A method for reconstructing a diffraction-limited image from data consisting of many short-exposure turbulence degraded images is described. The results of a computer simulation of the method are presented. The method should prove useful for obtaining high-angular resolution images from large earth bound telescopes. The simulation indicates that the method may be applicable to astronomical objects as faint as ~11th magnitude.
© 1982 Optical Society of America
Original Manuscript: February 12, 1982
Published: September 1, 1982
John G. Walker, "Computer simulation of a method for object reconstruction from stellar speckle interferometry data," Appl. Opt. 21, 3132-3137 (1982)