A comparison of MLT wind between meteor radar chain data and SD-WACCM results

A meteor radar chain located along the 120°E meridian in the Northern Hemisphere from low to middle latitudes provides long-term horizontal wind observations of the mesosphere and lower thermosphere (MLT) region. In this study, we report a seasonal variation and its latitudinal feature in the horizo...

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Main Authors: BaoZhu Zhou, XiangHui Xue, Wen Yi, HaiLun Ye, Jie Zeng, JinSong Chen, JianFei Wu, TingDi Chen, XianKang Dou
Format: Article
Language:English
Published: Science Press 2022-08-01
Series:Earth and Planetary Physics
Subjects:
Online Access:http://www.eppcgs.org/article/doi/10.26464/epp2022040?pageType=en
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author BaoZhu Zhou
XiangHui Xue
Wen Yi
HaiLun Ye
Jie Zeng
JinSong Chen
JianFei Wu
TingDi Chen
XianKang Dou
author_facet BaoZhu Zhou
XiangHui Xue
Wen Yi
HaiLun Ye
Jie Zeng
JinSong Chen
JianFei Wu
TingDi Chen
XianKang Dou
author_sort BaoZhu Zhou
collection DOAJ
description A meteor radar chain located along the 120°E meridian in the Northern Hemisphere from low to middle latitudes provides long-term horizontal wind observations of the mesosphere and lower thermosphere (MLT) region. In this study, we report a seasonal variation and its latitudinal feature in the horizontal mean wind in the MLT region observed by six meteor radar instruments located at Mohe (53.5°N, 122.3°E), Beijing (40.3°N, 116.2°E), Mengcheng (33.4°N, 116.5°E), Wuhan (30.6°N, 114.4°E), Kunming (25.6°N, 108.3°E), and Fuke (19.5°N, 109.1°E) stations. In addition, we compare the wind in the MLT region measured by the meteor radar stations with those simulated by the Whole Atmosphere Community Climate Model (WACCM). In general, the WACCM appears to capture well the seasonal and latitudinal variations in the zonal wind component. In particular, the temporal evolution of the eastward zonal wind maximum shifts from July to May as the latitude decreases. However, the simulated WACCM meridional wind exhibits differences from the meteor radar observations.
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spelling doaj.art-81c97a543650447ab71595cacf86fa342022-12-22T01:48:59ZengScience PressEarth and Planetary Physics2096-39552022-08-016545146410.26464/epp2022040RA325-zhoubaozhu-FA comparison of MLT wind between meteor radar chain data and SD-WACCM resultsBaoZhu Zhou0XiangHui Xue1Wen Yi2HaiLun Ye3Jie Zeng4JinSong Chen5JianFei Wu6TingDi Chen7XianKang Dou8CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaNational Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, ChinaA meteor radar chain located along the 120°E meridian in the Northern Hemisphere from low to middle latitudes provides long-term horizontal wind observations of the mesosphere and lower thermosphere (MLT) region. In this study, we report a seasonal variation and its latitudinal feature in the horizontal mean wind in the MLT region observed by six meteor radar instruments located at Mohe (53.5°N, 122.3°E), Beijing (40.3°N, 116.2°E), Mengcheng (33.4°N, 116.5°E), Wuhan (30.6°N, 114.4°E), Kunming (25.6°N, 108.3°E), and Fuke (19.5°N, 109.1°E) stations. In addition, we compare the wind in the MLT region measured by the meteor radar stations with those simulated by the Whole Atmosphere Community Climate Model (WACCM). In general, the WACCM appears to capture well the seasonal and latitudinal variations in the zonal wind component. In particular, the temporal evolution of the eastward zonal wind maximum shifts from July to May as the latitude decreases. However, the simulated WACCM meridional wind exhibits differences from the meteor radar observations.http://www.eppcgs.org/article/doi/10.26464/epp2022040?pageType=enmeteor radar chainmlt horizontal windtidesd-waccm
spellingShingle BaoZhu Zhou
XiangHui Xue
Wen Yi
HaiLun Ye
Jie Zeng
JinSong Chen
JianFei Wu
TingDi Chen
XianKang Dou
A comparison of MLT wind between meteor radar chain data and SD-WACCM results
Earth and Planetary Physics
meteor radar chain
mlt horizontal wind
tide
sd-waccm
title A comparison of MLT wind between meteor radar chain data and SD-WACCM results
title_full A comparison of MLT wind between meteor radar chain data and SD-WACCM results
title_fullStr A comparison of MLT wind between meteor radar chain data and SD-WACCM results
title_full_unstemmed A comparison of MLT wind between meteor radar chain data and SD-WACCM results
title_short A comparison of MLT wind between meteor radar chain data and SD-WACCM results
title_sort comparison of mlt wind between meteor radar chain data and sd waccm results
topic meteor radar chain
mlt horizontal wind
tide
sd-waccm
url http://www.eppcgs.org/article/doi/10.26464/epp2022040?pageType=en
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