Robert J. Hargreaves, Iouli E. Gordon, Xinchuan Huang, Geoffrey C. Toon, Laurence S. Rothman
{"title":"Updating the carbon dioxide line list in HITEMP","authors":"Robert J. Hargreaves, Iouli E. Gordon, Xinchuan Huang, Geoffrey C. Toon, Laurence S. Rothman","doi":"10.1016/j.jqsrt.2024.109324","DOIUrl":null,"url":null,"abstract":"An updated carbon dioxide line list for the HITEMP spectroscopic database is presented. This line list covers the 0–17<ce:hsp sp=\"0.16667\"></ce:hsp>697 cm<ce:sup loc=\"post\">−1</ce:sup> (<mml:math altimg=\"si1.svg\" display=\"inline\"><mml:mo>></mml:mo></mml:math>565 nm) spectral range and is built upon the AI-3000K semi-empirical line list for <ce:sup loc=\"post\">12</ce:sup>C<ce:sup loc=\"post\">16</ce:sup>O<ce:inf loc=\"post\">2</ce:inf>, <ce:sup loc=\"post\">13</ce:sup>C<ce:sup loc=\"post\">16</ce:sup>O<ce:inf loc=\"post\">2</ce:inf>, <ce:sup loc=\"post\">16</ce:sup>O<ce:sup loc=\"post\">12</ce:sup>C<ce:sup loc=\"post\">18</ce:sup>O, and <ce:sup loc=\"post\">16</ce:sup>O<ce:sup loc=\"post\">12</ce:sup>C<ce:sup loc=\"post\">17</ce:sup>O (Huang et al., 2023), combined with HITRAN2020 data, additional isotopologues, and further improvements described in this work. In order to make the line list practical for applications, over 36 billion individual transitions of the original AI-3000K line list have been separated into “strong” and “weak”. “Strong” transitions were adapted directly, while the weak transitions were then combined into so-called “effective” lines. The latter can accurately account for the intensity contribution of underlying weak AI-3000K transitions while reducing the database by over two orders of magnitude (to <mml:math altimg=\"si2.svg\" display=\"inline\"><mml:mo>∼</mml:mo></mml:math>326 million). In addition, pressure broadening parameters have been revised for this work to improve applicability at high temperatures. The line list has been added to HITEMP and is suitable for modeling the spectrum of carbon dioxide at temperatures up to 3000 K.","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"23 1","pages":""},"PeriodicalIF":2.3000,"publicationDate":"2024-12-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Quantitative Spectroscopy & Radiative Transfer","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1016/j.jqsrt.2024.109324","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"OPTICS","Score":null,"Total":0}
引用次数: 0
Abstract
An updated carbon dioxide line list for the HITEMP spectroscopic database is presented. This line list covers the 0–17697 cm−1 (>565 nm) spectral range and is built upon the AI-3000K semi-empirical line list for 12C16O2, 13C16O2, 16O12C18O, and 16O12C17O (Huang et al., 2023), combined with HITRAN2020 data, additional isotopologues, and further improvements described in this work. In order to make the line list practical for applications, over 36 billion individual transitions of the original AI-3000K line list have been separated into “strong” and “weak”. “Strong” transitions were adapted directly, while the weak transitions were then combined into so-called “effective” lines. The latter can accurately account for the intensity contribution of underlying weak AI-3000K transitions while reducing the database by over two orders of magnitude (to ∼326 million). In addition, pressure broadening parameters have been revised for this work to improve applicability at high temperatures. The line list has been added to HITEMP and is suitable for modeling the spectrum of carbon dioxide at temperatures up to 3000 K.
期刊介绍:
Papers with the following subject areas are suitable for publication in the Journal of Quantitative Spectroscopy and Radiative Transfer:
- Theoretical and experimental aspects of the spectra of atoms, molecules, ions, and plasmas.
- Spectral lineshape studies including models and computational algorithms.
- Atmospheric spectroscopy.
- Theoretical and experimental aspects of light scattering.
- Application of light scattering in particle characterization and remote sensing.
- Application of light scattering in biological sciences and medicine.
- Radiative transfer in absorbing, emitting, and scattering media.
- Radiative transfer in stochastic media.