Articles | Volume 16, issue 8
https://doi.org/10.5194/acp-16-5021-2016
© Author(s) 2016. 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-16-5021-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Research article
| 
22 Apr 2016
Research article |
| 22 Apr 2016
Comparison of VLT/X-shooter OH and O2 rotational temperatures with consideration of TIMED/SABER emission and temperature profiles
Institute for Astro- and Particle Physics, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
Wolfgang Kausch
Department of Astrophysics, University of Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria
Institute for Astro- and Particle Physics, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
Stefan Kimeswenger
Instituto de Astronomía, Universidad Católica del Norte, Avenida Angamos 0610, Antofagasta, Chile
Institute for Astro- and Particle Physics, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
Stefanie Unterguggenberger
Institute for Astro- and Particle Physics, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
Amy M. Jones
Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85748 Garching, Germany
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Cited
22 citations as recorded by crossref.
- 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
- 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
- Climatologies of Various OH Lines From About 90,000 X‐Shooter Spectra S. Noll et al. 10.1029/2022JD038275
- 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
- Observational evidence for a quasi-bidecadal oscillation in the summer mesopause region over Western Europe C. Kalicinsky et al. 10.1016/j.jastp.2018.05.008
- 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
- Hydroxyl airglow observations for investigating atmospheric dynamics: results and challenges S. Wüst et al. 10.5194/acp-23-1599-2023
- 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
- Observations and Modeling of Potassium Emission in the Terrestrial Nightglow S. Noll et al. 10.1029/2018JD030044
- Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude site I. Reid et al. 10.5194/angeo-35-567-2017
- Variability of the Brunt–Väisälä frequency at the OH* layer height S. Wüst et al. 10.5194/amt-10-4895-2017
- Long-term Spectroscopic Observations of the Atmospheric Airglow by the Sloan Digital Sky Survey M. Hart 10.1088/1538-3873/aae972
- A Comparison of Einstein A Coefficients for OH Rotational Temperature Measurements Using a Large Astronomical Data Set M. Hart 10.3390/atmos10100569
- OH level populations and accuracies of Einstein-<i>A</i> coefficients from hundreds of measured lines S. Noll et al. 10.5194/acp-20-5269-2020
- Technical note: Bimodality in mesospheric OH rotational population distributions and implications for temperature measurements K. Kalogerakis 10.5194/acp-19-2629-2019
- Structure, variability, and origin of the low-latitude nightglow continuum between 300 and 1800 nm: evidence for HO2 emission in the near-infrared S. Noll et al. 10.5194/acp-24-1143-2024
- A comparison of ground-based hydroxyl airglow temperatures with SABER/TIMED measurements over 23° N, India N. Parihar et al. 10.5194/angeo-35-353-2017
- Mesospheric OH layer altitude at midlatitudes: variability over the Sierra Nevada Observatory in Granada, Spain (37° N, 3° W) M. García-Comas et al. 10.5194/angeo-35-1151-2017
- The airglow layer emission altitude cannot be determined unambiguously from temperature comparison with lidars T. Dunker 10.5194/acp-18-6691-2018
- 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
- Effect of water vapour absorption on hydroxyl temperatures measured from Svalbard J. Chadney et al. 10.5194/angeo-35-481-2017
- 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
22 citations as recorded by crossref.
- 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
- 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
- Climatologies of Various OH Lines From About 90,000 X‐Shooter Spectra S. Noll et al. 10.1029/2022JD038275
- 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
- Observational evidence for a quasi-bidecadal oscillation in the summer mesopause region over Western Europe C. Kalicinsky et al. 10.1016/j.jastp.2018.05.008
- 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
- Hydroxyl airglow observations for investigating atmospheric dynamics: results and challenges S. Wüst et al. 10.5194/acp-23-1599-2023
- 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
- Observations and Modeling of Potassium Emission in the Terrestrial Nightglow S. Noll et al. 10.1029/2018JD030044
- Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude site I. Reid et al. 10.5194/angeo-35-567-2017
- Variability of the Brunt–Väisälä frequency at the OH* layer height S. Wüst et al. 10.5194/amt-10-4895-2017
- Long-term Spectroscopic Observations of the Atmospheric Airglow by the Sloan Digital Sky Survey M. Hart 10.1088/1538-3873/aae972
- A Comparison of Einstein A Coefficients for OH Rotational Temperature Measurements Using a Large Astronomical Data Set M. Hart 10.3390/atmos10100569
- OH level populations and accuracies of Einstein-<i>A</i> coefficients from hundreds of measured lines S. Noll et al. 10.5194/acp-20-5269-2020
- Technical note: Bimodality in mesospheric OH rotational population distributions and implications for temperature measurements K. Kalogerakis 10.5194/acp-19-2629-2019
- Structure, variability, and origin of the low-latitude nightglow continuum between 300 and 1800 nm: evidence for HO2 emission in the near-infrared S. Noll et al. 10.5194/acp-24-1143-2024
- A comparison of ground-based hydroxyl airglow temperatures with SABER/TIMED measurements over 23° N, India N. Parihar et al. 10.5194/angeo-35-353-2017
- Mesospheric OH layer altitude at midlatitudes: variability over the Sierra Nevada Observatory in Granada, Spain (37° N, 3° W) M. García-Comas et al. 10.5194/angeo-35-1151-2017
- The airglow layer emission altitude cannot be determined unambiguously from temperature comparison with lidars T. Dunker 10.5194/acp-18-6691-2018
- 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
- Effect of water vapour absorption on hydroxyl temperatures measured from Svalbard J. Chadney et al. 10.5194/angeo-35-481-2017
- 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
Saved (preprint)
Latest update: 18 Apr 2024
Short summary
We compare temperatures derived from simultaneous observations of 25 OH and two O2 mesospheric airglow bands taken with the X-shooter spectrograph at the Very Large Telescope in Chile. Considering emission and temperature profile data from the radiometer SABER on the TIMED satellite, we find significant time-dependent non-thermal contributions to the OH-based temperatures, especially for bands originating from high vibrational levels. Many studies of the mesopause region are affected.
We compare temperatures derived from simultaneous observations of 25 OH and two O2 mesospheric...
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