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Laser spectroscopic study of ozone in the 100←000 band for the SWIFT instrument
A complete spectroscopic study of 15 strong ozone lines in the 1132.5–1134.5 cm −1 spectral range has been undertaken in the framework of the development of the stratospheric wind interferometer for transport studies (SWIFT), led by the Canadian Space Agency. Measurements have been performed with an...
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| Published in: | Journal of quantitative spectroscopy & radiative transfer 2010-05, Vol.111 (7), p.961-972 |
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| Main Authors: | , , , |
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| cited_by | cdi_FETCH-LOGICAL-c370t-712d4a5fc3487aa693bfa1c90df1e5d7c7dc86b7915d089ac5d6893335e957523 |
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| cites | cdi_FETCH-LOGICAL-c370t-712d4a5fc3487aa693bfa1c90df1e5d7c7dc86b7915d089ac5d6893335e957523 |
| container_end_page | 972 |
| container_issue | 7 |
| container_start_page | 961 |
| container_title | Journal of quantitative spectroscopy & radiative transfer |
| container_volume | 111 |
| creator | Guinet, M. Mondelain, D. Janssen, C. Camy-Peyret, C. |
| description | A complete spectroscopic study of 15 strong ozone lines in the 1132.5–1134.5
cm
−1 spectral range has been undertaken in the framework of the development of the stratospheric wind interferometer for transport studies (SWIFT), led by the Canadian Space Agency. Measurements have been performed with an interferometrically stabilized tunable diode laser spectrometer. Absolute line positions and intensities have been determined with high accuracy (4×10
−5
cm
−1 and 1–2% respectively). Self- and air-broadening coefficients at 296
K have been obtained with an accuracy of 1%. The air-shifting coefficient and its temperature dependence have also been measured for unblended lines together with the temperature dependence of the air-broadening. Line intensities have been calibrated by simultaneously performed UV absorption measurements at 253.7
nm. Our IR/UV comparison supports a previously reported inconsistency between recommended IR intensities (HITRAN08) and UV absorption cross-sections and indicates that current IR intensities are too small by ∼3%. |
| doi_str_mv | 10.1016/j.jqsrt.2010.01.011 |
| format | article |
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cm
−1 spectral range has been undertaken in the framework of the development of the stratospheric wind interferometer for transport studies (SWIFT), led by the Canadian Space Agency. Measurements have been performed with an interferometrically stabilized tunable diode laser spectrometer. Absolute line positions and intensities have been determined with high accuracy (4×10
−5
cm
−1 and 1–2% respectively). Self- and air-broadening coefficients at 296
K have been obtained with an accuracy of 1%. The air-shifting coefficient and its temperature dependence have also been measured for unblended lines together with the temperature dependence of the air-broadening. Line intensities have been calibrated by simultaneously performed UV absorption measurements at 253.7
nm. Our IR/UV comparison supports a previously reported inconsistency between recommended IR intensities (HITRAN08) and UV absorption cross-sections and indicates that current IR intensities are too small by ∼3%.</description><identifier>ISSN: 0022-4073</identifier><identifier>EISSN: 1879-1352</identifier><identifier>DOI: 10.1016/j.jqsrt.2010.01.011</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><subject>Band spectra ; Calibration ; Cross sections ; Diode laser ; Infrared ; Infrared radiation ; Line parameter ; Optics ; Ozone ; Physics ; Spectroscopic analysis ; Spectroscopy ; Temperature dependence ; Ultraviolet</subject><ispartof>Journal of quantitative spectroscopy & radiative transfer, 2010-05, Vol.111 (7), p.961-972</ispartof><rights>2010 Elsevier Ltd</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c370t-712d4a5fc3487aa693bfa1c90df1e5d7c7dc86b7915d089ac5d6893335e957523</citedby><cites>FETCH-LOGICAL-c370t-712d4a5fc3487aa693bfa1c90df1e5d7c7dc86b7915d089ac5d6893335e957523</cites><orcidid>0000-0001-7896-9741</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://hal.science/hal-00997598$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Guinet, M.</creatorcontrib><creatorcontrib>Mondelain, D.</creatorcontrib><creatorcontrib>Janssen, C.</creatorcontrib><creatorcontrib>Camy-Peyret, C.</creatorcontrib><title>Laser spectroscopic study of ozone in the 100←000 band for the SWIFT instrument</title><title>Journal of quantitative spectroscopy & radiative transfer</title><description>A complete spectroscopic study of 15 strong ozone lines in the 1132.5–1134.5
cm
−1 spectral range has been undertaken in the framework of the development of the stratospheric wind interferometer for transport studies (SWIFT), led by the Canadian Space Agency. Measurements have been performed with an interferometrically stabilized tunable diode laser spectrometer. Absolute line positions and intensities have been determined with high accuracy (4×10
−5
cm
−1 and 1–2% respectively). Self- and air-broadening coefficients at 296
K have been obtained with an accuracy of 1%. The air-shifting coefficient and its temperature dependence have also been measured for unblended lines together with the temperature dependence of the air-broadening. Line intensities have been calibrated by simultaneously performed UV absorption measurements at 253.7
nm. Our IR/UV comparison supports a previously reported inconsistency between recommended IR intensities (HITRAN08) and UV absorption cross-sections and indicates that current IR intensities are too small by ∼3%.</description><subject>Band spectra</subject><subject>Calibration</subject><subject>Cross sections</subject><subject>Diode laser</subject><subject>Infrared</subject><subject>Infrared radiation</subject><subject>Line parameter</subject><subject>Optics</subject><subject>Ozone</subject><subject>Physics</subject><subject>Spectroscopic analysis</subject><subject>Spectroscopy</subject><subject>Temperature dependence</subject><subject>Ultraviolet</subject><issn>0022-4073</issn><issn>1879-1352</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNp9kMtKAzEUhoMoWC9P4CZLXUw9Z9JMJgsXpXiDgoiKy5AmGUxpJzWZCvUBXPuMPokZKy6FA4Gf7z9JPkJOEIYIWJ3Ph_PXFLthCTkBzIM7ZIC1kAUyXu6SAUBZFiMQbJ8cpDQHAMawGpD7qU4u0rRyposhmbDyhqZubTc0NDS8h9ZR39LuxVEE-Pr4zE06062lTYg_8cPz7dVjZlIX10vXdkdkr9GL5I5_z0PydHX5OLkppnfXt5PxtDBMQFcILO1I88awUS20riSbNRqNBNug41YYYU1dzYREbqGW2nBb1ZIxxp3kgpfskJxt977ohVpFv9Rxo4L26mY8VX0GIKXgsn7DzJ5u2VUMr2uXOrX0ybjFQrcurJPCKj-nZFDxjLItarKOFF3ztxtB9bLVXP3IVr1sBZinv-Bi23L5x2_eRZWMd61x1sdsVtng_-1_A31fh4k</recordid><startdate>20100501</startdate><enddate>20100501</enddate><creator>Guinet, M.</creator><creator>Mondelain, D.</creator><creator>Janssen, C.</creator><creator>Camy-Peyret, C.</creator><general>Elsevier Ltd</general><general>Elsevier</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7SR</scope><scope>7U5</scope><scope>8BQ</scope><scope>8FD</scope><scope>JG9</scope><scope>L7M</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0001-7896-9741</orcidid></search><sort><creationdate>20100501</creationdate><title>Laser spectroscopic study of ozone in the 100←000 band for the SWIFT instrument</title><author>Guinet, M. ; Mondelain, D. ; Janssen, C. ; Camy-Peyret, C.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c370t-712d4a5fc3487aa693bfa1c90df1e5d7c7dc86b7915d089ac5d6893335e957523</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Band spectra</topic><topic>Calibration</topic><topic>Cross sections</topic><topic>Diode laser</topic><topic>Infrared</topic><topic>Infrared radiation</topic><topic>Line parameter</topic><topic>Optics</topic><topic>Ozone</topic><topic>Physics</topic><topic>Spectroscopic analysis</topic><topic>Spectroscopy</topic><topic>Temperature dependence</topic><topic>Ultraviolet</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Guinet, M.</creatorcontrib><creatorcontrib>Mondelain, D.</creatorcontrib><creatorcontrib>Janssen, C.</creatorcontrib><creatorcontrib>Camy-Peyret, C.</creatorcontrib><collection>CrossRef</collection><collection>Engineered Materials Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>Materials Research Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Journal of quantitative spectroscopy & radiative transfer</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Guinet, M.</au><au>Mondelain, D.</au><au>Janssen, C.</au><au>Camy-Peyret, C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Laser spectroscopic study of ozone in the 100←000 band for the SWIFT instrument</atitle><jtitle>Journal of quantitative spectroscopy & radiative transfer</jtitle><date>2010-05-01</date><risdate>2010</risdate><volume>111</volume><issue>7</issue><spage>961</spage><epage>972</epage><pages>961-972</pages><issn>0022-4073</issn><eissn>1879-1352</eissn><abstract>A complete spectroscopic study of 15 strong ozone lines in the 1132.5–1134.5
cm
−1 spectral range has been undertaken in the framework of the development of the stratospheric wind interferometer for transport studies (SWIFT), led by the Canadian Space Agency. Measurements have been performed with an interferometrically stabilized tunable diode laser spectrometer. Absolute line positions and intensities have been determined with high accuracy (4×10
−5
cm
−1 and 1–2% respectively). Self- and air-broadening coefficients at 296
K have been obtained with an accuracy of 1%. The air-shifting coefficient and its temperature dependence have also been measured for unblended lines together with the temperature dependence of the air-broadening. Line intensities have been calibrated by simultaneously performed UV absorption measurements at 253.7
nm. Our IR/UV comparison supports a previously reported inconsistency between recommended IR intensities (HITRAN08) and UV absorption cross-sections and indicates that current IR intensities are too small by ∼3%.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/j.jqsrt.2010.01.011</doi><tpages>12</tpages><orcidid>https://orcid.org/0000-0001-7896-9741</orcidid></addata></record> |
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| ispartof | Journal of quantitative spectroscopy & radiative transfer, 2010-05, Vol.111 (7), p.961-972 |
| issn | 0022-4073 1879-1352 |
| language | eng |
| recordid | cdi_hal_primary_oai_HAL_hal_00997598v1 |
| source | ScienceDirect Freedom Collection 2022-2024 |
| subjects | Band spectra Calibration Cross sections Diode laser Infrared Infrared radiation Line parameter Optics Ozone Physics Spectroscopic analysis Spectroscopy Temperature dependence Ultraviolet |
| title | Laser spectroscopic study of ozone in the 100←000 band for the SWIFT instrument |
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