Articles | Volume 15, issue 7
https://doi.org/10.5194/acp-15-3647-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/acp-15-3647-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
OH populations and temperatures from simultaneous spectroscopic observations of 25 bands
Institute for Astro- and Particle Physics, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
W. Kausch
Institute for Astro- and Particle Physics, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
Department of Astrophysics, University of Vienna, Türkenschanzstr. 17, 1180 Vienna, Austria
S. Kimeswenger
Institute for Astro- and Particle Physics, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
Instituto de Astronom\'ia, Universidad Católica del Norte, Avenida Angamos 0610, Antofagasta, Chile
S. Unterguggenberger
Institute for Astro- and Particle Physics, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
A. M. Jones
Institute for Astro- and Particle Physics, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85748 Garching, Germany
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34 citations as recorded by crossref.
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- OH vibrational distributions: A comparison of Einstein A transition probabilities M. Hart 10.1016/j.jqsrt.2021.107770
- Mechanisms for varying non-LTE contributions to OH rotational temperatures from measurements and modelling. II. Kinetic model S. Noll et al. 10.1016/j.jastp.2018.05.005
- Observations and Modeling of Potassium Emission in the Terrestrial Nightglow S. Noll et al. 10.1029/2018JD030044
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- Effect of water vapour absorption on hydroxyl temperatures measured from Svalbard J. Chadney et al. 10.5194/angeo-35-481-2017
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- Technical note: Bimodality in mesospheric OH rotational population distributions and implications for temperature measurements K. Kalogerakis 10.5194/acp-19-2629-2019
- 15 years of VLT/UVES OH intensities and temperatures in comparison with TIMED/SABER data S. Noll et al. 10.1016/j.jastp.2017.05.012
- Comparison of VLT/X-shooter OH and O<sub>2</sub> rotational temperatures with consideration of TIMED/SABER emission and temperature profiles S. Noll et al. 10.5194/acp-16-5021-2016
- A Comparison of Einstein A Coefficients for OH Rotational Temperature Measurements Using a Large Astronomical Data Set M. Hart 10.3390/atmos10100569
- Multi-year behaviour of the midnight OH ∗ temperature according to observations at Zvenigorod over 2000–2016 V. Perminov et al. 10.1016/j.asr.2017.07.020
- Airglow Derived Measurements of Q-Branch Transition Probabilities for Several Hydroxyl Meinel Bands C. Franzen et al. 10.3390/atmos10100637
- Temperature estimation from hydroxyl airglow emission in the Venus night side mesosphere A. Migliorini et al. 10.1016/j.icarus.2017.09.026
- Comparison of rotational temperature derived from ground‐based OH airglow observations with TIMED/SABER to evaluate the Einstein coefficients W. Liu et al. 10.1002/2015JA021886
- New insights for mesospheric OH: multi-quantum vibrational relaxation as a driver for non-local thermodynamic equilibrium K. Kalogerakis et al. 10.5194/angeo-36-13-2018
- Atomic Oxygen Abundance Retrieved From SCIAMACHY Hydroxyl Nightglow Measurements Y. Zhu & M. Kaufmann 10.1029/2018GL079259
- A fast SWIR imager for observations of transient features in OH airglow P. Hannawald et al. 10.5194/amt-9-1461-2016
- Fringing Analysis and Simulation for the Vera C. Rubin Observatory’s Legacy Survey of Space and Time Z. Guo et al. 10.1088/1538-3873/acbe67
- Resolving the mesospheric nighttime 4.3 µm emission puzzle: Laboratory demonstration of new mechanism for OH(υ) relaxation K. Kalogerakis et al. 10.1002/2016GL069645
- Climatologies of Various OH Lines From About 90,000 X‐Shooter Spectra S. Noll et al. 10.1029/2022JD038275
- First ground-based observations of mesopause temperatures above the Eastern-Mediterranean Part I: Multi-day oscillations and tides I. Silber et al. 10.1016/j.jastp.2016.08.014
- Long-term Spectroscopic Observations of the Atmospheric Airglow by the Sloan Digital Sky Survey M. Hart 10.1088/1538-3873/aae972
- The airglow layer emission altitude cannot be determined unambiguously from temperature comparison with lidars T. Dunker 10.5194/acp-18-6691-2018
- Comparison between seasonal variations in tidal and internal gravity wave activity as derived from observations at Maimaga and Tiksi В. Сивцева et al. 10.12737/szf-42201811
- Mechanisms for varying non-LTE contributions to OH rotational temperatures from measurements and modelling. I. Climatology S. Noll et al. 10.1016/j.jastp.2018.05.004
- Modelled effects of temperature gradients and waves on the hydroxyl rotational distribution in ground-based airglow measurements C. Franzen et al. 10.5194/acp-20-333-2020
- A comparison of OH nightglow volume emission rates as measured by SCIAMACHY and SABER Y. Zhu et al. 10.5194/amt-13-3033-2020
- Measuring FeO variation using astronomical spectroscopic observations S. Unterguggenberger et al. 10.5194/acp-17-4177-2017
- 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
- 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
- Airglow in the Earth atmosphere: basic characteristics and excitation mechanisms C. Savigny 10.1007/s40828-017-0051-y
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Saved (preprint)
Latest update: 19 Nov 2024
Short summary
We discuss a high-quality data set of simultaneous observations of 25 OH bands with an astronomical echelle spectrograph. These data allowed us to analyse band-dependent OH populations and temperatures. In particular, we could find different non-LTE contributions to OH rotational temperatures depending on band, line set, and observing time. This is critical for mesopause studies that use these temperatures as a proxy of the true temperatures.
We discuss a high-quality data set of simultaneous observations of 25 OH bands with an...
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