Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude site
We consider 5 years of spectrometer measurements of OH(6–2) and O<sub>2</sub>(0–1) airglow emission intensities and temperatures made near Adelaide, Australia (35° S, 138° E), between September 2001 and August 2006 and compare them with measurements of the same parameters from at the...
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Format: | Article |
Language: | English |
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Copernicus Publications
2017-04-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/35/567/2017/angeo-35-567-2017.pdf |
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author | I. M. Reid I. M. Reid A. J. Spargo J. M. Woithe A. R. Klekociuk A. R. Klekociuk J. P. Younger J. P. Younger G. G. Sivjee |
author_facet | I. M. Reid I. M. Reid A. J. Spargo J. M. Woithe A. R. Klekociuk A. R. Klekociuk J. P. Younger J. P. Younger G. G. Sivjee |
author_sort | I. M. Reid |
collection | DOAJ |
description | We consider 5 years of spectrometer measurements of OH(6–2) and O<sub>2</sub>(0–1)
airglow emission intensities and temperatures made near Adelaide, Australia
(35° S, 138° E), between September 2001 and August 2006 and
compare them with measurements of the same parameters from at the same site
using an airglow imager, with the intensities of the OH(8–3) and O(<sup>1</sup>S)
emissions made with a filter photometer, and with 2 years of Aura MLS
(Microwave Limb Sounder) v3.3 temperatures and 4.5 years of TIMED SABER
(Thermosphere Ionosphere Mesosphere Energetics and Dynamics Sounding of the
Atmosphere using Broadband Emission Radiometry) v2.0 temperatures for the
same site. We also consider whether we can recover the actual emission
heights from the intercomparison of the ground-based and satellite
observations. We find a significant improvement in the correlation between
the spectrometer OH and SABER temperatures by interpolating the latter to
constant density surfaces determined using a meteor radar. |
first_indexed | 2024-12-11T05:37:18Z |
format | Article |
id | doaj.art-9e05655238d149e08d75e266522992b9 |
institution | Directory Open Access Journal |
issn | 0992-7689 1432-0576 |
language | English |
last_indexed | 2024-12-11T05:37:18Z |
publishDate | 2017-04-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Annales Geophysicae |
spelling | doaj.art-9e05655238d149e08d75e266522992b92022-12-22T01:19:14ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762017-04-013556758210.5194/angeo-35-567-2017Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude siteI. M. Reid0I. M. Reid1A. J. Spargo2J. M. Woithe3A. R. Klekociuk4A. R. Klekociuk5J. P. Younger6J. P. Younger7G. G. Sivjee8ATRAD Pty Ltd, 20 Phillips St., Thebarton, 5031, AustraliaSchool of Physical Sciences, University of Adelaide, Adelaide 5000, AustraliaSchool of Physical Sciences, University of Adelaide, Adelaide 5000, AustraliaATRAD Pty Ltd, 20 Phillips St., Thebarton, 5031, AustraliaSchool of Physical Sciences, University of Adelaide, Adelaide 5000, AustraliaAntarctica and the Global System, Australian Antarctic Division, Department of the Environment and Energy, Kingston, Tasmania, AustraliaATRAD Pty Ltd, 20 Phillips St., Thebarton, 5031, AustraliaSchool of Physical Sciences, University of Adelaide, Adelaide 5000, AustraliaEmbry Riddle Aeronautical University, Department Physical Sciences, Daytona Beach, FL 32114, USAWe consider 5 years of spectrometer measurements of OH(6–2) and O<sub>2</sub>(0–1) airglow emission intensities and temperatures made near Adelaide, Australia (35° S, 138° E), between September 2001 and August 2006 and compare them with measurements of the same parameters from at the same site using an airglow imager, with the intensities of the OH(8–3) and O(<sup>1</sup>S) emissions made with a filter photometer, and with 2 years of Aura MLS (Microwave Limb Sounder) v3.3 temperatures and 4.5 years of TIMED SABER (Thermosphere Ionosphere Mesosphere Energetics and Dynamics Sounding of the Atmosphere using Broadband Emission Radiometry) v2.0 temperatures for the same site. We also consider whether we can recover the actual emission heights from the intercomparison of the ground-based and satellite observations. We find a significant improvement in the correlation between the spectrometer OH and SABER temperatures by interpolating the latter to constant density surfaces determined using a meteor radar.https://www.ann-geophys.net/35/567/2017/angeo-35-567-2017.pdf |
spellingShingle | I. M. Reid I. M. Reid A. J. Spargo J. M. Woithe A. R. Klekociuk A. R. Klekociuk J. P. Younger J. P. Younger G. G. Sivjee Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude site Annales Geophysicae |
title | Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude site |
title_full | Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude site |
title_fullStr | Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude site |
title_full_unstemmed | Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude site |
title_short | Seasonal MLT-region nightglow intensities, temperatures, and emission heights at a Southern Hemisphere midlatitude site |
title_sort | seasonal mlt region nightglow intensities temperatures and emission heights at a southern hemisphere midlatitude site |
url | https://www.ann-geophys.net/35/567/2017/angeo-35-567-2017.pdf |
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