Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Noise deconvolution from probability density in laser atmospheric scintillation

Not Accessible

Your library or personal account may give you access

Abstract

A deconvolution procedure to remove large uncorrelated noise is applied to probability density histograms of intensity fluctuations of a laser beam after propagating a 1200-m path through atmospheric turbulence. The data were collected by very small (0.04 mm2) apertures at NOAA/ERL/WPL during an experiment not requiring noise resolved measurements at small irradiance.1 Each signal histogram contains data from a 64-s total signal (laser, background and noise) measurement. Each so-called noise histogram contains data obtained in the subsequent 3.2-s with the laser screened off; it therefore includes noise and background. The noise was independent of the laser signal.1

© 1991 Optical Society of America

PDF Article
More Like This
Analysis of probability density functions for laser scintillations in a turbulent atmosphere

P. R. TAPSTER, A. R. WEEKS, P. N. PUSEY, and E. JAKEMAN
THK41 Conference on Lasers and Electro-Optics (CLEO:S&I) 1989

Probability densities of atmospheric optical scintillation observed with large apertures

Andreas Muschinski and David G. Voelz
PTh3C.3 Propagation Through and Characterization of Atmospheric and Oceanic Phenomena (pcAOP) 2019

Atmospheric Effects on 2.09μm Laser Radar Performance

Richard Richmond, Michael J Kavaya, and Sammy W Henderson
TuB2 Coherent Laser Radar (CLR) 1991

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.