Resolving Lambertian surface orientation from fluctuating radiance
Name
resolving_lambertian JASA_2011.pdf
Size
429.08 KB
Format
Adobe PDF
Checksum (MD5)
9f3acabbd5a49a5c0ecbc164236b21ec
Author(s) •
Makris, Nicholas
Bertsatos, Ioannis
Date Issued
March 2011
Journal
Journal of the Acoustical Society of America
Publisher
American Institute of Physics
Citation
Makris, Nicholas C., and Ioannis Bertsatos. “Resolving Lambertian Surface Orientation from Fluctuating Radiance.” The Journal of the Acoustical Society of America 130, no. 3 (2011): 1222. © 2011 American Institute of Physics.
Version
Final published version
Abstract
A maximum likelihood method for estimating remote surface orientation from multi-static acoustic, optical, radar, or laser images is presented. It is assumed that the images are corrupted by signal-dependent noise, known as speckle, arising from complex Gaussian field fluctuations, and that the surface properties are effectively Lambertian. Surface orientation estimates for a single sample are shown to have biases and errors that vary dramatically depending on illumination direction. This is due to the signal-dependent nature of specklenoise and the nonlinear relationship between surface orientation, illumination direction, and fluctuating radiance. The minimum number of independent samples necessary for maximum likelihood estimates to become asymptotically unbiased and to attain the lower bound on resolution of classical estimation theory are derived, as are practical design thresholds.
MIT Department
Massachusetts Institute of Technology. Department of Mechanical Engineering
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
DOI of Published Version
https://doi.org/10.1121/1.3570949