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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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 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 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 nm) |
title_short |
Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725 nm) |
title_full |
Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725 nm) |
title_fullStr |
Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725 nm) |
title_full_unstemmed |
Scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725 nm) |
title_sort |
scattering and absorption cross sections of atmospheric gases in the ultraviolet–visible wavelength range (307–725 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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