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The HITRAN2024 molecular spectroscopic database

  • I. E. Gordon
  • , L. S. Rothman
  • , R. J. Hargreaves
  • , F. M. Gomez
  • , T. Bertin
  • , C. Hill
  • , R. V. Kochanov
  • , Y. Tan
  • , P. Wcisło
  • , V. Yu Makhnev
  • , P. F. Bernath
  • , M. Birk
  • , V. Boudon
  • , A. Campargue
  • , A. Coustenis
  • , B. J. Drouin
  • , R. R. Gamache
  • , J. T. Hodges
  • , D. Jacquemart
  • , E. J. Mlawer
  • A. V. Nikitin, V. I. Perevalov, M. Rotger, S. Robert, J. Tennyson, G. C. Toon, H. Tran, V. G. Tyuterev, E. M. Adkins, A. Barbe, D. M. Bailey, K. Bielska, L. Bizzocchi, T. A. Blake, C. A. Bowesman, P. Cacciani, P. Čermák, A. G. Császár, L. Denis, S. C. Egbert, O. Egorov, A. Yu Ermilov, A. J. Fleisher, H. Fleurbaey, A. Foltynowicz, T. Furtenbacher, M. Germann, E. R. Guest, J. J. Harrison, J. M. Hartmann, A. Hjältén, S. M. Hu, X. Huang, T. J. Johnson, H. Jóźwiak, S. Kassi, M. V. Khan, F. Kwabia-Tchana, T. J. Lee, D. Lisak, A. W. Liu, O. M. Lyulin, N. A. Malarich, L. Manceron, A. A. Marinina, S. T. Massie, J. Mascio, E. S. Medvedev, V. V. Meshkov, G. Ch Mellau, M. Melosso, S. N. Mikhailenko, D. Mondelain, H. S.P. Müller, M. O’Donnell, A. Owens, A. Perrin, O. L. Polyansky, P. L. Raston, Z. D. Reed, M. Rey, C. Richard, G. B. Rieker, C. Röske, S. W. Sharpe, E. Starikova, N. Stolarczyk, A. V. Stolyarov, K. Sung, F. Tamassia, J. Terragni, V. G. Ushakov, S. Vasilchenko, B. Vispoel, K. L. Vodopyanov, G. Wagner, S. Wójtewicz, S. N. Yurchenko, N. F. Zobov
  • Center for Astrophysics | Harvard & Smithsonian
  • International Atomic Energy Agency, Vienna International Centre
  • Russian Academy of Sciences
  • University of Science and Technology of China
  • Nicolaus Copernicus University
  • Old Dominion University
  • DLR
  • Centre de Recherches de Climatologie, CNRS UMR 5210, Université de Bourgogne
  • Laboratoire Interdisciplinaire de Physique
  • Université PSL
  • California Institute of Technology
  • University of Massachusetts-Lowell
  • National Institute of Standards and Technology
  • Sorbonne Université
  • Atmospheric and Environmental Research, Inc.
  • Technion - Israel Institute of Technology
  • UFR Des Sciences
  • Belgian Institute for Space Aeronomy
  • University College London
  • Tomsk State University
  • University of Bologna
  • Pacific Northwest National Laboratory
  • UMR 8523–PhLAM–Physique des Lasers Atomes et Molécules
  • Comenius University
  • Eötvös Loránd University
  • Institute of Life, Earth and Environment
  • University of Colorado Boulder
  • Moscow State University
  • Umeå University
  • European Organization for Nuclear Research
  • Natural Environment Research Council
  • University of Leicester
  • SETI Institute
  • NASA Ames Research Center
  • CNRS
  • Synchrotron SOLEIL
  • Russian Academy of Sciences
  • Justus-Liebig-Universität Giessen
  • Germany; University of Cologne
  • Bates College
  • Institute of Applied Physics of the Russian Academy of Sciences
  • University of Hawaii
  • The University of Adelaide
  • NASA Goddard Space Flight Center
  • University of Central Florida

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Résumé

The HITRAN database is a curated compilation of validated molecular spectroscopic parameters, established in the early 1970s. It 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 six major components. These components include the line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, experimentally derived 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. Responding to community requests, HITRAN2024 also incorporates — for the first time — a water-vapor continuum model. This paper describes the details of the choices of data and their compilation for the 2024 quadrennial edition of HITRAN. The HITRAN2024 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 2020 (including various updates during the intervening years). The extent of the updates of the line-by-line section in the HITRAN2024 edition ranges from updating a few lines of specific molecules/isotopologues to complete replacements of the lists, and also the introduction of additional isotopologues and six new (to HITRAN) molecules: H3+, CH3, S2, COFCl, HONO, ClNO2. Many new vibrational bands were added, extending the spectral coverage and completeness of the line lists. In addition, the accuracy of the parameters for major atmospheric absorbers has been increased substantially, often bringing the uncertainties down to unprecedented levels below 0.1%. The HITRAN2024 edition is available through www.hitran.org as well as the HITRAN Application Programming Interface (HAPI). The functionality of the tools to work with the HITRAN data has been extended for the new edition.

langue originaleAnglais
Numéro d'article109807
journalJournal of Quantitative Spectroscopy and Radiative Transfer
Volume353
Les DOIs
étatPublié - 1 avr. 2026

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