The HITRAN2020 molecular spectroscopic database

被引：1264

作者：

Gordon, I. E. ^{[1
]}

Rothman, L. S. ^{[1
]}

Hargreaves, R. J. ^{[1
]}

Hashemi, R. ^{[1
]}

Karlovets, E., V ^{[1
]}

Skinner, F. M. ^{[1
]}

Conway, E. K. ^{[1
]}

Hill, C. ^{[2
]}

Kochanov, R., V ^{[1
,3
,4
]}

Tan, Y. ^{[1
,5
]}

Wcislo, P. ^{[6
]}

Finenko, A. A. ^{[1
,7
]}

Nelson, K. ^{[1
]}

Bernath, P. F. ^{[8
]}

Birk, M. ^{[9
]}

Boudon, V ^{[10
]}

Campargue, A. ^{[11
]}

Chance, K., V ^{[1
]}

Coustenis, A. ^{[12
]}

Drouin, B. J. ^{[13
]}

Flaud, J-M ^{[19
]}

Gamache, R. R. ^{[15
]}

Hodges, J. T. ^{[16
]}

Jacquemart, D. ^{[17
]}

Mlawer, E. J. ^{[18
]}

Nikitin, A., V ^{[3
]}

Perevalov, V., I ^{[3
]}

Rotger, M. ^{[20
]}

Tennyson, J. ^{[21
]}

Toon, G. C. ^{[13
]}

Tran, H. ^{[12
]}

Tyuterev, V. G. ^{[3
,4
,20
]}

Adkins, E. M. ^{[16
]}

Baker, A. ^{[14
]}

Barbe, A. ^{[20
]}

Cane, E. ^{[23
]}

Csaszar, A. G. ^{[25
,26
]}

Dudaryonok, A. ^{[3
]}

Egorov, O. ^{[3
]}

Fleisher, A. J. ^{[16
]}

Fleurbaey, H. ^{[11
]}

Foltynowicz, A. ^{[27
]}

Furtenbacher, T. ^{[25
]}

Harrison, J. J. ^{[28
,29
,30
]}

Hartmann, J-M ^{[22
]}

Horneman, V-M ^{[31
]}

Huang, X. ^{[32
]}

Karman, T. ^{[1
]}

Karns, J. ^{[1
,50
,51
]}

Kassi, S. ^{[11
]}

机构：

[1] Ctr Astrophys Harvard & Smithsonian, Atom & Mol Phys Div, Cambridge, MA 02138 USA

[2] IAEA, Nucl Data Sect, Vienna Int Ctr, POB 100, A-1400 Vienna, Austria

[3] Russian Acad Sci, VE Zuev Inst Atmospher Opt, Lab Theoret Spect, Tomsk 634055, Russia

[4] Tomsk State Univ, QUAMER Lab, Tomsk 634050, Russia

[5] Univ Sci & Technol China, Hefei Natl Lab Phys Sci Microscale, Hefei, Peoples R China

[6] Nicolaus Copernicus Univ Torun, Fac Phys Astron & Informat, Inst Phys, Grudziadzka 5, PL-87100 Torun, Poland

[7] Lomonosov Moscow State Univ, Dept Chem, Moscow 119991, Russia

[8] Old Dominion Univ, Dept Chem, Norfolk, VA USA

[9] German Aerosp Ctr DLR, Remote Sensing Technol Inst, Wessling, Germany

[10] Univ Bourgogne Franche Comte, Lab Interdisciplinaire Carnot Bourgogne, UMR 6303 CNRS, Dijon, France

[11] Univ Grenoble Alpes, LIPhy, CNRS, F-38000 Grenoble, France

[12] Sorbonne Univ, PSL Univ, Paris Observ,CNRS, Lab Etud Spatiales & Instrumentat Astrophys, Paris, France

[13] CALTECH, Jet Prop Lab, Pasadena, CA USA

[14] CALTECH, Div Astron, Pasadena, CA 91125 USA

[15] Univ Massachusetts, Dept Environm Earth & Atmospher Sci, Lowell, MA USA

[16] NIST, Chem Sci Div, Gaithersburg, MD USA

[17] Sorbonne Univ, CNRS, MONARIS, MOl NAnoobjets Reactivite Interact & Spect, F-75005 Paris, France

[18] Atmospher & Environm Res, Lexington, MA USA

[19] Univ Paris Sud, Univ Paris Saclay, Inst Sci Mol Orsay, CNRS, F-91405 Orsay, France

[20] UMR CNRS 7331, Grp Spectrometrie Mol & Atmospher, BP 1039, F-51687 Reims 2, France

[21] UCL, Dept Phys & Astron, London WC1E 6BT, England

[22] Sorbonne Univ, PSL Res Univ, Lab Meteorol Dynam IPSL, Ecole Normale Super,CNRS,Ecole Polytech, F-91120 Palaiseau, France

[23] Univ Bologna, Dipartimento Chim Ind Toso Montanari, Viale Risorgimento 4, I-40136 Bologna, Italy

[24] Univ Bologna, Dipartimento Chim Giacomo Ciamician, Via F Selmi 2, I-40126 Bologna, Italy

[25] MTA ELTE Complex Chem Syst Res Grp, Budapest, Hungary

[26] Eotvos Lorand Univ, Inst Chem, Budapest, Hungary

[27] Umea Univ, Dept Phys, S-90187 Umea, Sweden

[28] Univ Leicester, Dept Phys & Astron, Leicester, Leics, England

[29] Univ Leicester, Natl Ctr Earth Observat, Leicester, Leics, England

[30] Univ Leicester, Leicester Inst Space & Earth Observat, Leicester, Leics, England

[31] Univ Oulu, Dept Phys, DIN-90014 Oulu, Finland

[32] SETI Inst, Mountain View, CA 94043 USA

[33] NASA, Planetary Syst Branch, Space Sci & Astrobiol Div, Ames Res Ctr, Moffett Field, CA 94035 USA

[34] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80309 USA

[35] Univ Cologne, Phys Inst 1, D-50937 Cologne, Germany

[36] James Madison Univ, Dept Chem & Biochem, Harrisonburg, VA 22807 USA

[37] Univ Adelaide, Dept Chem, Adelaide, SA 5005, Australia

[38] Sorbonne Univ, PSL Res Univ, Lab Meteorol Dynam IPSL, Ecole Polytech,CNRS,Ecole Normale Super, F-75005 Paris, France

[39] Univ Paris, F-75013 Paris, France

[40] Univ Paris Est Creteil, CNRS, LISA, F-75013 Paris, France

[41] Russian Acad Sci, Inst Appl Phys, Nizhnii Novgorod, Russia

[42] Leibniz Inst Plasma Sci & Technol INP, Greifswald, Germany

[43] Univ Libre Bruxelles, Spect Quantum Chem & Atmospher Remote Sensing SQU, CP 160-09, B-1050 Brussels, Belgium

[44] Russian Acad Sci, Obenglandhov Inst Atmospher Phys, Pyzhevsky Per 3, Moscow 119017, Russia

[45] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[46] Univ Namur UNamur, Inst Life Earth & Environm ILEE, Res Unit Lasers & Spect LLS, B-5000 Namur, Belgium

[47] Royal Belgian Inst Space Aeron BIRA IASB, B-1180 Brussels, Belgium

[48] Deutsch Elektronen Synchrotron DESY, Ctr Free Electron Laser Sci, Notkestr 85, D-22607 Hamburg, Germany

[49] Univ Hamburg, Hamburg Ctr Ultrafast Imaging, Luruper Chaussee 149, D-22761 Hamburg, Germany

[50] Rochester Inst Technol, Golisano Coll Comp & Informat Sci, Rochester, NY 14623 USA

来源：

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 2022年 / 277卷

基金：

欧洲研究理事会; 英国自然环境研究理事会; 俄罗斯科学基金会;

关键词：

HITRAN; Spectroscopic database; Molecular spectroscopy; Spectroscopic line parameters; Absorption cross-sections; Collision-induced absorption; Aerosols; Molecular opacities; ABSORPTION CROSS-SECTIONS; COLLISION-INDUCED ABSORPTION; HIGH-RESOLUTION ANALYSIS; LINE-SHAPE PARAMETERS; SENSITIVITY CAVITY RING; COMPLEX REFRACTIVE-INDEXES; MU-M REGION; INCLUDING TEMPERATURE DEPENDENCES; POTENTIAL-ENERGY SURFACE; VAPOR SELF-CONTINUUM;

D O I：

10.1016/j.jqsrt.2021.107949

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

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. (C) 2021 The Author(s). Published by Elsevier Ltd.

引用

页数：82

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