The HITRAN2016 molecular spectroscopic database

被引:2437
作者
Gordon, I. E. [1 ]
Rothman, L. S. [1 ]
Hill, C. [1 ,2 ]
Kochanov, R. V. [1 ,3 ]
Tan, Y.
Bernath, P. F. [4 ]
Birk, M. [5 ]
Boudon, V. [6 ]
Campargue, A. [7 ]
Chance, K. V. [1 ]
Drouin, B. J. [8 ]
Flaud, J. -M. [9 ]
Gamache, R. R. [10 ]
Hodges, J. T. [11 ]
Jacquemart, D. [12 ]
Perevalov, V. I. [13 ]
Perrin, A. [14 ]
Shine, K. P. [15 ]
Smith, M. -A. H. [16 ]
Tennyson, J.
Toon, G. C. [8 ]
Tran, H. [14 ]
Tyuterev, V. G. [17 ]
Barbe, A. [17 ]
Csaszar, A. G. [18 ,31 ]
Devi, V. M. [19 ]
Furtenbacher, T.
Harrison, J. J. [20 ,29 ,30 ]
Hartmann, J. -M.
Jolly, A. [9 ]
Johnson, T. J.
Karman, T. [22 ]
Kleiner, I. [9 ]
Kyuberis, A. A. [1 ,23 ]
Loos, J. [5 ]
Lyulin, O. M. [13 ]
Massie, S. T. [24 ]
Mikhailenko, S. N. [13 ]
Moazzen-Ahmadi, N. [25 ]
Mueller, H. S. P. [26 ]
Naumenko, O. V. [13 ]
Nikitin, A. V. [13 ]
Polyansky, O. L. [2 ,23 ]
Rey, M. [17 ]
Rotger, M. [17 ]
Sharpe, S. W. [21 ]
Sung, K. [7 ,8 ]
Starikova, E. [13 ]
Tashkun, S. A. [13 ]
Vander Auwera, J. [27 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, Atom & Mol Phys Div, Cambridge, MA 02138 USA
[2] UCL, Dept Phys & Astron, London WC1E 6BT, England
[3] Tomsk State Univ, Lab Quantum Mech Mol & Radiat Proc, Tomsk, Russia
[4] Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA USA
[5] DLR, Inst Remote Sensing Technol, Wessling, Germany
[6] Univ Bourgogne Franche Comte, Lab Interdisciplinaire Carnot Bourgogne, UMR 6303, CNRS, Dijon, France
[7] Univ Grenoble, Grenoble, France
[8] CALTECH, Jet Prop Lab, Pasadena, CA USA
[9] Univ Paris Est, LISA, Creteil, France
[10] Univ Massachusetts, Dept Environm Earth & Atmospher Sci, Lowell, MA USA
[11] NIST, Chem Sci Div, Gaithersburg, MD 20899 USA
[12] Univ Paris 06, LADIR, Paris, France
[13] Inst Atmospher Opt, Lab Theoret Spect, Tomsk, Russia
[14] Univ Paris Saclay, CNRS, Ecole Polytech, Lab Meteorol Dynam IPSL, F-91128 Palaiseau, France
[15] Univ Reading, Dept Meteorol, Reading, Berks, England
[16] NASA, Langley Res Ctr, Sci Directorate, Hampton, VA 23665 USA
[17] Univ Reims, GSMA, Reims, France
[18] MTA ELTE Complex Chem Syst Res Grp, Budapest, Hungary
[19] Coll William & Mary, Dept Phys, Williamsburg, VA 23185 USA
[20] Univ Leicester, Dept Phys & Astron, Leicester, Leics, England
[21] Battelle Pacific North West Natl Lab, Richland, WA USA
[22] Radboud Univ Nijmegen, Inst Mol & Mat, Nijmegen, Netherlands
[23] Russian Acad Sci, Inst Appl Phys, Nizhnii Novgorod, Russia
[24] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO USA
[25] Univ Calgary, Dept Phys & Astron, Calgary, AB, Canada
[26] Univ Cologne, Phys Inst 1, Cologne, Germany
[27] Univ Libre Bruxelles, Serv Chim Quant & Photophys, CP 160-09, B-1050 Brussels, Belgium
[28] Nicolaus Copernicus Univ, Inst Phys, Torun, Poland
[29] Univ Leicester, Natl Ctr Earth Observat, Leicester, Leics, England
[30] Univ Leicester, Leicester Inst Space & Earth Observat, Leicester, Leics, England
[31] Eotvos Lorand Univ, Inst Chem, Budapest, Hungary
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
HITRAN; Spectroscopic database; Molecular spectroscopy; Molecular absorption; Spectroscopic line parameters; Absorption cross-sections; Collision-induced absorption; Aerosols; ABSORPTION CROSS-SECTIONS; LINE-SHAPE PARAMETERS; GLOBAL WARMING POTENTIALS; M TRANSPARENCY WINDOW; TUNABLE DIODE-LASER; HIGH-RESOLUTION ANALYSIS; SENSITIVITY CAVITY RING; GAS-PHASE REACTIONS; INCLUDING TEMPERATURE DEPENDENCES; ROTATIONAL-VIBRATIONAL SPECTRA;
D O I
10.1016/j.jqsrt.2017.06.038
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
This paper describes the contents of the 2016 edition of the HITRAN molecular spectroscopic compilation. The new edition replaces the previous HITRAN edition of 2012 and its updates during the intervening years. The HITRAN molecular absorption compilation is composed of five major components: the traditional line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, infrared absorption cross-sections for molecules not yet amenable to representation in a line-by-line form, collision-induced absorption data, aerosol indices of refraction, and general tables such as partition sums that apply globally to the data. The new HITRAN is greatly extended in terms of accuracy, spectral coverage, additional absorption phenomena, added line-shape formalisms, and validity. Moreover, molecules, isotopologues, and perturbing gases have been added that address the issues of atmospheres beyond the Earth. Of considerable note, experimental IR cross-sections for almost 300 additional molecules important in different areas of atmospheric science have been added to the database. The compilation can be accessed through www.hitran.org. Most of the HITRAN data have now been cast into an underlying relational database structure that offers many advantages over the long-standing sequential text-based structure. The new structure empowers the user in many, ways. It enables the incorporation of an extended set of fundamental parameters per transition, sophisticated line-shape formalisms, easy user-defined output formats, and very convenient searching, filtering, and plotting of data. A powerful application programming interface making use of structured query language (SQL) features for higher-level applications of HITRAN is also provided. Published by Elsevier Ltd.
引用
收藏
页码:3 / 69
页数:67
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