Correlations of the phase gradients of the light wave propagating in a turbulent medium in the regime of weak scintillations
V. A. Bogachev, I. V. Kolokolov, V. V. Lebedev, A. V. Nemtseva, F. A. Starikov
TL;DR
The paper addresses how atmospheric turbulence affects the phase of a monochromatic beam in the weak scintillation regime, focusing on the off-diagonal phase-gradient correlation $Q_{xy}$ that is insensitive to the outer scale $L_0$. It uses direct numerical simulations with a chain of phase screens and a parabolic diffraction model to compute the pair correlations of the log-envelope $\eta=\ln(\Psi/\Psi_0)$ and their gradients, comparing against analytic expressions from Ref. $KLS25$ and related work. Findings show that the zeroth-order expression for $Q_{\alpha\beta}$ agrees with simulations for $\sigma_R^2$ up to about 0.5, and that $Q_{xy}$ exhibits a maximum at $r^\ast \approx 1.66 (\sigma_R^2)^{3/5} r_0$ independent of $L_0$, confirming uniform perturbation theory up to this regime. The results have practical implications for adaptive optics and turbulence diagnostics, suggesting that off-diagonal phase-gradient statistics can be used to estimate the Fried parameter $r_0$ and validate perturbative models, with planned experimental validation and extensions to non-Kolmogorov turbulence.
Abstract
We investigate numerically correlation functions of the phase of light waves that propagate through turbulent media. Special attention is paid to the off-diagonal component of the correlation function of the phase gradients which is insensitive to the outer scale of turbulence. The results of our simulations are in a good agreement with the analytical expressions obtained in Ref. \cite{KLS25}. Thus, we numerically confirm expectations based on uniformity of the perturbation theory for the logarithm of the envelope.
