International audienceThe Profiler of Moon Limb is a recent instrument dedicated to the monitoring of optical turbulence profile of the atmosphere. Fluctuations of the Moon or the Sun limb allow to evaluate the index refraction structure constant C 2 n (h) and the wavefront coherence outer scale L 0 (h) as a function of the altitude h. The atmosphere is split into 33 layers with an altitude resolution varying from 100m (at the ground) to 2km (in the upper atmosphere). Profiles are obtained every 3mn during daytime and nighttime. We report last advances on the instrument and present some results obtained at the Plateau de Calern (France)
International audienceThe optical turbulence measurement and characterization has become an essentia...
International audienceTo reach a high performance with an adaptive optics system, we need a calibrat...
International audienceThe optical turbulence measurement and characterization has become an essentia...
International audienceThe Profiler of Moon Limb is a recent instrument dedicated to the monitoring o...
International audienceThe Profiler of Moon Limb is a recent instrument dedicated to the monitoring o...
International audienceThe Profiler of Moon Limb is a recent instrument dedicated to the monitoring o...
Aims. Future extremely large telescopes will certainly be equipped with wide-field adaptiv...
International audienceThe futures large telescopes will be certainly equipped with Multi-Conjugate A...
International audienceWith the prospect of the next generation of ground-based telescopes, the extre...
International audienceWide-Field Adaptive Optics (WFAO) have been proposed for the next generation o...
The performance of large telescopes is directly related to the quality of the site. Of particular i...
International audienceTo reach a high performance with an adaptive optics system, we need a calibrat...
International audienceThe optical turbulence measurement and characterization has become an essentia...
International audienceTo reach a high performance with an adaptive optics system, we need a calibrat...
International audienceThe optical turbulence measurement and characterization has become an essentia...
International audienceThe optical turbulence measurement and characterization has become an essentia...
International audienceTo reach a high performance with an adaptive optics system, we need a calibrat...
International audienceThe optical turbulence measurement and characterization has become an essentia...
International audienceThe Profiler of Moon Limb is a recent instrument dedicated to the monitoring o...
International audienceThe Profiler of Moon Limb is a recent instrument dedicated to the monitoring o...
International audienceThe Profiler of Moon Limb is a recent instrument dedicated to the monitoring o...
Aims. Future extremely large telescopes will certainly be equipped with wide-field adaptiv...
International audienceThe futures large telescopes will be certainly equipped with Multi-Conjugate A...
International audienceWith the prospect of the next generation of ground-based telescopes, the extre...
International audienceWide-Field Adaptive Optics (WFAO) have been proposed for the next generation o...
The performance of large telescopes is directly related to the quality of the site. Of particular i...
International audienceTo reach a high performance with an adaptive optics system, we need a calibrat...
International audienceThe optical turbulence measurement and characterization has become an essentia...
International audienceTo reach a high performance with an adaptive optics system, we need a calibrat...
International audienceThe optical turbulence measurement and characterization has become an essentia...
International audienceThe optical turbulence measurement and characterization has become an essentia...
International audienceTo reach a high performance with an adaptive optics system, we need a calibrat...
International audienceThe optical turbulence measurement and characterization has become an essentia...