Atmospheric turbulence has been confirmed as the primary source affecting the quality of
ground-based telescope image. To reduce the effect of atmosphere, a good site should be …

The forecast for atmospheric and turbulence conditions above astronomical observatories is
of interest to the astronomical community because it allows observations to be planned with …

The refractive index structure constant (C n 2) is a key parameter used in describing the
influence of turbulence on laser transmissions in the atmosphere. Three different methods …

In solar observations, the vertical distribution of turbulence can be detected with a
multidirectional Shack–Hartmann wavefront sensor, based on SLODAR or S-DIMM+. By …

Adaptive optics (AO) systems are an essential part of large astronomical telescopes and
laser complexes operating through the atmosphere. Each AO system is individually …

Real time characterization of atmospheric turbulence using speckle texture - IOPscience This
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Free Space Optical (FSO) communication is an excellent tool for high-speed information
transmission across a wide range of applications. It is now a key technology to overcome the …

A backpropagation neural network (BPNN) approach is proposed for the forecasting and
verification of optical turbulence profiles in the offshore atmospheric boundary layer. To …

For the new generation of Extremely Large Telescopes the knowledge of atmospheric
turbulence conditions is become an information of primary importance to design and …

We present a method to develop a turbulence emulation bench for low-Earth-orbit satellite-to-
ground optical communication links under strong turbulence. We provide guidelines to …