% IMPORTANT: The following is UTF-8 encoded. This means that in the presence % of non-ASCII characters, it will not work with BibTeX 0.99 or older. % Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or % “biber”. @ARTICLE{Gordon:456234, author = {Gordon, Iouli and Rothman, Laurence S and Hargreaves, Robert and Hashemi, Robab and Karlovets, Ekaterina and Skinner, Frances and Conway, Eamon and Hill, Christian and Kochanov, Roman and Tan, Yan and Wcislo, Piotr and Finenko, Artem and Nelson, Kyle and Bernath, Peter and Birk, Manfred and Boudon, Vincent and Campargue, Alain and Chance, Kelly and Coustenis, Athena and Drouin, Brian and Flaud, Jean-Marie and Gamache, Robert R and Hodges, Joseph and Jacquemart, David and Mlawer, Eli and Nikitin, Andrey and Perevalov, Valery and Rotger, Maud and Tennyson, Jonathan and Toon, Geoofrey and Tran, Ha and Tyuterev, Vladimir and Adkins, Erin and Baker, Ashley and Barbe, Alain and Cané, Elisabetta and Császár, Attila and Egorov, Oleg and Fleisher, Adam and Fleurbaey, Helene and Foltynowicz, Aleksandra and Furtenbacher, Tibor and Harrison, Jeremy and Hartmann, Jean-Michel and Horneman, Veli-Matti and Huang, Xinchuan and Karman, Tijs and Karns, Joshua and Kassi, Samir and Kleiner, Isabelle and Kofman, Vincent and Kwabia, Fridolin and Lee, Timothy and Long, David and Lukashevskaya, Anastasia and Schwenke, David and Lyulin, Oleg and Makhnev, Vladimir and Matt, Wyatt and Massie, Steven and Melosso, Mattia and Mikhailenko, Semen and Mondelain, Didier and Muller, Holger and Naumenko, Olga and Perrin, Agnes and Polyansky, Oleg and Raddaoui, emna and Raston, Paul and Reed, Zachary and Rey, Michael and Richard, Cyril and Tobias, Roland and Sadiek, Ibrahim and Starikova, Evgenia and Sung, Keeyoon and Tamassia, Filippo and Tashkun, Sergey and Auwera, Jean Vander and Vasilenko, Irina and Vigasin, Andrey and Villanueva, Geronimo and Vispoel, Bastien and Wagner, Georg and Yachmenev, Andrey and Yurchenko, Sergey}, title = {{T}he {HITRAN}2020 molecular spectroscopic database}, journal = {Journal of quantitative spectroscopy $\&$ radiative transfer}, volume = {277}, issn = {0022-4073}, address = {New York, NY [u.a.]}, publisher = {Elsevier}, reportid = {PUBDB-2021-01416}, pages = {107949}, year = {2021}, abstract = {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, CH$_3$F, GeH$_4$, CS$_2$, CH$_3$I and NF. 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.}, cin = {FS-CFEL-CMI}, ddc = {530}, cid = {I:(DE-H253)FS-CFEL-CMI-20220405}, pnm = {631 - Matter – Dynamics, Mechanisms and Control (POF4-631)}, pid = {G:(DE-HGF)POF4-631}, experiment = {EXP:(DE-MLZ)NOSPEC-20140101}, typ = {PUB:(DE-HGF)16}, UT = {WOS:000744248200001}, doi = {10.1016/j.jqsrt.2021.107949}, url = {https://bib-pubdb1.desy.de/record/456234}, }