Dmitriy S. Makarov, Evgeniy A. Serov, Tatyana A. Galanina, Aleksandra O. Koroleva, Mikhail Yu. Tretyakov
{"title":"The molecular oxygen 118-GHz line intensity revision","authors":"Dmitriy S. Makarov, Evgeniy A. Serov, Tatyana A. Galanina, Aleksandra O. Koroleva, Mikhail Yu. Tretyakov","doi":"10.1016/j.jms.2023.111792","DOIUrl":null,"url":null,"abstract":"<div><p>The intensity of the atmospheric diagnostic fine-structure line of the O<span><math><msub><mrow></mrow><mrow><mn>2</mn></mrow></msub></math></span><span> molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O</span><span><math><msub><mrow></mrow><mrow><mn>2</mn></mrow></msub></math></span> and O<span><math><msub><mrow></mrow><mrow><mn>2</mn></mrow></msub></math></span>–N<span><math><msub><mrow></mrow><mrow><mn>2</mn></mrow></msub></math></span> mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3)<span><math><mrow><mi>⋅</mi><mn>1</mn><msup><mrow><mn>0</mn></mrow><mrow><mo>−</mo><mn>25</mn></mrow></msup></mrow></math></span> cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to <span><math><mo>∼</mo></math></span>0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"395 ","pages":"Article 111792"},"PeriodicalIF":1.4000,"publicationDate":"2023-05-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Molecular Spectroscopy","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0022285223000577","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"PHYSICS, ATOMIC, MOLECULAR & CHEMICAL","Score":null,"Total":0}
引用次数: 0
Abstract
The intensity of the atmospheric diagnostic fine-structure line of the O molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O and O–N mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large.
期刊介绍:
The Journal of Molecular Spectroscopy presents experimental and theoretical articles on all subjects relevant to molecular spectroscopy and its modern applications. An international medium for the publication of some of the most significant research in the field, the Journal of Molecular Spectroscopy is an invaluable resource for astrophysicists, chemists, physicists, engineers, and others involved in molecular spectroscopy research and practice.