Title
The Significance Of The Class Of K-Distributions
Abstract
The statistical fluctuations developed by an optical wave, after passing through atmospheric turbulence, have a non-Gaussian nature. The detected optical intensity appears to have two separate time scales of fluctuations. This paper discusses a plausible physical model for the turbulence scattering of an optical wave that would give rise to a two-time scale fluctuation. The K distribution, H-K distribution and I-K distribution are analyzed as to the possible scattering conditions, by turbulence, these distributions represent. © 1988 SPIE.
Publication Date
8-10-1988
Publication Title
Proceedings of SPIE - The International Society for Optical Engineering
Volume
926
Number of Pages
2-7
Document Type
Article; Proceedings Paper
Personal Identifier
scopus
DOI Link
https://doi.org/10.1117/12.945753
Copyright Status
Unknown
Socpus ID
0042055335 (Scopus)
Source API URL
https://api.elsevier.com/content/abstract/scopus_id/0042055335
STARS Citation
Phillips, Ronald L. and Andrews, Larry C., "The Significance Of The Class Of K-Distributions" (1988). Scopus Export 1980s. 289.
https://stars.library.ucf.edu/scopus1980/289