Titlebook: Boundary Layer Studies and Applications; A Special Issue of B R. E. Munn Book 1989 Kluwer Academic Publishers 1989 Meteorology.Scale.Wind s

facetious

庇護(hù)

F. Creuzet,G. Creuzet,B. Hamzic,D. Jéromeg at the top of a strongly stratified nocturnal inversion layer as observed by fast response aircraft data. The spatial variation of the coefficients of the principal components identify regular coherent structures with mainly horizontal motions. Conditional sampling is formulated in terms of this s

ATOPY

Low-Dimensional Cooperative Phenomenaements have recently been undertaken to attempt to widen the scope of applicability of such measurements. However, because of the intermittency of turbulent transfer, flux measurements must be averaged over long periods of time or long distances to give reproducible results. This requirement makes i

使虛弱

Huguette Launois,Halina Niedobapeed and air temperature over the ocean in the mesoscale frequency range were studied. The averaged composite spectrum of wind speed for the whole period shows the existence of a spectral gap in the frequency range from 10. to 5 × 10. Hz. However, significant peaks in this range are often seen in pa

ALERT

鴿子

https://doi.org/10.1007/978-1-4899-7031-2ls described by Nieuwstadt (1984, 1985) and Sorbjan (1986) and the numerical model of Duynkerke and Driedonks (1987). These theoretical profiles are compared with observed profiles from the meteorological mast at Cabauw, The Netherlands. From the observations, it is found that .. is large in the sur

BABY

Huguette Launois,Halina Niedobaese experiments generally exhibit an inertial subrange at high frequencies with a slope of ?5/3 and indicate peak energy at a time period of about 50 to 100s. These periods of peak energy are a factor of two to five less than those for the peak of the wind speed fluctuation (.’ or .’) spectra. A gen

作繭自縛

Exciton Mechanism of Superconductivity,tion of the spectral tensor Φ.(.) for isotropic turbulence and we show how in the limit of isotropy, Φ.(.) becomes equal to Φ.(.). Whereas Φ.(.) is determined entirely by one scalar function of . = |.|, namely the energy spectrum, we need three independent scalar functions of . to specify Φ.(.). We

Somber

FIS