Articles | Volume 35, issue 1
https://doi.org/10.5194/angeo-35-107-2017
© Author(s) 2017. 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-35-107-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Vertical wavenumber spectra of three-dimensional winds revealed by radiosonde observations at midlatitude
Shao Dong Zhang
CORRESPONDING AUTHOR
School of Electronic Information, Wuhan University, Wuhan, Hubei,
People's Republic of China
Key Laboratory of Geospace Environment and Geodesy, Ministry of
Education, Wuhan, Hubei, People's Republic of China
State Key Laboratory of Information Engineering in Surveying, Mapping
and Remote Sensing, Wuhan University, Wuhan, People's Republic of China
Chun Ming Huang
School of Electronic Information, Wuhan University, Wuhan, Hubei,
People's Republic of China
Key Laboratory of Geospace Environment and Geodesy, Ministry of
Education, Wuhan, Hubei, People's Republic of China
Kai Ming Huang
School of Electronic Information, Wuhan University, Wuhan, Hubei,
People's Republic of China
Key Laboratory of Geospace Environment and Geodesy, Ministry of
Education, Wuhan, Hubei, People's Republic of China
Ye Hui Zhang
College of Hydrometeorology, Nanjing University of Information
Science and Technology, Nanjing, People's Republic of China
Yun Gong
School of Electronic Information, Wuhan University, Wuhan, Hubei,
People's Republic of China
Key Laboratory of Geospace Environment and Geodesy, Ministry of
Education, Wuhan, Hubei, People's Republic of China
School of Electronic Information, Wuhan University, Wuhan, Hubei,
People's Republic of China
Key Laboratory of Geospace Environment and Geodesy, Ministry of
Education, Wuhan, Hubei, People's Republic of China
Related authors
Jia Shao, Jian Zhang, Wuke Wang, Shaodong Zhang, Tao Yu, and Wenjun Dong
Atmos. Chem. Phys., 23, 12589–12607, https://doi.org/10.5194/acp-23-12589-2023, https://doi.org/10.5194/acp-23-12589-2023, 2023
Short summary
Short summary
Kelvin–Helmholtz instability (KHI) is indicated by the critical value of the Richardson (Ri) number, which is usually predicted to be 1/4. Compared to high-resolution radiosondes, the threshold value of Ri could be approximated as 1 rather than 1/4 when using ERA5-based Ri as a proxy for KHI. The occurrence frequency of subcritical Ri exhibits significant seasonal cycles over all climate zones and is closely associated with gravity waves and background flows.
Zheng Ma, Yun Gong, Shaodong Zhang, Qiao Xiao, Chunming Huang, and Kaiming Huang
Atmos. Chem. Phys., 22, 13725–13737, https://doi.org/10.5194/acp-22-13725-2022, https://doi.org/10.5194/acp-22-13725-2022, 2022
Short summary
Short summary
We present a novel method to measure the amplitudes of traveling quasi-5-day oscillations (Q5DOs) in the middle atmosphere during sudden stratospheric warming events based on satellite observations. Simulations and observations demonstrate that the previously reported traveling Q5DOs might be contaminated by stationary planetary waves (SPWs). The new fitting method is developed by inhibiting the effect of a rapid and large change in SPWs.
Xiansi Huang, Kaiming Huang, Hao Cheng, Shaodong Zhang, Wei Cheng, Chunming Huang, and Yun Gong
Atmos. Chem. Phys. Discuss., https://doi.org/10.5194/acp-2022-407, https://doi.org/10.5194/acp-2022-407, 2022
Revised manuscript not accepted
Short summary
Short summary
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.
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
Short summary
Short summary
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.
Minkang Du, Kaiming Huang, Shaodong Zhang, Chunming Huang, Yun Gong, and Fan Yi
Atmos. Chem. Phys., 21, 13553–13569, https://doi.org/10.5194/acp-21-13553-2021, https://doi.org/10.5194/acp-21-13553-2021, 2021
Short summary
Short summary
El Niño has an important influence on climate systems. There are obviously negative water vapor anomalies from radiosonde observations in the tropical western Pacific during El Niño. The tropical Hadley, Walker, and monsoon circulation variations are revealed to play different roles in the observed water vapor anomaly in different types of El Niños. The Walker (monsoon) circulation anomaly made a major contribution in the 2015/16 (2009/10) strong eastern Pacific (central Pacific) El Niño event.
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
Atmos. Meas. Tech., 13, 5697–5713, https://doi.org/10.5194/amt-13-5697-2020, https://doi.org/10.5194/amt-13-5697-2020, 2020
Feilong Chen, Gang Chen, Yufang Tian, Shaodong Zhang, Kaiming Huang, Chen Wu, and Weifan Zhang
Ann. Geophys., 37, 631–643, https://doi.org/10.5194/angeo-37-631-2019, https://doi.org/10.5194/angeo-37-631-2019, 2019
Short summary
Short summary
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.
Jian Zhang, Shao Dong Zhang, Chun Ming Huang, Kai Ming Huang, Ye Hui Zhang, Yun Gong, and Quan Gan
Ann. Geophys. Discuss., https://doi.org/10.5194/angeo-2018-114, https://doi.org/10.5194/angeo-2018-114, 2018
Publication in ANGEO not foreseen
Short summary
Short summary
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.
Feilong Chen, Gang Chen, Chunhua Shi, Yufang Tian, Shaodong Zhang, and Kaiming Huang
Ann. Geophys., 36, 1403–1417, https://doi.org/10.5194/angeo-36-1403-2018, https://doi.org/10.5194/angeo-36-1403-2018, 2018
Short summary
Short summary
Downward stratospheric intrusions are well known as an important source of tropospheric ozone. In the light of the present understanding, several unanswered questions remain regarding the use of VHF radars to identify stratospheric intrusions. Our study found that the radar-observed strong downdrafts preceding the rapid tropopause ascent are a strong diagnostic for possible intrusions. This will have important implications for air-quality monitoring and long-term estimation of troposphere ozone.
Yue Jia, Shao Dong Zhang, Fan Yi, Chun Ming Huang, Kai Ming Huang, Yun Gong, and Quan Gan
Ann. Geophys., 34, 331–345, https://doi.org/10.5194/angeo-34-331-2016, https://doi.org/10.5194/angeo-34-331-2016, 2016
K. M. Huang, A. Z. Liu, S. D. Zhang, F. Yi, C. M. Huang, Q. Gan, Y. Gong, Y. H. Zhang, and R. Wang
Ann. Geophys., 33, 1321–1330, https://doi.org/10.5194/angeo-33-1321-2015, https://doi.org/10.5194/angeo-33-1321-2015, 2015
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
Short summary
Short summary
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
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
Zirui Zhang, Kaiming Huang, Fan Yi, Fuchao Liu, Jian Zhang, and Yue Jia
EGUsphere, https://doi.org/10.5194/egusphere-2024-933, https://doi.org/10.5194/egusphere-2024-933, 2024
Short summary
Short summary
The CBLH is related to our health due to its crucial role in pollutant dispersion. The vertical velocity from MMCR can capture the CBLH evolution, especially the initial stage of CBLH rise and the final stage of CBLH dissipation due to little blind range and less impact by residual layer, thus the MMCR observation can clearly identify the diurnal evolution of CBLH. The study shows that the CBLH has an obvious seasonal feature, and is affected by radiation, humidity, cloud and precipitation.
Jia Shao, Jian Zhang, Wuke Wang, Shaodong Zhang, Tao Yu, and Wenjun Dong
Atmos. Chem. Phys., 23, 12589–12607, https://doi.org/10.5194/acp-23-12589-2023, https://doi.org/10.5194/acp-23-12589-2023, 2023
Short summary
Short summary
Kelvin–Helmholtz instability (KHI) is indicated by the critical value of the Richardson (Ri) number, which is usually predicted to be 1/4. Compared to high-resolution radiosondes, the threshold value of Ri could be approximated as 1 rather than 1/4 when using ERA5-based Ri as a proxy for KHI. The occurrence frequency of subcritical Ri exhibits significant seasonal cycles over all climate zones and is closely associated with gravity waves and background flows.
Zheng Ma, Yun Gong, Shaodong Zhang, Qiao Xiao, Chunming Huang, and Kaiming Huang
Atmos. Chem. Phys., 22, 13725–13737, https://doi.org/10.5194/acp-22-13725-2022, https://doi.org/10.5194/acp-22-13725-2022, 2022
Short summary
Short summary
We present a novel method to measure the amplitudes of traveling quasi-5-day oscillations (Q5DOs) in the middle atmosphere during sudden stratospheric warming events based on satellite observations. Simulations and observations demonstrate that the previously reported traveling Q5DOs might be contaminated by stationary planetary waves (SPWs). The new fitting method is developed by inhibiting the effect of a rapid and large change in SPWs.
Xiansi Huang, Kaiming Huang, Hao Cheng, Shaodong Zhang, Wei Cheng, Chunming Huang, and Yun Gong
Atmos. Chem. Phys. Discuss., https://doi.org/10.5194/acp-2022-407, https://doi.org/10.5194/acp-2022-407, 2022
Revised manuscript not accepted
Short summary
Short summary
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.
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
Short summary
Short summary
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.
Minkang Du, Kaiming Huang, Shaodong Zhang, Chunming Huang, Yun Gong, and Fan Yi
Atmos. Chem. Phys., 21, 13553–13569, https://doi.org/10.5194/acp-21-13553-2021, https://doi.org/10.5194/acp-21-13553-2021, 2021
Short summary
Short summary
El Niño has an important influence on climate systems. There are obviously negative water vapor anomalies from radiosonde observations in the tropical western Pacific during El Niño. The tropical Hadley, Walker, and monsoon circulation variations are revealed to play different roles in the observed water vapor anomaly in different types of El Niños. The Walker (monsoon) circulation anomaly made a major contribution in the 2015/16 (2009/10) strong eastern Pacific (central Pacific) El Niño event.
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
Atmos. Meas. Tech., 13, 5697–5713, https://doi.org/10.5194/amt-13-5697-2020, https://doi.org/10.5194/amt-13-5697-2020, 2020
Feilong Chen, Gang Chen, Yufang Tian, Shaodong Zhang, Kaiming Huang, Chen Wu, and Weifan Zhang
Ann. Geophys., 37, 631–643, https://doi.org/10.5194/angeo-37-631-2019, https://doi.org/10.5194/angeo-37-631-2019, 2019
Short summary
Short summary
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.
Jian Zhang, Shao Dong Zhang, Chun Ming Huang, Kai Ming Huang, Ye Hui Zhang, Yun Gong, and Quan Gan
Ann. Geophys. Discuss., https://doi.org/10.5194/angeo-2018-114, https://doi.org/10.5194/angeo-2018-114, 2018
Publication in ANGEO not foreseen
Short summary
Short summary
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.
Feilong Chen, Gang Chen, Chunhua Shi, Yufang Tian, Shaodong Zhang, and Kaiming Huang
Ann. Geophys., 36, 1403–1417, https://doi.org/10.5194/angeo-36-1403-2018, https://doi.org/10.5194/angeo-36-1403-2018, 2018
Short summary
Short summary
Downward stratospheric intrusions are well known as an important source of tropospheric ozone. In the light of the present understanding, several unanswered questions remain regarding the use of VHF radars to identify stratospheric intrusions. Our study found that the radar-observed strong downdrafts preceding the rapid tropopause ascent are a strong diagnostic for possible intrusions. This will have important implications for air-quality monitoring and long-term estimation of troposphere ozone.
Yue Jia, Shao Dong Zhang, Fan Yi, Chun Ming Huang, Kai Ming Huang, Yun Gong, and Quan Gan
Ann. Geophys., 34, 331–345, https://doi.org/10.5194/angeo-34-331-2016, https://doi.org/10.5194/angeo-34-331-2016, 2016
K. M. Huang, A. Z. Liu, S. D. Zhang, F. Yi, C. M. Huang, Q. Gan, Y. Gong, Y. H. Zhang, and R. Wang
Ann. Geophys., 33, 1321–1330, https://doi.org/10.5194/angeo-33-1321-2015, https://doi.org/10.5194/angeo-33-1321-2015, 2015
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
Short summary
Short summary
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
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
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.
We present the first statistical results of vertical wind fluctuation spectra, which revealed a...