Articles | Volume 33, issue 10
https://doi.org/10.5194/angeo-33-1321-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-33-1321-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Observational evidence of quasi-27-day oscillation propagating from the lower atmosphere to the mesosphere over 20° N
K. M. Huang
School of Electronic Information, Wuhan University, Wuhan, China
State Observatory for Atmospheric Remote Sensing, Wuhan, China
A. Z. Liu
Department of Physical Science, Embry-Riddle Aeronautical University, Daytona Beach, Florida, USA
S. D. Zhang
CORRESPONDING AUTHOR
School of Electronic Information, Wuhan University, Wuhan, China
State Observatory for Atmospheric Remote Sensing, Wuhan, China
School of Electronic Information, Wuhan University, Wuhan, China
State Observatory for Atmospheric Remote Sensing, Wuhan, China
C. M. Huang
School of Electronic Information, Wuhan University, Wuhan, China
State Observatory for Atmospheric Remote Sensing, Wuhan, China
Q. Gan
School of Electronic Information, Wuhan University, Wuhan, China
State Observatory for Atmospheric Remote Sensing, Wuhan, China
Y. Gong
School of Electronic Information, Wuhan University, Wuhan, China
State Observatory for Atmospheric Remote Sensing, Wuhan, China
Y. H. Zhang
College of Hydrometeorology, Nanjing University of Information Science and Technology, Nanjing, China
R. Wang
SOA Key Laboratory for Polar Science, Polar Research Institute of China, Shanghai, China
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Short summary
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Using radar observations and reanalysis data for 9 years, we demonstrate clearly for the first time that resonant interactions between tides and annual and semiannual oscillations do occur in the mesosphere and lower thermosphere. The resonant matching conditions of frequency and wavenumber are exactly satisfied for the interacting triad. At some altitudes, the secondary waves are stronger than the tides, thus in tidal studies, the secondary waves may be mistaken for the tides if no carefully.
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Jianping Guo, Jian Zhang, Kun Yang, Hong Liao, Shaodong Zhang, Kaiming Huang, Yanmin Lv, Jia Shao, Tao Yu, Bing Tong, Jian Li, Tianning Su, Steve H. L. Yim, Ad Stoffelen, Panmao Zhai, and Xiaofeng Xu
Atmos. Chem. Phys., 21, 17079–17097, https://doi.org/10.5194/acp-21-17079-2021, https://doi.org/10.5194/acp-21-17079-2021, 2021
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The planetary boundary layer (PBL) is the lowest part of the troposphere, and boundary layer height (BLH) is the depth of the PBL and is of critical importance to the dispersion of air pollution. The study presents the first near-global BLH climatology by using high-resolution (5-10 m) radiosonde measurements. The variations in BLH exhibit large spatial and temporal dependence, with a peak at 17:00 local solar time. The most promising reanalysis product is ERA-5 in terms of modeling BLH.
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Lei Qiao, Gang Chen, Shaodong Zhang, Qi Yao, Wanlin Gong, Mingkun Su, Feilong Chen, Erxiao Liu, Weifan Zhang, Huangyuan Zeng, Xuesi Cai, Huina Song, Huan Zhang, and Liangliang Zhang
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Feilong Chen, Gang Chen, Yufang Tian, Shaodong Zhang, Kaiming Huang, Chen Wu, and Weifan Zhang
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Using the Beijing MST radar echo-power observations collected during the period November 2011–May 2017, the structure and variability of the tropopause over Xianghe, China (39.75° N, 116.96° E), was presented. Our comparison results showed a good agreement between the radar and thermal tropopauses during all seasons. In contrast, the consistency between the radar and dynamical tropopauses is poor during summer. Diurnal oscillation in tropopause height is commonly observed during all seasons.
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Short summary
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Turbulence dissipation rate has inter-annual variations and follows a lognormal distribution. The magnitudes of turbulence detected by radiosonde and radar are roughly comparable. Turbulence cannot predicted by instabilities well but trends to be vigorous under the instability condition. The propagating gravity waves in the lower atmosphere can enhance atmospheric instabilities, and the temporal variations of waves can roughly estimate the turbulence dissipation rate at different height.
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Short summary
Short summary
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Short summary
Short summary
We present the first statistical results of vertical wind fluctuation spectra, which revealed a very shallow spectral structure, with mean slopes of −0.58 and −0.23 in the troposphere and lower stratosphere, respectively. No existing spectral theories can comprehensively explain the observed three-dimensional wind spectra, indicating that the spectral features of atmospheric fluctuations are far from fully understood.
Yue Jia, Shao Dong Zhang, Fan Yi, Chun Ming Huang, Kai Ming Huang, Yun Gong, and Quan Gan
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Q. Gan, J. Yue, L. C. Chang, W. B. Wang, S. D. Zhang, and J. Du
Ann. Geophys., 33, 913–922, https://doi.org/10.5194/angeo-33-913-2015, https://doi.org/10.5194/angeo-33-913-2015, 2015
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The 6.5-day traveling planetary wave is able to impact the ionosphere/thermosphere via a dissipation mechanism. Ionospheric TEC and thermosphere O/N2 exhibit an apparent decrease as the result of extra meridional circulation induced by 6.5-day wave dissipation. Our work suggests that the modulation of E-dynamo is not the unique pathway through which planetary waves substantially influence the IT system.
C. Huang, S. Zhang, Q. Zhou, F. Yi, K. Huang, Y. Gong, Y. Zhang, and Q. Gan
Ann. Geophys., 33, 865–874, https://doi.org/10.5194/angeo-33-865-2015, https://doi.org/10.5194/angeo-33-865-2015, 2015
Short summary
Short summary
The diurnal tide and its variability in the lower atmosphere over Chongyang (114.14ºE,29.53ºN) were studied based on the newly established Wuhan University VHF radar observations in the whole year of 2012. We find that the diurnal tide was the dominant tidal component and showed remarkable height and season variations, as well as dramatic short-term variability.
S. D. Zhang, C. M. Huang, K. M. Huang, F. Yi, Y. H. Zhang, Y. Gong, and Q. Gan
Ann. Geophys., 32, 1129–1143, https://doi.org/10.5194/angeo-32-1129-2014, https://doi.org/10.5194/angeo-32-1129-2014, 2014
J.-S. Wang, Z. Chen, and C.-M. Huang
Ann. Geophys., 32, 563–569, https://doi.org/10.5194/angeo-32-563-2014, https://doi.org/10.5194/angeo-32-563-2014, 2014
K. M. Huang, S. D. Zhang, F. Yi, C. M. Huang, Q. Gan, Y. Gong, and Y. H. Zhang
Ann. Geophys., 32, 263–275, https://doi.org/10.5194/angeo-32-263-2014, https://doi.org/10.5194/angeo-32-263-2014, 2014
K. M. Huang, A. Z. Liu, S. D. Zhang, F. Yi, C. M. Huang, Q. Gan, Y. Gong, and Y. H. Zhang
Ann. Geophys., 31, 2039–2048, https://doi.org/10.5194/angeo-31-2039-2013, https://doi.org/10.5194/angeo-31-2039-2013, 2013
C. M. Huang, S. D. Zhang, F. Yi, K. M. Huang, Y. H. Zhang, Q. Gan, and Y. Gong
Ann. Geophys., 31, 1731–1743, https://doi.org/10.5194/angeo-31-1731-2013, https://doi.org/10.5194/angeo-31-1731-2013, 2013
Y. Y. Huang, S. D. Zhang, F. Yi, C. M. Huang, K. M. Huang, Q. Gan, and Y. Gong
Ann. Geophys., 31, 1061–1075, https://doi.org/10.5194/angeo-31-1061-2013, https://doi.org/10.5194/angeo-31-1061-2013, 2013