MF radar observation of mean wind and tides of winter mesopause (80-98 km) region over Wuhan (30°N, 114°E)

被引:26
作者
Zhang, SD [1 ]
Yi, F
Hu, X
机构
[1] Wuhan Univ, Dept Elect Engn, Wuhan 430072, Hubei, Peoples R China
[2] Wuhan Univ, Lab Geosp Environm & Geodesy, Wuhan 430072, Hubei, Peoples R China
[3] Chinese Acad Sci, Wuhan Inst Phys & Math, Wuhan 430072, Hubei, Peoples R China
基金
中国国家自然科学基金;
关键词
ME radar observation; mesopause; mean wind; tides;
D O I
10.1016/j.jastp.2003.10.006
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Data obtained from the medium-frequency radar at Wuhan (30degreesN, 114degreesE) from 11 to 25 February and from 28 February to 13 March have been used to study the mean wind and tidal oscillations at mesopause (80-98 km) region over Wuhan in winter. The observed zonal and meridional mean winds show obvious temporal variation and usually decrease with the increasing heights. In most observational time, the zonal mean wind is eastward. A dynamic spectral analysis of disturbance amplitude illustrates a prominent peak at a period of 24 h at all heights and almost uninterrupted, and there are occasionally slightly strong semidiurnal and weak terdiurnal tidal disturbances, indicating that in the mid-latitude regions, the diurnal tide is the dominant tidal disturbance at mesopause in winter. The temporal variation of tidal amplitudes and their wave kinematical energies illustrates that there may be significant resonant interaction among the diurnal, semidiurnal and terdiurnal tides. A quantitative comparison with the global-scale wave model (GSWM) demonstrates that the observed diurnal and semidiurnal tidal amplitudes are less and larger than the results of GSWM-02, respectively. The essentially linear GSWM cannot predict the decrease of diurnal tidal amplitude at higher heights, which may be due to several possible nonlinear processes, such as wave-wave interaction and wave break. Although the height variations of tidal phases are consistently well with the predictions of GSWM, there are evident phase differences between our observation and the model. The profiles of the diurnal tidal phases show obvious decrease trend with the increasing height, indicating the observed diurnal tide is propagating upward. The vertical wavelength of the observed diurnal tide is estimated to be about 37 km, and the corresponding downward phase velocity is about 1.5 km(-1) h. (C) 2003 Elsevier Ltd. All rights reserved.
引用
收藏
页码:15 / 25
页数:11
相关论文
共 38 条
[1]   HIGH-LATITUDE TIDAL BEHAVIOR IN THE MESOSPHERE AND LOWER THERMOSPHERE [J].
AVERY, SK ;
VINCENT, RA ;
PHILLIPS, A ;
MANSON, AH ;
FRASER, GJ .
JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS, 1989, 51 (7-8) :595-608
[2]   Non-linear interactions between tides and planetary waves resulting in periodic tidal variability [J].
Beard, AG ;
Mitchell, NJ ;
Williams, PJS ;
Kunitake, M .
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 1999, 61 (05) :363-376
[3]   ON TIDAL VARIABILITY AND THE EXISTENCE OF PLANETARY WAVE-LIKE OSCILLATIONS IN THE UPPER THERMOSPHERE .2. NONLINEAR-INTERACTIONS AND GLOBAL-SCALE OSCILLATIONS [J].
CANZIANI, PO .
JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS, 1994, 56 (08) :913-930
[4]  
CEVOLANI G, 1992, ADV SPACE RES-SERIES, V12, P77, DOI 10.1016/0273-1177(92)90446-5
[5]   Bispectral analysis of mesosphere winds [J].
Clark, RR ;
Bergin, JS .
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 1997, 59 (06) :629-639
[6]  
FRITTS DC, 1994, J ATMOS SCI, V51, P2145, DOI 10.1175/1520-0469(1994)051<2145:MMATAT>2.0.CO
[7]  
2
[8]  
FRITTS DC, 1987, J ATMOS SCI, V44, P605, DOI 10.1175/1520-0469(1987)044<0605:MMFSAA>2.0.CO
[9]  
2
[10]   A comparison of optical and radar measurements of mesospheric winds and tides [J].
Greet, PA ;
Murphy, DJ ;
Vincent, R ;
Dyson, PL .
GEOPHYSICAL RESEARCH LETTERS, 2000, 27 (16) :2477-2480