We explain discrepancies in comparing estimations of the refractive-index structure constant Cn2 in clear air by means of different techniques by taking into account atmospheric intermittency effects. We formulate a model of C,2 in intermittent turbulence on the basis of the Tatarskii theory, and we calculate the mean value of Cn2 through a probabilistic approach. We deduce a factor, which gives a measure of the statistical reduction of turbulence that is due to intermittency, within the model framework. A procedure for estimating the mean value of Cn2 from data of a specific radiosonde observation is illustrated
New analytical models of the spatial power spectra of temperature fluctuations and refractive-index ...
The alternative Bendersky, Kopeika, and Blaunstein (BKB) model of measuring the refractive structure...
We present a method of data reduction and analysis that has been developed for a novel experiment to...
The refractive-index structure parameter C2, defined from [n(x)- n(x + r)]2 = Cn2r"3 (1.1) is a...
Analytical models of the spatial power spectra of temperature fluctuations and refractive index fluc...
In order to quantitatively determine the strength of atmospheric turbulence mostly scintillometers a...
We present results from an experiment to estimate the parameters of homogeneous, isotropic optical t...
The knowledge of atmospheric refractive-index structure constant (Cn2) profiles is fundamental to de...
The structure constant of the atmospheric refractive index is used for characterizing the turbulence...
This work is dedicated to structural parameter of the refractive index in the atmosphere Cn2 and his...
Estimates of the performance of an imager working in a turbulent atmosphere can often be obtained if...
The structure parameter of refractive index of air (Cn2) is the basic parameter derived from the sci...
The aim of this work is to examine theoretical knowledge of the refractive index structure parameter...
Current theories of stellar scintillation and astronomical seeing suppose that there is a disturbed ...
Atmospheric turbulence has significant impairments on the operation of Free-Space Optical (FSO) comm...
New analytical models of the spatial power spectra of temperature fluctuations and refractive-index ...
The alternative Bendersky, Kopeika, and Blaunstein (BKB) model of measuring the refractive structure...
We present a method of data reduction and analysis that has been developed for a novel experiment to...
The refractive-index structure parameter C2, defined from [n(x)- n(x + r)]2 = Cn2r"3 (1.1) is a...
Analytical models of the spatial power spectra of temperature fluctuations and refractive index fluc...
In order to quantitatively determine the strength of atmospheric turbulence mostly scintillometers a...
We present results from an experiment to estimate the parameters of homogeneous, isotropic optical t...
The knowledge of atmospheric refractive-index structure constant (Cn2) profiles is fundamental to de...
The structure constant of the atmospheric refractive index is used for characterizing the turbulence...
This work is dedicated to structural parameter of the refractive index in the atmosphere Cn2 and his...
Estimates of the performance of an imager working in a turbulent atmosphere can often be obtained if...
The structure parameter of refractive index of air (Cn2) is the basic parameter derived from the sci...
The aim of this work is to examine theoretical knowledge of the refractive index structure parameter...
Current theories of stellar scintillation and astronomical seeing suppose that there is a disturbed ...
Atmospheric turbulence has significant impairments on the operation of Free-Space Optical (FSO) comm...
New analytical models of the spatial power spectra of temperature fluctuations and refractive-index ...
The alternative Bendersky, Kopeika, and Blaunstein (BKB) model of measuring the refractive structure...
We present a method of data reduction and analysis that has been developed for a novel experiment to...