Atmospheric turbulence decay during the solar total eclipse of 11 August 1999

被引:29
|
作者
Anfossi, D [1 ]
Schayes, G
Degrazia, G
Goulart, A
机构
[1] CNR, Ist Sci Atmosfera & Clima, I-10126 Turin, Italy
[2] UCL, Inst Astron & Geophys, Louvain, Belgium
[3] Univ Fed Santa Maria, Dept Fis, BR-97119900 Santa Maria, RS, Brazil
[4] URI, Dept Ciencias Exatas & Terra, Santo Angelo, Brazil
关键词
solar eclipse; turbulence decay; wind measurements;
D O I
10.1023/B:BOUN.0000016491.28111.43
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
The studies of turbulence decay were based in the past on measurements carried out in neutrally stratified wind tunnels and, more recently, on large-eddy simulation runs. Here the atmospheric turbulence decay process during the solar total eclipse of 11 August 1999 is examined. Thus a rapid transition from convective boundary-layer turbulence to that of a neutral or slightly stable one is considered. A u-v-w propeller anemometer and a fast response temperature sensor located in northern France on top of a 9-m mast recorded the turbulence observations. The measurements, in terms of turbulent kinetic energy decay with time, were found to be in good agreement with those prescribed by a theoretical model of turbulence decay recently proposed. In particular, it was found that the exponent of the power law describing the decay process has the value -2.
引用
收藏
页码:301 / 311
页数:11
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