Mazzoni, TommasoTommasoMazzoniBUSONI, LORENZOLORENZOBUSONIBONAGLIA, MARCOMARCOBONAGLIAESPOSITO, SimoneSimoneESPOSITO2021-01-072021-01-072016978151060197097815106019870277-786Xhttp://hdl.handle.net/20.500.12386/29595ARGOS is the Ground Layer Adaptive Optics system of the Large Binocular Telescope, it uses three Laser Guide Stars, generated by Rayleigh backscattered light of pulsed lasers. Three Shack-Hartmann WFS measure the wavefront distortion in the Ground Layer. The SLOpe Detection And Ranging (SLODAR) is a method used to measure the turbulence profiles. Cross correlation of wavefronts gradient from multiple stars is used to estimate the relative strengths of turbulent layers at different altitudes. We present here the results on sky of the SLODAR profile on ARGOS.ELETTRONICOenConference paper10.1117/12.22342682-s2.0-85002243986000387429700110https://www.spiedigitallibrary.org/conference-proceedings-of-spie/9909/1/Atmospheric-turbulence-profiling-using-the-SLODAR-technique-with-ARGOS-at/10.1117/12.2234268.short2016SPIE.9909E..3RMFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_17 Instrumentation – telescopes, detectors and techniques