Articles | Volume 20, issue 9
https://doi.org/10.5194/acp-20-5269-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/acp-20-5269-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Research article
| 
06 May 2020
Research article |
| 06 May 2020
OH level populations and accuracies of Einstein-A coefficients from hundreds of measured lines
Institut für Physik, Universität Augsburg, Augsburg, Germany
Deutsches Fernerkundungsdatenzentrum, Deutsches Zentrum für Luft-
und Raumfahrt, Weßling-Oberpfaffenhofen, Germany
Holger Winkler
Institut für Umweltphysik, Universität Bremen, Bremen, Germany
Oleg Goussev
Deutsches Fernerkundungsdatenzentrum, Deutsches Zentrum für Luft-
und Raumfahrt, Weßling-Oberpfaffenhofen, Germany
Bastian Proxauf
Max-Planck-Institut für Sonnensystemforschung, Göttingen,
Germany
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Cited
15 citations as recorded by crossref.
- Global modelling of the observed line positions for the spectra of ultraviolet bands: Dunham coefficients for the A2Σ+ excited state of the 16OH molecule O. Sulakshina & Y. Borkov 10.1080/00268976.2023.2222346
- Non-local thermal equilibrium spectra of atmospheric molecules for exoplanets S. Wright et al. 10.1093/mnras/stac654
- Infrared Spectra of Small Radicals for Exoplanetary Spectroscopy: OH, NH, CN and CH: The State of Current Knowledge S. Civiš et al. 10.3390/molecules28083362
- Intra-annual variations of spectrally resolved gravity wave activity in the upper mesosphere/lower thermosphere (UMLT) region R. Sedlak et al. 10.5194/amt-13-5117-2020
- Studies of atmospheric waves by ground-based observations of OH(3–1) emission and rotational temperature using PRL airglow InfraRed spectrograph (PAIRS) R. Singh et al. 10.1016/j.jastp.2023.106039
- Global modelling of the observed line positions: Dunham coefficients for the ground state of 16OH molecule O. Sulakshina & Y. Borkov 10.1080/00268976.2022.2072408
- The HITRAN2020 molecular spectroscopic database I. Gordon et al. 10.1016/j.jqsrt.2021.107949
- Hydroxyl airglow observations for investigating atmospheric dynamics: results and challenges S. Wüst et al. 10.5194/acp-23-1599-2023
- First Detection of Hydroxyl Radical Emission from an Exoplanet Atmosphere: High-dispersion Characterization of WASP-33b Using Subaru/IRD S. Nugroho et al. 10.3847/2041-8213/abec71
- OH vibrational distributions: A comparison of Einstein A transition probabilities M. Hart 10.1016/j.jqsrt.2021.107770
- Climatologies of Various OH Lines From About 90,000 X‐Shooter Spectra S. Noll et al. 10.1029/2022JD038275
- A Spectroscopic Thermometer: Individual Vibrational Band Spectroscopy with the Example of OH in the Atmosphere of WASP-33b S. Wright et al. 10.3847/1538-3881/acdb75
- A high throughput rapid scanning dispersive spectrometer for longwave infrared absorption spectroscopy A. Butler et al. 10.1088/1361-6501/ac9d5b
- Effective Emission Heights of Various OH Lines From X‐Shooter and SABER Observations of a Passing Quasi‐2‐Day Wave S. Noll et al. 10.1029/2022JD036610
- Analysis of 24 years of mesopause region OH rotational temperature observations at Davis, Antarctica – Part 1: long-term trends W. French et al. 10.5194/acp-20-6379-2020
14 citations as recorded by crossref.
- Global modelling of the observed line positions for the spectra of ultraviolet bands: Dunham coefficients for the A2Σ+ excited state of the 16OH molecule O. Sulakshina & Y. Borkov 10.1080/00268976.2023.2222346
- Non-local thermal equilibrium spectra of atmospheric molecules for exoplanets S. Wright et al. 10.1093/mnras/stac654
- Infrared Spectra of Small Radicals for Exoplanetary Spectroscopy: OH, NH, CN and CH: The State of Current Knowledge S. Civiš et al. 10.3390/molecules28083362
- Intra-annual variations of spectrally resolved gravity wave activity in the upper mesosphere/lower thermosphere (UMLT) region R. Sedlak et al. 10.5194/amt-13-5117-2020
- Studies of atmospheric waves by ground-based observations of OH(3–1) emission and rotational temperature using PRL airglow InfraRed spectrograph (PAIRS) R. Singh et al. 10.1016/j.jastp.2023.106039
- Global modelling of the observed line positions: Dunham coefficients for the ground state of 16OH molecule O. Sulakshina & Y. Borkov 10.1080/00268976.2022.2072408
- The HITRAN2020 molecular spectroscopic database I. Gordon et al. 10.1016/j.jqsrt.2021.107949
- Hydroxyl airglow observations for investigating atmospheric dynamics: results and challenges S. Wüst et al. 10.5194/acp-23-1599-2023
- First Detection of Hydroxyl Radical Emission from an Exoplanet Atmosphere: High-dispersion Characterization of WASP-33b Using Subaru/IRD S. Nugroho et al. 10.3847/2041-8213/abec71
- OH vibrational distributions: A comparison of Einstein A transition probabilities M. Hart 10.1016/j.jqsrt.2021.107770
- Climatologies of Various OH Lines From About 90,000 X‐Shooter Spectra S. Noll et al. 10.1029/2022JD038275
- A Spectroscopic Thermometer: Individual Vibrational Band Spectroscopy with the Example of OH in the Atmosphere of WASP-33b S. Wright et al. 10.3847/1538-3881/acdb75
- A high throughput rapid scanning dispersive spectrometer for longwave infrared absorption spectroscopy A. Butler et al. 10.1088/1361-6501/ac9d5b
- Effective Emission Heights of Various OH Lines From X‐Shooter and SABER Observations of a Passing Quasi‐2‐Day Wave S. Noll et al. 10.1029/2022JD036610
Latest update: 01 Oct 2023
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.
Line emission from hydroxyl (OH) molecules at altitudes of about 90 km strongly contributes to...
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