Light Propagation in Turbulent Media
Abstract
First, we make a revision of the up-to-date Passive Scalar Fields properties: also, the refractive index is among them. Afterwards, we formulated the properties that make the family of `isotropic' fractional Brownian motion (with parameter H) a good candidate to simulate the turbulent refractive index. Moreover, we obtained its fractal dimension which matches the estimated by Constantin for passive scalar, and thus the parameter H determines the state of the turbulence. Next, using a path integral velocity representation, with the Markovian model, to calculate the effects of the turbulence over a system of grids. Finally, with the tools of Stochastic Calculus for fractional Brownian motions we studied the ray-equation coming from the Geometric Optics in the turbulent case. Our analysis covers those cases where average temperature gradients are relevant.
Cite
@article{arxiv.physics/0307144,
title = {Light Propagation in Turbulent Media},
author = {Dario G. Perez},
journal= {arXiv preprint arXiv:physics/0307144},
year = {2007}
}
Comments
172 pages, 10 figures, PhD thesis (translated to English from the original Spanish version)