Articles | Volume 24, issue 23
https://doi.org/10.5194/acp-24-13299-2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/acp-24-13299-2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
The impact of quasi-biennial oscillation (QBO) disruptions on diurnal tides over the low- and mid-latitude mesosphere and lower thermosphere (MLT) region observed by a meteor radar chain
Jianyuan Wang
National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, China
Kunming Electro-magnetic Environment Observation and Research Station, Qujing 655500, China
CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China
CAS Center for Excellence in Comparative Planetology, Anhui Mengcheng Geophysics National Observation and Research Station, University of Science and Technology of China, Hefei, China
National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, China
Kunming Electro-magnetic Environment Observation and Research Station, Qujing 655500, China
CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China
CAS Center for Excellence in Comparative Planetology, Anhui Mengcheng Geophysics National Observation and Research Station, University of Science and Technology of China, Hefei, China
CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China
CAS Center for Excellence in Comparative Planetology, Anhui Mengcheng Geophysics National Observation and Research Station, University of Science and Technology of China, Hefei, China
Hefei National Laboratory, University of Science and Technology of China, Hefei, China
Collaborate Innovation Center of Astronautical Science and Technology, Harbin 150001, China
Iain M. Reid
ATRAD Pty Ltd., Adelaide, SA 5032, Australia
School of Physical Sciences, University of Adelaide, Adelaide, SA 5005, Australia
Jianfei Wu
CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China
CAS Center for Excellence in Comparative Planetology, Anhui Mengcheng Geophysics National Observation and Research Station, University of Science and Technology of China, Hefei, China
Hailun Ye
CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China
CAS Center for Excellence in Comparative Planetology, Anhui Mengcheng Geophysics National Observation and Research Station, University of Science and Technology of China, Hefei, China
Jian Li
CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China
CAS Center for Excellence in Comparative Planetology, Anhui Mengcheng Geophysics National Observation and Research Station, University of Science and Technology of China, Hefei, China
Zonghua Ding
National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, China
Kunming Electro-magnetic Environment Observation and Research Station, Qujing 655500, China
Jinsong Chen
National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, China
Kunming Electro-magnetic Environment Observation and Research Station, Qujing 655500, China
Guozhu Li
Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
Yaoyu Tian
National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, China
Boyuan Chang
National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, China
Jiajing Wu
National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, China
Lei Zhao
National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, China
Kunming Electro-magnetic Environment Observation and Research Station, Qujing 655500, China
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Cited
4 citations as recorded by crossref.
- Major Advances in Aerospace Transition Zone Atmospheric Dynamics Research Z. SHENG et al.
- Migrating diurnal tide anomalies during QBO disruptions in 2016 and 2020: morphology and mechanism S. Liu et al.
- Investigating MLT response to active geomagnetic conditions using WACCM-X simulations, Wuhan meteor radar and SABER observations A. Mahmoudian et al.
- On the recent biennial variability of the lower stratospheric water vapor R. Dutta & S. Sridharan
4 citations as recorded by crossref.
- Major Advances in Aerospace Transition Zone Atmospheric Dynamics Research Z. SHENG et al.
- Migrating diurnal tide anomalies during QBO disruptions in 2016 and 2020: morphology and mechanism S. Liu et al.
- Investigating MLT response to active geomagnetic conditions using WACCM-X simulations, Wuhan meteor radar and SABER observations A. Mahmoudian et al.
- On the recent biennial variability of the lower stratospheric water vapor R. Dutta & S. Sridharan
Saved (final revised paper)
Latest update: 03 May 2026
Short summary
We present the impact of quasi-biennial oscillation (QBO) disruption events on diurnal tides over the low- and mid-latitude MLT region observed by a meteor radar chain. By using a global atmospheric model and reanalysis data, it is found that the stratospheric QBO winds can affect the mesospheric diurnal tides by modulating the subtropical ozone variability in the upper stratosphere and the interaction between tides and gravity waves in the mesosphere.
We present the impact of quasi-biennial oscillation (QBO) disruption events on diurnal tides...
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