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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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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1725094587491418112 |