In this study we demonstrate that we can provide forecasts of all the main astroclimatic
parameters (seeing, wavefront coherence time, isoplanatic angle, and ground-layer fraction) …

The present “state of the art” and the path to future progress in high-spatial-resolution
imaging interferometry is reviewed. The review begins with a treatment of the fundamentals …

We present an overview of the MOSE (MOdelling ESO Sites) project that aims to prove the
feasibility of the forecast of the classical atmospheric parameters (wind-speed intensity and …

One of the main goals of the feasibility study MOSE (MOdelling ESO Sites) is to evaluate the
performances of a method conceived to forecast the optical turbulence (OT) above the …

We present a comparison between in situ measurements and forecasted data at the
Observatorio del Roque de Los Muchachos. Forecasting is obtained with the Weather …

The methods to obtain atmospheric refractive index structure constant (Cn2) by instrument
measurement are limited spatially and temporally and they are more difficult and expensive …

Atmospheric turbulence is a primary concern for astronomers. Turbulence causes amplitude
and phase fluctuations in electromagnetic waves propagating through the atmosphere …

In preceding papers we have presented comparisons between simulated and measured
profiles above two of the best astronomical sites: Cerro Paranal (Chile)(Masciadri et …

We show results obtained from simulations of the optical turbulence (OT), provided by the
atmospheric non-hydrostatic Meso-Nh model applied to the astronomical site of Roque de …

We present a method for simultaneous measurement of the vertical distribution of the optical
turbulence strength and wind velocity in the Earth's atmosphere, based on an analysis of …