WHU VHF radar observations of the diurnal tide and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N), China
The diurnal tide (DT) and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N) were studied based on the newly established Wuhan University (WHU) VHF radar observations with the height intervals of 0.145 km (below 9 km) and 0.58 km (above 9 km) in the whole year of 2012....
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Copernicus Publications
2015-07-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/33/865/2015/angeo-33-865-2015.pdf |
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DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
C. Huang C. Huang C. Huang C. Huang S. Zhang S. Zhang S. Zhang S. Zhang Q. Zhou F. Yi F. Yi F. Yi F. Yi K. Huang K. Huang K. Huang K. Huang Y. Gong Y. Gong Y. Gong Y. Gong Y. Zhang Q. Gan Q. Gan Q. Gan Q. Gan |
spellingShingle |
C. Huang C. Huang C. Huang C. Huang S. Zhang S. Zhang S. Zhang S. Zhang Q. Zhou F. Yi F. Yi F. Yi F. Yi K. Huang K. Huang K. Huang K. Huang Y. Gong Y. Gong Y. Gong Y. Gong Y. Zhang Q. Gan Q. Gan Q. Gan Q. Gan WHU VHF radar observations of the diurnal tide and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N), China Annales Geophysicae |
author_facet |
C. Huang C. Huang C. Huang C. Huang S. Zhang S. Zhang S. Zhang S. Zhang Q. Zhou F. Yi F. Yi F. Yi F. Yi K. Huang K. Huang K. Huang K. Huang Y. Gong Y. Gong Y. Gong Y. Gong Y. Zhang Q. Gan Q. Gan Q. Gan Q. Gan |
author_sort |
C. Huang |
title |
WHU VHF radar observations of the diurnal tide and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N), China |
title_short |
WHU VHF radar observations of the diurnal tide and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N), China |
title_full |
WHU VHF radar observations of the diurnal tide and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N), China |
title_fullStr |
WHU VHF radar observations of the diurnal tide and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N), China |
title_full_unstemmed |
WHU VHF radar observations of the diurnal tide and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N), China |
title_sort |
whu vhf radar observations of the diurnal tide and its variability in the lower atmosphere over chongyang (114.14° e, 29.53° n), china |
publisher |
Copernicus Publications |
series |
Annales Geophysicae |
issn |
0992-7689 1432-0576 |
publishDate |
2015-07-01 |
description |
The diurnal tide (DT) and its variability in the lower atmosphere over
Chongyang (114.14° E, 29.53° N) were studied based on the
newly established Wuhan University (WHU) VHF radar observations with the
height intervals of 0.145 km (below 9 km) and 0.58 km (above 9 km) in the
whole year of 2012. We find that the DT was the dominant tidal component and
showed remarkable height and season variations. A prominent seasonally
dependent height variability characteristic is that maximum DT amplitude
usually occurs around 6 km in the winter and spring months, which might be
due to the tidal wave energy concentration arising from the reflections from
the strong eastward tropospheric jet around 13 km and the ground surface.
Our results suggest that the background wind is a crucial cause for height
variability and seasonal variability of DT. In April 2012, a notable
strengthening of DT is observed. Meanwhile, the
significant higher harmonics of
tides, i.e., the semidiurnal, terdiurnal, and even quarterdiurnal tides, can
also be observed, which has seldom been reported. Interestingly, these four
tidal components displayed consistent short-term variability, implying that
they were excited by the same dramatically varying tidal source. In addition,
we identified two symptoms of the coupling of DT and planetary waves (PWs),
which can also lead to the short-term DT variability. One is the sum and
difference interactions between DT and PWs, causing the tidal amplitude
short-term variability as a consequence of the energy exchange among the
interacting waves. The other one is the modulation of DT by PWs, leading to
that the amplitude of DT varies with the periods of the PWs. |
url |
https://www.ann-geophys.net/33/865/2015/angeo-33-865-2015.pdf |
work_keys_str_mv |
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doaj-bbc117919e494101abd1e4da4daf2d5a2020-11-24T23:55:23ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762015-07-013386587410.5194/angeo-33-865-2015WHU VHF radar observations of the diurnal tide and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N), ChinaC. Huang0C. Huang1C. Huang2C. Huang3S. Zhang4S. Zhang5S. Zhang6S. Zhang7Q. Zhou8F. Yi9F. Yi10F. Yi11F. Yi12K. Huang13K. Huang14K. Huang15K. Huang16Y. Gong17Y. Gong18Y. Gong19Y. Gong20Y. Zhang21Q. Gan22Q. Gan23Q. Gan24Q. Gan25School of Electronic Information, Wuhan University, Wuhan, Hubei, ChinaKey Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan, Hubei, ChinaState Observatory for Atmospheric Remote Sensing, Wuhan, Hubei, ChinaState Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan, Hubei, ChinaSchool of Electronic Information, Wuhan University, Wuhan, Hubei, ChinaKey Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan, Hubei, ChinaState Observatory for Atmospheric Remote Sensing, Wuhan, Hubei, ChinaState Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan, Hubei, ChinaElectrical and Computer Engineering Department, Miami University, Oxford, Ohio, USASchool of Electronic Information, Wuhan University, Wuhan, Hubei, ChinaKey Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan, Hubei, ChinaState Observatory for Atmospheric Remote Sensing, Wuhan, Hubei, ChinaState Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan, Hubei, ChinaSchool of Electronic Information, Wuhan University, Wuhan, Hubei, ChinaKey Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan, Hubei, ChinaState Observatory for Atmospheric Remote Sensing, Wuhan, Hubei, ChinaState Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan, Hubei, ChinaSchool of Electronic Information, Wuhan University, Wuhan, Hubei, ChinaKey Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan, Hubei, ChinaState Observatory for Atmospheric Remote Sensing, Wuhan, Hubei, ChinaState Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan, Hubei, ChinaCollege of Hydrometeorology, Nanjing University of Information Science and Technology, Nanjing, ChinaSchool of Electronic Information, Wuhan University, Wuhan, Hubei, ChinaKey Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan, Hubei, ChinaState Observatory for Atmospheric Remote Sensing, Wuhan, Hubei, ChinaState Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan, Hubei, ChinaThe diurnal tide (DT) and its variability in the lower atmosphere over Chongyang (114.14° E, 29.53° N) were studied based on the newly established Wuhan University (WHU) VHF radar observations with the height intervals of 0.145 km (below 9 km) and 0.58 km (above 9 km) in the whole year of 2012. We find that the DT was the dominant tidal component and showed remarkable height and season variations. A prominent seasonally dependent height variability characteristic is that maximum DT amplitude usually occurs around 6 km in the winter and spring months, which might be due to the tidal wave energy concentration arising from the reflections from the strong eastward tropospheric jet around 13 km and the ground surface. Our results suggest that the background wind is a crucial cause for height variability and seasonal variability of DT. In April 2012, a notable strengthening of DT is observed. Meanwhile, the significant higher harmonics of tides, i.e., the semidiurnal, terdiurnal, and even quarterdiurnal tides, can also be observed, which has seldom been reported. Interestingly, these four tidal components displayed consistent short-term variability, implying that they were excited by the same dramatically varying tidal source. In addition, we identified two symptoms of the coupling of DT and planetary waves (PWs), which can also lead to the short-term DT variability. One is the sum and difference interactions between DT and PWs, causing the tidal amplitude short-term variability as a consequence of the energy exchange among the interacting waves. The other one is the modulation of DT by PWs, leading to that the amplitude of DT varies with the periods of the PWs.https://www.ann-geophys.net/33/865/2015/angeo-33-865-2015.pdf |