The HITRAN2016 molecular spectroscopic database
•HITRAN2016 molecular spectroscopic database is described.•Dynamic web interface at www.hitran.org is introduced.•HITRAN Application Programming Interface is introduced.•Substantial extent of the amount and quality of the data highlighted.•Many new spectroscopic parameters are now available in HITRA...
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| Veröffentlicht in: | Journal of quantitative spectroscopy & radiative transfer 2017-12, Vol.203, p.3-69 |
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| creator | Gordon, I.E. Rothman, L.S. Hill, C. Kochanov, R.V. Tan, Y. Bernath, P.F. Birk, M. Boudon, V. Campargue, A. Chance, K.V. Drouin, B.J. Flaud, J.-M. Gamache, R.R. Hodges, J.T. Jacquemart, D. Perevalov, V.I. Perrin, A. Shine, K.P. Smith, M.-A.H. Tennyson, J. Toon, G.C. Tran, H. Tyuterev, V.G. Barbe, A. Császár, A.G. Devi, V.M. Furtenbacher, T. Harrison, J.J. Hartmann, J.-M. Jolly, A. Johnson, T.J. Karman, T. Kleiner, I. Kyuberis, A.A. Loos, J. Lyulin, O.M. Massie, S.T. Mikhailenko, S.N. Moazzen-Ahmadi, N. Müller, H.S.P. Naumenko, O.V. Nikitin, A.V. Polyansky, O.L. Rey, M. Rotger, M. Sharpe, S.W. Sung, K. Starikova, E. Tashkun, S.A. Auwera, J. Vander Wagner, G. Wilzewski, J. Wcisło, P. Yu, S. Zak, E.J. |
| description | •HITRAN2016 molecular spectroscopic database is described.•Dynamic web interface at www.hitran.org is introduced.•HITRAN Application Programming Interface is introduced.•Substantial extent of the amount and quality of the data highlighted.•Many new spectroscopic parameters are now available in HITRAN.
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. |
| doi_str_mv | 10.1016/j.jqsrt.2017.06.038 |
| format | Article |
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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.</description><identifier>ISSN: 0022-4073</identifier><identifier>EISSN: 1879-1352</identifier><identifier>DOI: 10.1016/j.jqsrt.2017.06.038</identifier><language>eng</language><publisher>2230 Support: Elsevier Ltd</publisher><subject>Absorption cross-sections ; Aerosols ; Atmospheric and Oceanic Physics ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; Collision-induced Absorption ; HITRAN ; Instrumentation and Detectors ; Molecular absorption ; Molecular spectroscopy ; Optics ; Physics ; Spectroscopic database ; Spectroscopic line parameters</subject><ispartof>Journal of quantitative spectroscopy & radiative transfer, 2017-12, Vol.203, p.3-69</ispartof><rights>2017</rights><rights>Copyright Determination: MAY_INCLUDE_COPYRIGHT_MATERIAL</rights><rights>Attribution</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c430t-e1253b17f2477898779e436f3b023259a3f0632ae3d3e26c882b34ba45116a143</citedby><cites>FETCH-LOGICAL-c430t-e1253b17f2477898779e436f3b023259a3f0632ae3d3e26c882b34ba45116a143</cites><orcidid>0000-0002-7339-7577 ; 0000-0002-1574-9597 ; 0000-0002-8030-7410 ; 0000-0002-2472-7998 ; 0000-0001-5165-5099 ; 0000-0001-9846-9816 ; 0000-0002-2181-1158 ; 0000-0001-7493-0719 ; 0000-0003-1644-7555 ; 0000-0002-4280-4096 ; 0000-0001-5015-6538 ; 0000-0002-9587-9884 ; 0000-0001-5287-2888</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0022407317301073$$EHTML$$P50$$Gelsevier$$Hfree_for_read</linktohtml><link.rule.ids>230,314,776,780,796,881,3537,27901,27902,65534</link.rule.ids><backlink>$$Uhttps://hal.science/hal-01765945$$DView record in HAL$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/servlets/purl/1368409$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Gordon, I.E.</creatorcontrib><creatorcontrib>Rothman, L.S.</creatorcontrib><creatorcontrib>Hill, C.</creatorcontrib><creatorcontrib>Kochanov, R.V.</creatorcontrib><creatorcontrib>Tan, Y.</creatorcontrib><creatorcontrib>Bernath, P.F.</creatorcontrib><creatorcontrib>Birk, M.</creatorcontrib><creatorcontrib>Boudon, V.</creatorcontrib><creatorcontrib>Campargue, A.</creatorcontrib><creatorcontrib>Chance, K.V.</creatorcontrib><creatorcontrib>Drouin, B.J.</creatorcontrib><creatorcontrib>Flaud, J.-M.</creatorcontrib><creatorcontrib>Gamache, R.R.</creatorcontrib><creatorcontrib>Hodges, J.T.</creatorcontrib><creatorcontrib>Jacquemart, D.</creatorcontrib><creatorcontrib>Perevalov, V.I.</creatorcontrib><creatorcontrib>Perrin, A.</creatorcontrib><creatorcontrib>Shine, K.P.</creatorcontrib><creatorcontrib>Smith, M.-A.H.</creatorcontrib><creatorcontrib>Tennyson, J.</creatorcontrib><creatorcontrib>Toon, G.C.</creatorcontrib><creatorcontrib>Tran, H.</creatorcontrib><creatorcontrib>Tyuterev, V.G.</creatorcontrib><creatorcontrib>Barbe, A.</creatorcontrib><creatorcontrib>Császár, A.G.</creatorcontrib><creatorcontrib>Devi, V.M.</creatorcontrib><creatorcontrib>Furtenbacher, T.</creatorcontrib><creatorcontrib>Harrison, J.J.</creatorcontrib><creatorcontrib>Hartmann, J.-M.</creatorcontrib><creatorcontrib>Jolly, A.</creatorcontrib><creatorcontrib>Johnson, T.J.</creatorcontrib><creatorcontrib>Karman, T.</creatorcontrib><creatorcontrib>Kleiner, I.</creatorcontrib><creatorcontrib>Kyuberis, A.A.</creatorcontrib><creatorcontrib>Loos, J.</creatorcontrib><creatorcontrib>Lyulin, O.M.</creatorcontrib><creatorcontrib>Massie, S.T.</creatorcontrib><creatorcontrib>Mikhailenko, S.N.</creatorcontrib><creatorcontrib>Moazzen-Ahmadi, N.</creatorcontrib><creatorcontrib>Müller, H.S.P.</creatorcontrib><creatorcontrib>Naumenko, O.V.</creatorcontrib><creatorcontrib>Nikitin, A.V.</creatorcontrib><creatorcontrib>Polyansky, O.L.</creatorcontrib><creatorcontrib>Rey, M.</creatorcontrib><creatorcontrib>Rotger, M.</creatorcontrib><creatorcontrib>Sharpe, S.W.</creatorcontrib><creatorcontrib>Sung, K.</creatorcontrib><creatorcontrib>Starikova, E.</creatorcontrib><creatorcontrib>Tashkun, S.A.</creatorcontrib><creatorcontrib>Auwera, J. Vander</creatorcontrib><creatorcontrib>Wagner, G.</creatorcontrib><creatorcontrib>Wilzewski, J.</creatorcontrib><creatorcontrib>Wcisło, P.</creatorcontrib><creatorcontrib>Yu, S.</creatorcontrib><creatorcontrib>Zak, E.J.</creatorcontrib><creatorcontrib>Pacific Northwest National Lab. (PNNL), Richland, WA (United States)</creatorcontrib><title>The HITRAN2016 molecular spectroscopic database</title><title>Journal of quantitative spectroscopy & radiative transfer</title><description>•HITRAN2016 molecular spectroscopic database is described.•Dynamic web interface at www.hitran.org is introduced.•HITRAN Application Programming Interface is introduced.•Substantial extent of the amount and quality of the data highlighted.•Many new spectroscopic parameters are now available in HITRAN.
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.</description><subject>Absorption cross-sections</subject><subject>Aerosols</subject><subject>Atmospheric and Oceanic Physics</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>Collision-induced Absorption</subject><subject>HITRAN</subject><subject>Instrumentation and Detectors</subject><subject>Molecular absorption</subject><subject>Molecular spectroscopy</subject><subject>Optics</subject><subject>Physics</subject><subject>Spectroscopic database</subject><subject>Spectroscopic line parameters</subject><issn>0022-4073</issn><issn>1879-1352</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNp9kEFLxDAQhYMouK7-Aj0Ubx7anWTStD14WBZ1hUVB1nNI05RN6bZrUhf896ZWPHoamPfe8OYj5JpCQoGKRZM0H94NCQOaJSASwPyEzGieFTHFlJ2SGQBjMYcMz8mF9w0AIFIxI4vtzkTr5-3b8iWERbTvW6M_W-UifzB6cL3X_cHqqFKDKpU3l-SsVq03V79zTt4fH7ardbx5fXpeLTex5ghDbChLsaRZzXiW5UWeZYXhKGosgSFLC4U1CGTKYIWGCZ3nrEReKp5SKhTlOCe3093eD1Z6bQejd7rvulBKUhQ5hyKY7ibTTrXy4OxeuS_ZKyvXy40cdwGHSAueHmnw4uTV4SfvTP0XoCBHiLKRPxDlCFGCkAFiSN1MqU55JbvB-SAzDPgopGmQ7yfZBBRHa9zY1HTaVNaNRave_nv-G1q_f9Y</recordid><startdate>20171201</startdate><enddate>20171201</enddate><creator>Gordon, I.E.</creator><creator>Rothman, L.S.</creator><creator>Hill, C.</creator><creator>Kochanov, R.V.</creator><creator>Tan, Y.</creator><creator>Bernath, P.F.</creator><creator>Birk, M.</creator><creator>Boudon, V.</creator><creator>Campargue, A.</creator><creator>Chance, K.V.</creator><creator>Drouin, B.J.</creator><creator>Flaud, J.-M.</creator><creator>Gamache, R.R.</creator><creator>Hodges, J.T.</creator><creator>Jacquemart, D.</creator><creator>Perevalov, V.I.</creator><creator>Perrin, A.</creator><creator>Shine, K.P.</creator><creator>Smith, M.-A.H.</creator><creator>Tennyson, J.</creator><creator>Toon, G.C.</creator><creator>Tran, H.</creator><creator>Tyuterev, V.G.</creator><creator>Barbe, A.</creator><creator>Császár, A.G.</creator><creator>Devi, V.M.</creator><creator>Furtenbacher, T.</creator><creator>Harrison, J.J.</creator><creator>Hartmann, J.-M.</creator><creator>Jolly, A.</creator><creator>Johnson, T.J.</creator><creator>Karman, T.</creator><creator>Kleiner, I.</creator><creator>Kyuberis, A.A.</creator><creator>Loos, J.</creator><creator>Lyulin, O.M.</creator><creator>Massie, S.T.</creator><creator>Mikhailenko, S.N.</creator><creator>Moazzen-Ahmadi, N.</creator><creator>Müller, H.S.P.</creator><creator>Naumenko, O.V.</creator><creator>Nikitin, A.V.</creator><creator>Polyansky, O.L.</creator><creator>Rey, M.</creator><creator>Rotger, M.</creator><creator>Sharpe, S.W.</creator><creator>Sung, K.</creator><creator>Starikova, E.</creator><creator>Tashkun, S.A.</creator><creator>Auwera, J. 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Vander ; Wagner, G. ; Wilzewski, J. ; Wcisło, P. ; Yu, S. ; Zak, E.J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c430t-e1253b17f2477898779e436f3b023259a3f0632ae3d3e26c882b34ba45116a143</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Absorption cross-sections</topic><topic>Aerosols</topic><topic>Atmospheric and Oceanic Physics</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>Collision-induced Absorption</topic><topic>HITRAN</topic><topic>Instrumentation and Detectors</topic><topic>Molecular absorption</topic><topic>Molecular spectroscopy</topic><topic>Optics</topic><topic>Physics</topic><topic>Spectroscopic database</topic><topic>Spectroscopic line parameters</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gordon, I.E.</creatorcontrib><creatorcontrib>Rothman, L.S.</creatorcontrib><creatorcontrib>Hill, C.</creatorcontrib><creatorcontrib>Kochanov, R.V.</creatorcontrib><creatorcontrib>Tan, Y.</creatorcontrib><creatorcontrib>Bernath, P.F.</creatorcontrib><creatorcontrib>Birk, M.</creatorcontrib><creatorcontrib>Boudon, V.</creatorcontrib><creatorcontrib>Campargue, A.</creatorcontrib><creatorcontrib>Chance, K.V.</creatorcontrib><creatorcontrib>Drouin, B.J.</creatorcontrib><creatorcontrib>Flaud, J.-M.</creatorcontrib><creatorcontrib>Gamache, R.R.</creatorcontrib><creatorcontrib>Hodges, J.T.</creatorcontrib><creatorcontrib>Jacquemart, D.</creatorcontrib><creatorcontrib>Perevalov, V.I.</creatorcontrib><creatorcontrib>Perrin, A.</creatorcontrib><creatorcontrib>Shine, K.P.</creatorcontrib><creatorcontrib>Smith, M.-A.H.</creatorcontrib><creatorcontrib>Tennyson, J.</creatorcontrib><creatorcontrib>Toon, G.C.</creatorcontrib><creatorcontrib>Tran, H.</creatorcontrib><creatorcontrib>Tyuterev, V.G.</creatorcontrib><creatorcontrib>Barbe, A.</creatorcontrib><creatorcontrib>Császár, A.G.</creatorcontrib><creatorcontrib>Devi, V.M.</creatorcontrib><creatorcontrib>Furtenbacher, T.</creatorcontrib><creatorcontrib>Harrison, J.J.</creatorcontrib><creatorcontrib>Hartmann, J.-M.</creatorcontrib><creatorcontrib>Jolly, A.</creatorcontrib><creatorcontrib>Johnson, T.J.</creatorcontrib><creatorcontrib>Karman, T.</creatorcontrib><creatorcontrib>Kleiner, I.</creatorcontrib><creatorcontrib>Kyuberis, A.A.</creatorcontrib><creatorcontrib>Loos, J.</creatorcontrib><creatorcontrib>Lyulin, O.M.</creatorcontrib><creatorcontrib>Massie, S.T.</creatorcontrib><creatorcontrib>Mikhailenko, S.N.</creatorcontrib><creatorcontrib>Moazzen-Ahmadi, N.</creatorcontrib><creatorcontrib>Müller, H.S.P.</creatorcontrib><creatorcontrib>Naumenko, O.V.</creatorcontrib><creatorcontrib>Nikitin, A.V.</creatorcontrib><creatorcontrib>Polyansky, O.L.</creatorcontrib><creatorcontrib>Rey, M.</creatorcontrib><creatorcontrib>Rotger, M.</creatorcontrib><creatorcontrib>Sharpe, S.W.</creatorcontrib><creatorcontrib>Sung, K.</creatorcontrib><creatorcontrib>Starikova, E.</creatorcontrib><creatorcontrib>Tashkun, S.A.</creatorcontrib><creatorcontrib>Auwera, J. Vander</creatorcontrib><creatorcontrib>Wagner, G.</creatorcontrib><creatorcontrib>Wilzewski, J.</creatorcontrib><creatorcontrib>Wcisło, P.</creatorcontrib><creatorcontrib>Yu, S.</creatorcontrib><creatorcontrib>Zak, E.J.</creatorcontrib><creatorcontrib>Pacific Northwest National Lab. (PNNL), Richland, WA (United States)</creatorcontrib><collection>ScienceDirect Open Access Titles</collection><collection>Elsevier:ScienceDirect:Open Access</collection><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Journal of quantitative spectroscopy & radiative transfer</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gordon, I.E.</au><au>Rothman, L.S.</au><au>Hill, C.</au><au>Kochanov, R.V.</au><au>Tan, Y.</au><au>Bernath, P.F.</au><au>Birk, M.</au><au>Boudon, V.</au><au>Campargue, A.</au><au>Chance, K.V.</au><au>Drouin, B.J.</au><au>Flaud, J.-M.</au><au>Gamache, R.R.</au><au>Hodges, J.T.</au><au>Jacquemart, D.</au><au>Perevalov, V.I.</au><au>Perrin, A.</au><au>Shine, K.P.</au><au>Smith, M.-A.H.</au><au>Tennyson, J.</au><au>Toon, G.C.</au><au>Tran, H.</au><au>Tyuterev, V.G.</au><au>Barbe, A.</au><au>Császár, A.G.</au><au>Devi, V.M.</au><au>Furtenbacher, T.</au><au>Harrison, J.J.</au><au>Hartmann, J.-M.</au><au>Jolly, A.</au><au>Johnson, T.J.</au><au>Karman, T.</au><au>Kleiner, I.</au><au>Kyuberis, A.A.</au><au>Loos, J.</au><au>Lyulin, O.M.</au><au>Massie, S.T.</au><au>Mikhailenko, S.N.</au><au>Moazzen-Ahmadi, N.</au><au>Müller, H.S.P.</au><au>Naumenko, O.V.</au><au>Nikitin, A.V.</au><au>Polyansky, O.L.</au><au>Rey, M.</au><au>Rotger, M.</au><au>Sharpe, S.W.</au><au>Sung, K.</au><au>Starikova, E.</au><au>Tashkun, S.A.</au><au>Auwera, J. Vander</au><au>Wagner, G.</au><au>Wilzewski, J.</au><au>Wcisło, P.</au><au>Yu, S.</au><au>Zak, E.J.</au><aucorp>Pacific Northwest National Lab. (PNNL), Richland, WA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The HITRAN2016 molecular spectroscopic database</atitle><jtitle>Journal of quantitative spectroscopy & radiative transfer</jtitle><date>2017-12-01</date><risdate>2017</risdate><volume>203</volume><spage>3</spage><epage>69</epage><pages>3-69</pages><issn>0022-4073</issn><eissn>1879-1352</eissn><abstract>•HITRAN2016 molecular spectroscopic database is described.•Dynamic web interface at www.hitran.org is introduced.•HITRAN Application Programming Interface is introduced.•Substantial extent of the amount and quality of the data highlighted.•Many new spectroscopic parameters are now available in HITRAN.
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.</abstract><cop>2230 Support</cop><pub>Elsevier Ltd</pub><doi>10.1016/j.jqsrt.2017.06.038</doi><tpages>67</tpages><orcidid>https://orcid.org/0000-0002-7339-7577</orcidid><orcidid>https://orcid.org/0000-0002-1574-9597</orcidid><orcidid>https://orcid.org/0000-0002-8030-7410</orcidid><orcidid>https://orcid.org/0000-0002-2472-7998</orcidid><orcidid>https://orcid.org/0000-0001-5165-5099</orcidid><orcidid>https://orcid.org/0000-0001-9846-9816</orcidid><orcidid>https://orcid.org/0000-0002-2181-1158</orcidid><orcidid>https://orcid.org/0000-0001-7493-0719</orcidid><orcidid>https://orcid.org/0000-0003-1644-7555</orcidid><orcidid>https://orcid.org/0000-0002-4280-4096</orcidid><orcidid>https://orcid.org/0000-0001-5015-6538</orcidid><orcidid>https://orcid.org/0000-0002-9587-9884</orcidid><orcidid>https://orcid.org/0000-0001-5287-2888</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0022-4073 |
| ispartof | Journal of quantitative spectroscopy & radiative transfer, 2017-12, Vol.203, p.3-69 |
| issn | 0022-4073 1879-1352 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1368409 |
| source | Elsevier ScienceDirect Journals Complete; NASA Technical Reports Server |
| subjects | Absorption cross-sections Aerosols Atmospheric and Oceanic Physics CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS Collision-induced Absorption HITRAN Instrumentation and Detectors Molecular absorption Molecular spectroscopy Optics Physics Spectroscopic database Spectroscopic line parameters |
| title | The HITRAN2016 molecular spectroscopic database |
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