A previously presented method for modeling Kolmogorov phase fluctuations ov
er a finite aperture is both formalized and improved on. The method relies
on forming an initial low-resolution Kolmogorov phase screen from direct fa
ctorization of a covariance. The resolution of the screen is then increased
by a randomized interpolation to produce a Kolmogorov phase screen of the
desired size. The computational requirement is asymptotically proportional
to the number of points in the phase screen. (C) 1999 Optical Society of Am
erica.