Share Email Print

Proceedings Paper

Speckle Grain Noise In Heterodyne Technique For Holographic Interferometry And Speckle Photogrammetry
Author(s): Jin Seung Kim
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 analyze the ultimate accuracy of interference phase neasrement that can be achieved by using heterodyne technique in conjunction with interfering speckle fields. We show that the mean square fluctuation of the measured phase depends not only on the traditionally introduced scintillation noise but also on the spatially random arrangement of the speckles over the detector aperture (speckle grain noise). Scintillation noise arises because the two speckle fields are partially decorrelated, in which case the interference pattern does not become completely dark even when the two speckle fields are out-of-phase since destructive interference is not complete. However, even in the case of perfect correlation, intrinsic random noise is to be expected, since the position of the speckles over the detector is random and therefore the total signal exhibits statistical fluctuations, which we call speckle grain noise. Our formula show, as expected, that scintillation noise can be reduced by enlarging the detector aperture which, however, cannot be larger than half of an interfringe spacing. On the contrary speckle grain noise cannot be reduced by enlarging the detect& aperture since the effect of increased sampling is cancelled by the increased range of phase variation.

Paper Details

Date Published: 17 February 1987
PDF: 6 pages
Proc. SPIE 0814, Photomechanics and Speckle Metrology, (17 February 1987); doi: 10.1117/12.941725
Show Author Affiliations
Jin Seung Kim, Chonbuk National University (Republic of Korea)

Published in SPIE Proceedings Vol. 0814:
Photomechanics and Speckle Metrology
Fu-Pen Chiang, Editor(s)

© SPIE. Terms of Use
Back to Top