As of today, Laser Guide Star adaptive optics can not measure the image motion induced by atmospheric turbulence. In this paper we review one of the proposed methods, never tested: the time-delay method. We will look at its application for the 1m class CaNaPy system, for the 8m class systems and potentially for extremely large telescopes. ESO and ESA are collaborating in this R&D, creating the CaNaPy-LASCA LGS-AO facility for both, Astrophysics and Optical Communications field experiments. We present the concept, its optimal setup, the potential difficulties of the time-delay method as well as the numerical simulations results when retrieving the atmospheric tip-tilt, for different telescope diameters, including the 8m+ class telescopes.
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