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1、The HITRAN2012 molecular spectroscopic database L.S. Rothman a,n, I.E. Gordona, Y. Babikovb, A. Barbec, D. Chris Bennerd, P.F. Bernath e, M. Birkf, L. Bizzocchig, V. Boudonh, L.R. Browni, A. Camparguej, K. Chance a, E.A. Coheni, L.H. Coudertk, V.M. Devid, B.J. Drouini, A. Faytl, J.-M. Flaud k, R.R.
2、Gamachem, J.J. Harrisonn, J.-M. Hartmannk, C. Hillo, J.T. Hodges p, D. Jacquemartq, A. Jollyk, J. Lamourouxk,m, R.J. Le Royr, G. Lia, D.A. Long p, O.M. Lyulinb, C.J. Mackiea,1, S.T. Massies, S. Mikhailenkob, H.S.P. Mller t, O.V. Naumenkob, A.V. Nikitinb, J. Orphalu, V. Perevalovb, A. Perrin k, E.R.
3、Polovtsevab, C. Richarda, M.A.H. Smithv, E. Starikovab, K. Sungi, S. Tashkun b, J. Tennysono, G.C. Tooni, Vl.G. Tyuterevc, G. Wagnerf aHarvard-Smithsonian Center for Astrophysics, Atomic and Molecular Physics Division, Cambridge, MA 02138, USA bV.E. Zuev Institute of Atmospheric Optics SB RAS, Tomsk
4、 634021, Russia cUniversit de Reims-Champagne-Ardenne, Groupe de Spectromtrie Molculaire et Atmosphrique, 51062 Reims, France dThe College of William and Mary, Department of Physics, Williamsburg, VA 23187, USA eOld Dominion University, Department of Chemistry and Biochemistry, Norfolk, VA 23529, US
5、A fDLR, Remote Sensing Technology Institute, Wessling 82234, Germany gCAAUL, Observatrio Astronmico de Lisboa, Lisboa, Portugal hLaboratoire Interdisciplinaire Carnot de Bourgogne, UMR 6303 CNRS-Universit de Bourgogne, 21078 Dijon, France iJet Propulsion Laboratory, California Institute of Technolog
6、y, Pasadena, CA 91109, USA jUniversit Grenoble 1/CNRS, UMR5588 LIPhy, 38402 Grenoble, France kCNRS et Universits Paris Est et Paris 7, Laboratoire Inter-Universitaire des Systmes Atmosphriques, 94010 Crteil, France lUniversit Catholique de Louvain, Lab. de Spectroscopie Molculaire, 1348 Louvain-la-N
7、euve, Belgium mUniversity of Mass Lowell, Department of Environmental Earth and Atmospheric Sciences, Lowell, MA 01854, USA nUniversity of York, Department of Chemistry, York YO10 5DD, UK oUniversity College London, Department of Physics and Astronomy, London WC1E 6BT, UK pNational Institute of Stan
8、dards and Technology, Gaithersburg, MD 20899, USA qUPMC Univ. Paris 06, UMR 7075, Laboratoire de Dynamique, Interactions et Ractivit, 75252 Paris, France rUniversity of Waterloo, Department of Chemistry, Waterloo, Ont N2L 3G1, Canada sNational Center for Atmospheric Research, Boulder, CO 80307, USA
9、tUniversitt zu Kln, I. Physikalisches Institut, Cologne 50937, Germany uKarlsruhe Institute of Technology, Institute for Meteorology and Climate Research, Eggenstein-Leopoldshafen 76344, Germany vNASA Langley Research Center, Science Directorate, Hampton, VA 23681, USA a r t i c l e i n f o Article
10、history: Received 6 April 2013 Received in revised form 2 July 2013 Accepted 4 July 2013 Available online 12 July 2013 Keywords: HITRAN Spectroscopic database a b s t r a c t This paper describes the status of the 2012 edition of the HITRAN molecular spectroscopic compilation. The new edition replac
11、es the previous HITRAN edition of 2008 and its updates during the intervening years. The HITRAN molecular absorption compilation is comprised of six major components structured into folders that are freely accessible on the internet. These folders consist of the traditional line-by-line spectroscopi
12、c 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, ultraviolet spectroscopic parameters, aerosol indices of refraction, collision-induced absorption data, Contents lists avail
13、able at ScienceDirect journal homepage: Journal of Quantitative Spectroscopy fax: +1 617 496 7519. E-mail addresses: LSR_JQSRT, LRothmancfa.harvard.edu (L.S. Rothman). 1 Current address: University of Western Ontario, Department of Physics and Astronomy London, Ont., Canada N6A 3K7. Journal of Quant
14、itative Spectroscopy (2) infrared absorp- tion cross-sections (generally representing absorption by molecules that have very dense spectra or many low-lying vibrational modes); (3) ultraviolet datasets (both line-by-line and cross-section); (4) tables of aerosol refractive indices; (5) collision-ind
15、uced absorption datasets; and (6) global data and software for filtering and managing the data. The updates to these six portions of HITRAN will be discussed in the following sections. The data that enter HITRAN or replace previous entries go through a rigorous process. Fig. 1 is a schematic of the
16、general process. The vertical box on the left (source box) is a representation of the many sources that come to the attention of the HITRAN committee. This committee is formed of an international group of spectroscopists with expertise that cover all the molecules and spectral regions encompassed by HITRAN. Sources selected (which can include measurements or calculations of line positions, intensities, line-shape parameters, etc.) are then cast into the format of the HITRAN line list, or cross-
