Share Email Print
cover

Proceedings Paper

Retrieving atmospheric turbulence features from differential laser tracking motion data
Author(s): Darío G. Pérez; Ángel Férnandez; Gustavo Funes; Damián Gulich; Luciano Zunino
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

We have previously introduced the Differential Laser Tracking Motion Meter (DLTMM) [Proc. SPIE 7476, 74760D (2009)] as a robust device to determine many optical parameters related to atmospheric turbulence. It consisted of two thin laser beams—whose separations can be modified—that propagate through convective air, then each random wandering was registered with position detectors, sampled at 800 Hz. The hypothesis that the analysis of differential coordinates is less affected by noise induced by mechanical vibration was tested. Although we detected a trend to the Kolmogorov’s power exponent with the turbulence increasing strength, we were unable to relate it to the Rytov variance. Also, analyzing the behaviour of the multi-fractal degree estimator (calculated by means of multi-fractal detrended fluctuation analysis, MFDFA) at different laser-beam separations for these differential series resulted in the appreciation of characteristic spatial scales; nevertheless, errors induced by the technique forbid an accurate comparison with scales estimated under more standard methods. In the present work we introduce both an improved experimental setup and refined analyses techniques that eliminate many of the uncertainties found in our previous study. A new version of the DLTMM employs cross-polarized laser beams that allows us to inspect more carefully distances in the range of the inner-scale, thus even superimposed beams can be discriminated. Moreover, in this experimental setup the convective turbulence produced by electrical heaters previously used was superseded by a chamber that replicates isotropic atmospheric turbulence—anisotropic turbulence is also reproducible. Therefore, we are able to replicate the same state of the turbulent flow, specified by Rytov variance, for every separation between beams through the course of the experience. In this way, we are able to study the change in our MFDFA quantifiers with different strengths of the turbulence, and their relation with better known optical quantities. The movements of the two laser beams are recorded at 6 kHz; this apparent oversampling is crucial for detecting the turbulence’s characteristics scales under improved MFDFA techniques. The estimated characteristic scales and multi-fractal nature detected by this experiment provides insight into the non-Gaussian nature of propagated light.

Paper Details

Date Published: 1 November 2012
PDF: 11 pages
Proc. SPIE 8535, Optics in Atmospheric Propagation and Adaptive Systems XV, 853508 (1 November 2012); doi: 10.1117/12.974652
Show Author Affiliations
Darío G. Pérez, Pontificia Univ. Católica de Valparaíso (Chile)
Ángel Férnandez, Pontificia Univ. Católica de Valparaíso (Chile)
Gustavo Funes, Ctr. de Investigaciones Opticas (Argentina)
Damián Gulich, Ctr. de Investigaciones Opticas (Argentina)
Luciano Zunino, Ctr. de Investigaciones Opticas (Argentina)
Univ. Nacional de la Plata (Argentina)


Published in SPIE Proceedings Vol. 8535:
Optics in Atmospheric Propagation and Adaptive Systems XV
Karin Stein; John Gonglewski, Editor(s)

© SPIE. Terms of Use
Back to Top