First Comparison of Mesospheric Winds Measured with a Fabry-Perot

A Fabry-Perot interferometer (FPI) for mesospheric observations was installed at King Sejong Station (62.2°S, 58.9°W) in Antarctica in 2017. For the initial validation of the FPI measurements, we compare neutral wind data recorded with the FPI with those from a Meteor Radar (MR) located nearby. Th...

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Main Authors: Wonseok Lee, Yong Ha Kim, Changsup Lee, Qian Wu
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 2018-12-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://janss.kr/journal/article.php?code=64510
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spelling doaj-dd34da9c13994c59bcef7a4a8c95cf1b2020-11-25T01:29:48ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14092018-12-01354235242https://doi.org/10.5140/JASS.2018.35.4.235First Comparison of Mesospheric Winds Measured with a Fabry-PerotWonseok Lee0Yong Ha Kim1Changsup Lee2Qian Wu3Space Science and Geology, Chungnam National UniversitySpace Science and Geology, Chungnam National UniversityKorea Polar Research InstituteNational Center for Atmospheric Research, BoulderA Fabry-Perot interferometer (FPI) for mesospheric observations was installed at King Sejong Station (62.2°S, 58.9°W) in Antarctica in 2017. For the initial validation of the FPI measurements, we compare neutral wind data recorded with the FPI with those from a Meteor Radar (MR) located nearby. The overall characteristics of the FPI and MR winds of both OH 892.0 nm (87 km) and OI 557.7 nm (97 km) airglow layers are similar. The FPI winds of both layers generally match the MR winds well on the observed days, with a few exceptions. The correlation analysis of the FPI and MR wind data shows that the correlation coefficients for the zonal winds at 87 and 97 km are 0.28 and 0.54, respectively, and those for the meridional winds are 0.36 and 0.54, respectively. Based on the assumption that the distribution of the airglow emissions has a Gaussian function with respect to the altitude, we calculated the weighted mean winds from the MR wind profile and compared them with the FPI winds. By adjusting the peak height and full width at half maximum of the Gaussian function, we determined the change of the correlation between the two winds. The best correlation for the OH and OI airglow layers was obtained at a peak height of 88–89 km and 97–98 km, respectively.http://janss.kr/journal/article.php?code=64510mesosphere and lower thermosphereFabry-Perot interferometermeteor radar
collection DOAJ
language English
format Article
sources DOAJ
author Wonseok Lee
Yong Ha Kim
Changsup Lee
Qian Wu
spellingShingle Wonseok Lee
Yong Ha Kim
Changsup Lee
Qian Wu
First Comparison of Mesospheric Winds Measured with a Fabry-Perot
Journal of Astronomy and Space Sciences
mesosphere and lower thermosphere
Fabry-Perot interferometer
meteor radar
author_facet Wonseok Lee
Yong Ha Kim
Changsup Lee
Qian Wu
author_sort Wonseok Lee
title First Comparison of Mesospheric Winds Measured with a Fabry-Perot
title_short First Comparison of Mesospheric Winds Measured with a Fabry-Perot
title_full First Comparison of Mesospheric Winds Measured with a Fabry-Perot
title_fullStr First Comparison of Mesospheric Winds Measured with a Fabry-Perot
title_full_unstemmed First Comparison of Mesospheric Winds Measured with a Fabry-Perot
title_sort first comparison of mesospheric winds measured with a fabry-perot
publisher Korean Space Science Society (KSSS)
series Journal of Astronomy and Space Sciences
issn 2093-5587
2093-1409
publishDate 2018-12-01
description A Fabry-Perot interferometer (FPI) for mesospheric observations was installed at King Sejong Station (62.2°S, 58.9°W) in Antarctica in 2017. For the initial validation of the FPI measurements, we compare neutral wind data recorded with the FPI with those from a Meteor Radar (MR) located nearby. The overall characteristics of the FPI and MR winds of both OH 892.0 nm (87 km) and OI 557.7 nm (97 km) airglow layers are similar. The FPI winds of both layers generally match the MR winds well on the observed days, with a few exceptions. The correlation analysis of the FPI and MR wind data shows that the correlation coefficients for the zonal winds at 87 and 97 km are 0.28 and 0.54, respectively, and those for the meridional winds are 0.36 and 0.54, respectively. Based on the assumption that the distribution of the airglow emissions has a Gaussian function with respect to the altitude, we calculated the weighted mean winds from the MR wind profile and compared them with the FPI winds. By adjusting the peak height and full width at half maximum of the Gaussian function, we determined the change of the correlation between the two winds. The best correlation for the OH and OI airglow layers was obtained at a peak height of 88–89 km and 97–98 km, respectively.
topic mesosphere and lower thermosphere
Fabry-Perot interferometer
meteor radar
url http://janss.kr/journal/article.php?code=64510
work_keys_str_mv AT wonseoklee firstcomparisonofmesosphericwindsmeasuredwithafabryperot
AT yonghakim firstcomparisonofmesosphericwindsmeasuredwithafabryperot
AT changsuplee firstcomparisonofmesosphericwindsmeasuredwithafabryperot
AT qianwu firstcomparisonofmesosphericwindsmeasuredwithafabryperot
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