectroscopy

KW - Spectroscopic database

KW - Spectroscopic line parameters

UR - http://www.scopus.com/inward/record.url?scp=85118584595&partnerID=8YFLogxK

U2 - 10.1016/j.jqsrt.2021.107949

DO - 10.1016/j.jqsrt.2021.107949

M3 - Article

SN - 0022-4073

VL - 277

JO - Journal of Quantitative Spectroscopy and Radiative Transfer

JF - Journal of Quantitative Spectroscopy and Radiative Transfer

M1 - 107949

ER -

The HITRAN2020 molecular spectroscopic database

Abstract

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Experimental and theoretical study of line shape parameters and their temperature dependence for infrared absorption lines of molecules with atmospheric interest

Optics, Lasers and spectroscopy

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The HITRAN2020 molecular spectroscopic database

Abstract

Keywords

Access to Document

Other files and links

Fingerprint

Projects

Experimental and theoretical study of line shape parameters and their temperature dependence for infrared absorption lines of molecules with atmospheric interest

Equipment

Optics, Lasers and spectroscopy

Cite this