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Article Contents
1 Introduction
2 A model of the phase screen
3 General characteristics of the temperature and phase turbulent spectra
4 Spatial power spectral density
5 The variance of differential image motion averaged with respect to the wind and baseline orientations
6 Measurements in a specially selected direction
7 Using $\vec{r_0}$ and $\vec{\sigma _{30}}$ for calibration of $\vec \Delta$ at ill-defined $\vec{p}$
8 Conclusions
References

Copyright ESO 2002
Published by EDP Sciences