Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725 nm)

<p>Accurate Rayleigh scattering and absorption cross sections of atmospheric gases are essential for understanding the propagation of electromagnetic radiation in planetary atmospheres. Accurate extinction cross sections are also essential for calibrating high-finesse optical cavities and diff...

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Main Authors: Q. He, Z. Fang, O. Shoshanim, S. S. Brown, Y. Rudich
Format: Article
Language:English
Published: Copernicus Publications 2021-10-01
Series:Atmospheric Chemistry and Physics
Online Access:https://acp.copernicus.org/articles/21/14927/2021/acp-21-14927-2021.pdf
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spelling doaj-2157e368e26944d6a273b129231c46c92021-10-08T06:45:08ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242021-10-0121149271494010.5194/acp-21-14927-2021Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725&thinsp;nm)Q. He0Z. Fang1O. Shoshanim2S. S. Brown3S. S. Brown4Y. Rudich5Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, IsraelDepartment of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, IsraelDepartment of Environmental Physics, Institute for Biological Research, Ness Ziona 74100, IsraelChemical Sciences Division, Earth System Research Laboratory, National Oceanic and Atmospheric Administration, 325, Broadway, Boulder, CO 80305, USADepartment of Chemistry, University of Colorado, 216 UCB, Boulder, CO 80309, USADepartment of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, Israel<p>Accurate Rayleigh scattering and absorption cross sections of atmospheric gases are essential for understanding the propagation of electromagnetic radiation in planetary atmospheres. Accurate extinction cross sections are also essential for calibrating high-finesse optical cavities and differential optical absorption spectroscopy and for accurate remote sensing. In this study, we measured the scattering and absorption cross sections of carbon dioxide, nitrous oxide, sulfur hexafluoride, oxygen, and methane in the continuous wavelength range of 307–725 nm using broadband cavity-enhanced spectroscopy (BBCES). The experimentally derived Rayleigh scattering cross sections for CO<span class="inline-formula"><sub>2</sub></span>, N<span class="inline-formula"><sub>2</sub></span>O, SF<span class="inline-formula"><sub>6</sub></span>, O<span class="inline-formula"><sub>2</sub></span>, and CH<span class="inline-formula"><sub>4</sub></span> agree with refractive index-based calculations, with a difference of (0.4 <span class="inline-formula">±</span> 1.2) %, (<span class="inline-formula">−</span>0.6 <span class="inline-formula">±</span> 1.1) %, (0.9 <span class="inline-formula">±</span> 1.4) %, (2.8 <span class="inline-formula">±</span> 1.2) %, and (0.9 <span class="inline-formula">±</span> 2.2) %, respectively. The O<span class="inline-formula"><sub>2</sub></span>–O<span class="inline-formula"><sub>2</sub></span> collision-induced absorption and absorption by methane are obtained with high precision at the 0.8 nm resolution of our BBCES instrument in the 307–725 nm wavelength range. New dispersion relations for N<span class="inline-formula"><sub>2</sub></span>O, SF<span class="inline-formula"><sub>6</sub></span>, and CH<span class="inline-formula"><sub>4</sub></span> were derived using data in the UV–vis wavelength range. This study provides dispersion relations for refractive indices, <span class="inline-formula"><i>n</i></span>-based Rayleigh scattering cross sections, and absorption cross sections based on more continuous and more extended wavelength ranges than available in the current literature.</p>https://acp.copernicus.org/articles/21/14927/2021/acp-21-14927-2021.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Q. He
Z. Fang
O. Shoshanim
S. S. Brown
S. S. Brown
Y. Rudich
spellingShingle Q. He
Z. Fang
O. Shoshanim
S. S. Brown
S. S. Brown
Y. Rudich
Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725&thinsp;nm)
Atmospheric Chemistry and Physics
author_facet Q. He
Z. Fang
O. Shoshanim
S. S. Brown
S. S. Brown
Y. Rudich
author_sort Q. He
title Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725&thinsp;nm)
title_short Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725&thinsp;nm)
title_full Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725&thinsp;nm)
title_fullStr Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725&thinsp;nm)
title_full_unstemmed Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725&thinsp;nm)
title_sort scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725&thinsp;nm)
publisher Copernicus Publications
series Atmospheric Chemistry and Physics
issn 1680-7316
1680-7324
publishDate 2021-10-01
description <p>Accurate Rayleigh scattering and absorption cross sections of atmospheric gases are essential for understanding the propagation of electromagnetic radiation in planetary atmospheres. Accurate extinction cross sections are also essential for calibrating high-finesse optical cavities and differential optical absorption spectroscopy and for accurate remote sensing. In this study, we measured the scattering and absorption cross sections of carbon dioxide, nitrous oxide, sulfur hexafluoride, oxygen, and methane in the continuous wavelength range of 307–725 nm using broadband cavity-enhanced spectroscopy (BBCES). The experimentally derived Rayleigh scattering cross sections for CO<span class="inline-formula"><sub>2</sub></span>, N<span class="inline-formula"><sub>2</sub></span>O, SF<span class="inline-formula"><sub>6</sub></span>, O<span class="inline-formula"><sub>2</sub></span>, and CH<span class="inline-formula"><sub>4</sub></span> agree with refractive index-based calculations, with a difference of (0.4 <span class="inline-formula">±</span> 1.2) %, (<span class="inline-formula">−</span>0.6 <span class="inline-formula">±</span> 1.1) %, (0.9 <span class="inline-formula">±</span> 1.4) %, (2.8 <span class="inline-formula">±</span> 1.2) %, and (0.9 <span class="inline-formula">±</span> 2.2) %, respectively. The O<span class="inline-formula"><sub>2</sub></span>–O<span class="inline-formula"><sub>2</sub></span> collision-induced absorption and absorption by methane are obtained with high precision at the 0.8 nm resolution of our BBCES instrument in the 307–725 nm wavelength range. New dispersion relations for N<span class="inline-formula"><sub>2</sub></span>O, SF<span class="inline-formula"><sub>6</sub></span>, and CH<span class="inline-formula"><sub>4</sub></span> were derived using data in the UV–vis wavelength range. This study provides dispersion relations for refractive indices, <span class="inline-formula"><i>n</i></span>-based Rayleigh scattering cross sections, and absorption cross sections based on more continuous and more extended wavelength ranges than available in the current literature.</p>
url https://acp.copernicus.org/articles/21/14927/2021/acp-21-14927-2021.pdf
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