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Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
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Line emission from hydroxyl (OH) molecules at altitudes of about 90 km strongly contributes to the Earth's night-sky brightness and is therefore used as an important indicator of atmospheric chemistry and dynamics. However, interpreting the measurements can be ambiguous since necessary molecular parameters and the internal state of OH are not well known. Based on high-quality spectral data, we investigated these issues and found solutions for a better understanding of the OH line intensities.
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ACP | Articles | Volume 20, issue 9
ACP | Articles | Volume 20, issue 9
Atmos. Chem. Phys., 20, 5269–5292, 2020
https://doi.org/10.5194/acp-20-5269-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
Atmos. Chem. Phys., 20, 5269–5292, 2020
https://doi.org/10.5194/acp-20-5269-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
ACP | Articles | Volume 20, issue 9

Research article 06 May 2020

Research article | 06 May 2020

OH level populations and accuracies of Einstein-A coefficients from hundreds of measured lines

Stefan Noll et al.

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Short summary
Line emission from hydroxyl (OH) molecules at altitudes of about 90 km strongly contributes to the Earth's night-sky brightness and is therefore used as an important indicator of atmospheric chemistry and dynamics. However, interpreting the measurements can be ambiguous since necessary molecular parameters and the internal state of OH are not well known. Based on high-quality spectral data, we investigated these issues and found solutions for a better understanding of the OH line intensities.
Read more
Citation
Altmetrics
Final-revised paper
Preprint
Atmospheric Chemistry and Physics

An interactive open-access journal of the European Geosciences Union

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