Abstract
A fifty-five-element Hartmann wavefront sensor has been constructed using an array of lenses and an array of position sensing devices. Daytime measurements of ro (Fried’s seeing parameter), the wavefront tilt power spectrum, and the atmospheric phase structure function have been made by tracking the image motion of solar pores. Results are presented and compared to theoretical predictions.
© 1991 Optical Society of America
PDF ArticleMore Like This
Darryl J. Sanchez, Denis W. Oesch, and Patrick R. Kelly
PTu3E.2 Propagation Through and Characterization of Distributed Volume Turbulence (pcAOP) 2014
David Dayton, John Gonglewski, and Boris Venet
AMC3 Adaptive Optics for Large Telescopes (AOLT) 1992
Valeri A. Tartakovski and Vladimir P. ukin
AThC.2 Adaptive Optics (AO) 1996