Starting with the Wigner distribution formulation for beam wave propagation in Hölder continuous non-Gaussian random refractive index fields we show that the wave beam regime naturally leads to the white-noise scaling limit and converges to a Gaussian white-noise model which is characterized by the martingale problem associated to a stochastic differential-integral equation of the Itô type. In the simultaneous geometrical optics the convergence to the Gaussian white-noise model for the Liouville equation is also established if the ultraviolet cutoff or the Fresnel number vanishes sufficiently slowly. The advantage of the Gaussian white-noise model is that its
n-point correlation functions are governed by closed form equations.
Communicated by P. Constantin
The research is supported in part by The Centennial Fellowship from American Mathematical Society, the UC Davis Chancellor
s Fellowship and U.S. National Science Foundation grant DMS 0306659.Acknowledgement I thank the referee for a careful reading of the manuscript and the suggestions which lead to improvement of the presentation. I also benefited from the inspiring program of the Mathematical Geophysics Summer School at Stanford University, 2002.