The HITRAN 2004 molecular spectroscopic database

被引:2457
作者
Rothman, LS
Jacquemart, D
Barbe, A
Benner, DC
Birk, M
Brown, LR
Carleer, MR
Chackerian, C
Chance, K
Coudert, LH
Dana, V
Devi, VM
Flaud, JM
Gamache, RR
Goldman, A
Hartmann, JM
Jucks, KW
Maki, AG
Mandin, JY
Massie, ST
Orphal, J
Perrin, A
Rinsland, CP
Smith, MAH
Tennyson, J
Tolchenov, RN
Toth, RA
Vander Auwera, J
Varanasi, P
Wagner, G
机构
[1] Harvard Smithsonian Ctr Astrophys, Atom & Mol Phys Div, Cambridge, MA 02138 USA
[2] Univ Reims, Grp Spectrometrie Mol & Atmospher, F-51062 Reims, France
[3] Coll William & Mary, Dept Phys, Williamsburg, VA 23187 USA
[4] DLR, Remote Sensing Technol Inst, Wessling, Germany
[5] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[6] Free Univ Brussels, Serv Chim Quant & Photophys, B-1050 Brussels, Belgium
[7] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[8] Univ Paris 11, Photophys Mol Lab, F-91405 Orsay, France
[9] Univ Paris 06, Lab Phys Mol & Applicat, F-75252 Paris, France
[10] Univ Mass Lowell, Dept Environm Earth & Atmospher Sci, Lowell, MA 01854 USA
[11] Univ Denver, Dept Phys, Denver, CO 80208 USA
[12] Harvard Smithsonian Ctr Astrophys, Opt & Infrared Astron Div, Cambridge, MA 02138 USA
[13] Natl Ctr Atmospher Res, Boulder, CO 80307 USA
[14] NASA, Langley Res Ctr, Hampton, VA 23681 USA
[15] UCL, Dept Phys & Astron, London WC1E 6BT, England
[16] SUNY Stony Brook, Stony Brook, NY 11794 USA
基金
英国自然环境研究理事会;
关键词
HITRAN; spectroscopic database; molecular spectroscopy; molecular absorption; line parameters; absorption cross-sections; aerosols;
D O I
10.1016/j.jqsrt.2004.10.008
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
This paper describes the status of the 2004 edition of the HITRAN molecular spectroscopic database. The HITRAN compilation consists of several components that serve as input for radiative transfer calculation codes: individual line parameters for the microwave through visible spectra of molecules in the gas phase; absorption cross-sections for molecules having dense spectral features, i.e., spectra in which the individual lines are unresolvable; individual line parameters and absorption cross-sections for bands in the ultra-violet; refractive indices of aerosols; tables and files of general properties associated with the database; and database management software. The line-by-line portion of the database contains spectroscopic parameters for 39 molecules including many of their isotopologues. The format of the section of the database on individual line parameters of HITRAN has undergone the most extensive enhancement in almost two decades. It now lists the Einstein A-coefficients, statistical weights of the upper and lower levels of the transitions, a better system for the representation of quantum identifications, and enhanced referencing and uncertainty codes. In addition, there is a provision for making corrections to the broadening of line transitions due to line mixing. (C) 2005 Elsevier Ltd. All rights reserved.
引用
收藏
页码:139 / 204
页数:66
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