{"title":"现代光谱数据库中 16 700-17 000 cm-1 区域的水蒸气吸收线分析","authors":"L. N. Sinitsa, T. Yu. Chesnokova","doi":"10.1134/S1024856024010123","DOIUrl":null,"url":null,"abstract":"<p>The validation of H<sub>2</sub>O absorption lines parameters in the modern spectroscopic databases such as HITRAN2016, HITRAN2020, GEISA2020, and W2020 is carried out in the visible region 16 700–17 000 cm<sup>−1</sup>. The H<sub>2</sub>O transmission spectra are simulated with the spectroscopic databases and compared with laboratory spectra of pure water vapor and H<sub>2</sub>O–N<sub>2</sub> mixture (<i>P</i> = 1 atm) recorded using a Fourier spectrometer with light-emitting diodes of high luminance. The parameters of 65 H<sub>2</sub>O absorption lines from HITRAN2020 database are corrected on the basis of the measurements. The positions of 32 lines, intensities of 51 lines, and self-broadening coefficients of 10 lines are improved. The ratio of the HITRAN2020 broadening coefficients to the experimental values is close to 1, whereas the air pressure-induced line shift coefficients in the spectroscopic databases are, on average, two times higher than the experimental values, and therefore, our previously obtained experimental values of N<sub>2</sub> pressure-induced line shift coefficients are used to simulate the transmission spectra of the H<sub>2</sub>O–N<sub>2</sub> mixture. The difference of the experimental spectra from the spectra calculated with HITRAN2016, HITRAN2020, GEISA2020, W2020, and corrected HITRAN2020cor is estimated by the root-mean-square deviations RMS = 1.49 × 10<sup>–4</sup>, 1.64 × 10<sup>–4</sup>, 3.96 × 10<sup>–4</sup>, 3.49 × 10<sup>–4</sup>, and 1.26 × 10<sup>–4</sup>, respectively, in the case of pure water vapor and 1.15 × 10<sup>–4</sup>, 1.1 × 10<sup>–4</sup>, 2.23 × 10<sup>–4</sup>, 2.28 × 10<sup>–4</sup>, and 0.86 × 10<sup>–4</sup> in the case of H<sub>2</sub>O–N<sub>2</sub> mixture.</p>","PeriodicalId":46751,"journal":{"name":"Atmospheric and Oceanic Optics","volume":null,"pages":null},"PeriodicalIF":0.9000,"publicationDate":"2024-03-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Analysis of Water Vapor Absorption Lines in Modern Spectroscopic Databases in the 16 700–17 000 cm−1 Region\",\"authors\":\"L. N. Sinitsa, T. Yu. Chesnokova\",\"doi\":\"10.1134/S1024856024010123\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>The validation of H<sub>2</sub>O absorption lines parameters in the modern spectroscopic databases such as HITRAN2016, HITRAN2020, GEISA2020, and W2020 is carried out in the visible region 16 700–17 000 cm<sup>−1</sup>. The H<sub>2</sub>O transmission spectra are simulated with the spectroscopic databases and compared with laboratory spectra of pure water vapor and H<sub>2</sub>O–N<sub>2</sub> mixture (<i>P</i> = 1 atm) recorded using a Fourier spectrometer with light-emitting diodes of high luminance. The parameters of 65 H<sub>2</sub>O absorption lines from HITRAN2020 database are corrected on the basis of the measurements. The positions of 32 lines, intensities of 51 lines, and self-broadening coefficients of 10 lines are improved. The ratio of the HITRAN2020 broadening coefficients to the experimental values is close to 1, whereas the air pressure-induced line shift coefficients in the spectroscopic databases are, on average, two times higher than the experimental values, and therefore, our previously obtained experimental values of N<sub>2</sub> pressure-induced line shift coefficients are used to simulate the transmission spectra of the H<sub>2</sub>O–N<sub>2</sub> mixture. The difference of the experimental spectra from the spectra calculated with HITRAN2016, HITRAN2020, GEISA2020, W2020, and corrected HITRAN2020cor is estimated by the root-mean-square deviations RMS = 1.49 × 10<sup>–4</sup>, 1.64 × 10<sup>–4</sup>, 3.96 × 10<sup>–4</sup>, 3.49 × 10<sup>–4</sup>, and 1.26 × 10<sup>–4</sup>, respectively, in the case of pure water vapor and 1.15 × 10<sup>–4</sup>, 1.1 × 10<sup>–4</sup>, 2.23 × 10<sup>–4</sup>, 2.28 × 10<sup>–4</sup>, and 0.86 × 10<sup>–4</sup> in the case of H<sub>2</sub>O–N<sub>2</sub> mixture.</p>\",\"PeriodicalId\":46751,\"journal\":{\"name\":\"Atmospheric and Oceanic Optics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.9000,\"publicationDate\":\"2024-03-23\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Atmospheric and Oceanic Optics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://link.springer.com/article/10.1134/S1024856024010123\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"OPTICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Atmospheric and Oceanic Optics","FirstCategoryId":"1085","ListUrlMain":"https://link.springer.com/article/10.1134/S1024856024010123","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"OPTICS","Score":null,"Total":0}
Analysis of Water Vapor Absorption Lines in Modern Spectroscopic Databases in the 16 700–17 000 cm−1 Region
The validation of H2O absorption lines parameters in the modern spectroscopic databases such as HITRAN2016, HITRAN2020, GEISA2020, and W2020 is carried out in the visible region 16 700–17 000 cm−1. The H2O transmission spectra are simulated with the spectroscopic databases and compared with laboratory spectra of pure water vapor and H2O–N2 mixture (P = 1 atm) recorded using a Fourier spectrometer with light-emitting diodes of high luminance. The parameters of 65 H2O absorption lines from HITRAN2020 database are corrected on the basis of the measurements. The positions of 32 lines, intensities of 51 lines, and self-broadening coefficients of 10 lines are improved. The ratio of the HITRAN2020 broadening coefficients to the experimental values is close to 1, whereas the air pressure-induced line shift coefficients in the spectroscopic databases are, on average, two times higher than the experimental values, and therefore, our previously obtained experimental values of N2 pressure-induced line shift coefficients are used to simulate the transmission spectra of the H2O–N2 mixture. The difference of the experimental spectra from the spectra calculated with HITRAN2016, HITRAN2020, GEISA2020, W2020, and corrected HITRAN2020cor is estimated by the root-mean-square deviations RMS = 1.49 × 10–4, 1.64 × 10–4, 3.96 × 10–4, 3.49 × 10–4, and 1.26 × 10–4, respectively, in the case of pure water vapor and 1.15 × 10–4, 1.1 × 10–4, 2.23 × 10–4, 2.28 × 10–4, and 0.86 × 10–4 in the case of H2O–N2 mixture.
期刊介绍:
Atmospheric and Oceanic Optics is an international peer reviewed journal that presents experimental and theoretical articles relevant to a wide range of problems of atmospheric and oceanic optics, ecology, and climate. The journal coverage includes: scattering and transfer of optical waves, spectroscopy of atmospheric gases, turbulent and nonlinear optical phenomena, adaptive optics, remote (ground-based, airborne, and spaceborne) sensing of the atmosphere and the surface, methods for solving of inverse problems, new equipment for optical investigations, development of computer programs and databases for optical studies. Thematic issues are devoted to the studies of atmospheric ozone, adaptive, nonlinear, and coherent optics, regional climate and environmental monitoring, and other subjects.