Passive Optical Observation of Mesosphere and Thermosphere Wind Over Three Stations in China

Author:

Wei Yafei12,Gu Sheng‐Yang123ORCID,Li Na4ORCID,Qin Yusong1ORCID,Sun Ruidi1ORCID,Wang Dong1,Hu Guoyuan1ORCID,Le Huijun5ORCID,Yuan Wei6ORCID

Affiliation:

1. Electronic Information School Wuhan University Wuhan China

2. Hubei Luojia Laboratory Wuhan China

3. Wuhan Institute of Quantum Technology Wuhan China

4. National Key Laboratory of Electromagnetic Environment China Research Institute of Radio‐Wave Propagation Qingdao China

5. Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China

6. National Space Science Center Chinese Academy of Sciences Beijing China

Abstract

AbstractFabry Perot interferometer (FPI) is an essential ground‐based passive optical observation device to detect middle and upper atmospheric information. Three FPIs are located at Kunming (103.8°E, 25.6°N), Xinglong (117.4°E, 40.2°N), and Mohe (122.3°E, 53.5°N), China. The diurnal and annual variation of night wind at 87, 97, and 250 km are investigated from 2019 to 2021, compared to Horizontal Wind Model 14 (HWM14) to check the prediction accuracy for the local wind field. Our results are as follows: (a) At 87 km, the zonal winds are similar in Kunming and Xinglong, but the meridional winds are generally stronger in Kunming. The zonal and meridional winds in both locations are dominated by semidiurnal variations. (b) At 97 km, the duration of semidiurnal variation of zonal winds and diurnal variation of meridional winds in Kunming is long, which is opposite to that of Xinglong. (c) At 250 km, the wind speed increases with latitude for both zonal and meridional winds, which are both dominated by diurnal variations for all the three sites. Unlike 87 and 97 km, the entire wind field at 250 km is dominated by annual variation, except for a significant semiannual variation at midnight in Mohe. (d) Overall, the HWM14 predictions are stronger than the FPI measurements at peak wind speeds and similar at 87 and 97 km, which surpasses the performance at 250 km. Especially at 250 km, the model results are worse for the zonal winds of Kunming and the meridional winds of Mohe. These results will help to understand the wind field in the middle and upper atmosphere and improve the accuracy of the model.

Publisher

American Geophysical Union (AGU)

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