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On the rate coefficient of the N(2D)+O2→NO+O reaction in the terrestrial thermosphere
The temperature dependence of the rate coefficient of the N(2D)+O2→NO+O reaction has been determined using ab initio potential energy surfaces (PES) and classical dynamics. The calculation agrees with the recommended rate coefficient at 300 K (∼110 km altitude). The rate coefficient is given by the...
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Published in: | Geophysical research letters 2003-03, Vol.30 (5), p.63.1-n/a |
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creator | Duff, J. W. Dothe, H. Sharma, R. D. |
description | The temperature dependence of the rate coefficient of the N(2D)+O2→NO+O reaction has been determined using ab initio potential energy surfaces (PES) and classical dynamics. The calculation agrees with the recommended rate coefficient at 300 K (∼110 km altitude). The rate coefficient is given by the expression k(T) = 6.2 × 10−12(T/300) cm3/s/molec. In contrast to the nearly temperature‐independent value of this rate coefficient previously recommended, the value given here increases by almost a factor of about four as the altitude increases from 110 to 200 km. It is also shown that even though N(2D) atoms in the thermosphere are produced with large translational energies, using the value of the rate coefficient at the local temperature introduces negligible error in the amount of NO produced. The new value of this rate coefficient will significantly increase the amount of NO computed in the aeronomic models causing a re‐evaluation of the heat budget and temperature and density structure of the thermosphere. In particular, implications of the larger rate coefficient for the recent observations of dramatically enhanced 5.3 μm emission from NO in the thermosphere due to solar storms are discussed. |
doi_str_mv | 10.1029/2002GL016720 |
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W. ; Dothe, H. ; Sharma, R. D.</creator><creatorcontrib>Duff, J. W. ; Dothe, H. ; Sharma, R. D.</creatorcontrib><description>The temperature dependence of the rate coefficient of the N(2D)+O2→NO+O reaction has been determined using ab initio potential energy surfaces (PES) and classical dynamics. The calculation agrees with the recommended rate coefficient at 300 K (∼110 km altitude). The rate coefficient is given by the expression k(T) = 6.2 × 10−12(T/300) cm3/s/molec. In contrast to the nearly temperature‐independent value of this rate coefficient previously recommended, the value given here increases by almost a factor of about four as the altitude increases from 110 to 200 km. It is also shown that even though N(2D) atoms in the thermosphere are produced with large translational energies, using the value of the rate coefficient at the local temperature introduces negligible error in the amount of NO produced. The new value of this rate coefficient will significantly increase the amount of NO computed in the aeronomic models causing a re‐evaluation of the heat budget and temperature and density structure of the thermosphere. In particular, implications of the larger rate coefficient for the recent observations of dramatically enhanced 5.3 μm emission from NO in the thermosphere due to solar storms are discussed.</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/2002GL016720</identifier><identifier>CODEN: GPRLAJ</identifier><language>eng</language><publisher>Washington, DC: Blackwell Publishing Ltd</publisher><subject>Atmospheric composition. Chemical and photochemical reactions ; Earth, ocean, space ; Exact sciences and technology ; External geophysics ; Physics of the high neutral atmosphere</subject><ispartof>Geophysical research letters, 2003-03, Vol.30 (5), p.63.1-n/a</ispartof><rights>Copyright 2003 by the American Geophysical Union.</rights><rights>2003 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2002GL016720$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2002GL016720$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,780,784,11514,27924,27925,46468,46892</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=14892717$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Duff, J. W.</creatorcontrib><creatorcontrib>Dothe, H.</creatorcontrib><creatorcontrib>Sharma, R. D.</creatorcontrib><title>On the rate coefficient of the N(2D)+O2→NO+O reaction in the terrestrial thermosphere</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>The temperature dependence of the rate coefficient of the N(2D)+O2→NO+O reaction has been determined using ab initio potential energy surfaces (PES) and classical dynamics. The calculation agrees with the recommended rate coefficient at 300 K (∼110 km altitude). The rate coefficient is given by the expression k(T) = 6.2 × 10−12(T/300) cm3/s/molec. In contrast to the nearly temperature‐independent value of this rate coefficient previously recommended, the value given here increases by almost a factor of about four as the altitude increases from 110 to 200 km. It is also shown that even though N(2D) atoms in the thermosphere are produced with large translational energies, using the value of the rate coefficient at the local temperature introduces negligible error in the amount of NO produced. The new value of this rate coefficient will significantly increase the amount of NO computed in the aeronomic models causing a re‐evaluation of the heat budget and temperature and density structure of the thermosphere. In particular, implications of the larger rate coefficient for the recent observations of dramatically enhanced 5.3 μm emission from NO in the thermosphere due to solar storms are discussed.</description><subject>Atmospheric composition. Chemical and photochemical reactions</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>External geophysics</subject><subject>Physics of the high neutral atmosphere</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><recordid>eNpNkN2O0zAQhS0EEqVwxwPkBgSqAmMnseNL1GVTUNVI_LSX1sSZCEOadO1Uu32BfQAekSchJRVwNX_nOxodxp5zeMNB6LcCQBRr4FIJeMBmXKdpnAOoh2wGoMdeKPmYPQnhOwAkkPAZ25VdNHyjyONAke2paZx11A1R3_zZb16Jq9eLUvy6_7kpF2XkCe3g-i5yEzeQ9xQG77A9z37fh8NY6Cl71GAb6NmlztnX6_dflqt4XRYflu_WsRMykzEXSmdK1zJveJ1iTnlNWKWY5hWq2taW5xZk1chKikaTIpRaoKqsrVHIKkvm7OXke_D9zXH8xOxdsNS22FF_DGb0h1SnMApfXIQYLLaNx866YA7e7dGfDE9zLRRXo05MulvX0unfHcw5YvN_xKb4tOZSKjlC8QS5MNDdXwj9DyNVojKz2xSmSD6v4ON2a7bJb1tXf2o</recordid><startdate>200303</startdate><enddate>200303</enddate><creator>Duff, J. W.</creator><creator>Dothe, H.</creator><creator>Sharma, R. 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Chemical and photochemical reactions</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>External geophysics</topic><topic>Physics of the high neutral atmosphere</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Duff, J. W.</creatorcontrib><creatorcontrib>Dothe, H.</creatorcontrib><creatorcontrib>Sharma, R. D.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Duff, J. W.</au><au>Dothe, H.</au><au>Sharma, R. D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>On the rate coefficient of the N(2D)+O2→NO+O reaction in the terrestrial thermosphere</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>2003-03</date><risdate>2003</risdate><volume>30</volume><issue>5</issue><spage>63.1</spage><epage>n/a</epage><pages>63.1-n/a</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><coden>GPRLAJ</coden><abstract>The temperature dependence of the rate coefficient of the N(2D)+O2→NO+O reaction has been determined using ab initio potential energy surfaces (PES) and classical dynamics. The calculation agrees with the recommended rate coefficient at 300 K (∼110 km altitude). The rate coefficient is given by the expression k(T) = 6.2 × 10−12(T/300) cm3/s/molec. In contrast to the nearly temperature‐independent value of this rate coefficient previously recommended, the value given here increases by almost a factor of about four as the altitude increases from 110 to 200 km. It is also shown that even though N(2D) atoms in the thermosphere are produced with large translational energies, using the value of the rate coefficient at the local temperature introduces negligible error in the amount of NO produced. The new value of this rate coefficient will significantly increase the amount of NO computed in the aeronomic models causing a re‐evaluation of the heat budget and temperature and density structure of the thermosphere. In particular, implications of the larger rate coefficient for the recent observations of dramatically enhanced 5.3 μm emission from NO in the thermosphere due to solar storms are discussed.</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2002GL016720</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Atmospheric composition. Chemical and photochemical reactions Earth, ocean, space Exact sciences and technology External geophysics Physics of the high neutral atmosphere |
title | On the rate coefficient of the N(2D)+O2→NO+O reaction in the terrestrial thermosphere |
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