Abstract
We present a detailed investigation, qualitative and quantitative, on how the atmospheric turbulence with a non-Kolmogorov power spectrum affects the major statistics of stochastic electromagnetic beams, such as the spectral composition and the states of coherence and polarization. We suggest a detailed survey on how these properties evolve on propagation of beams generated by electromagnetic Gaussian Schell-model sources, depending on the fractal constant α of the atmospheric power spectrum.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 10650-10658 |
| Number of pages | 9 |
| Journal | Optics Express |
| Volume | 18 |
| Issue number | 10 |
| DOIs | |
| State | Published - May 10 2010 |
Fingerprint
ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics
Cite this
Second-order statistics of stochastic electromagnetic beams propagating through non-Kolmogorov turbulence. / Shchepakina, Elena; Korotkova, Olga.
In: Optics Express, Vol. 18, No. 10, 10.05.2010, p. 10650-10658.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Second-order statistics of stochastic electromagnetic beams propagating through non-Kolmogorov turbulence
AU - Shchepakina, Elena
AU - Korotkova, Olga
PY - 2010/5/10
Y1 - 2010/5/10
N2 - We present a detailed investigation, qualitative and quantitative, on how the atmospheric turbulence with a non-Kolmogorov power spectrum affects the major statistics of stochastic electromagnetic beams, such as the spectral composition and the states of coherence and polarization. We suggest a detailed survey on how these properties evolve on propagation of beams generated by electromagnetic Gaussian Schell-model sources, depending on the fractal constant α of the atmospheric power spectrum.
AB - We present a detailed investigation, qualitative and quantitative, on how the atmospheric turbulence with a non-Kolmogorov power spectrum affects the major statistics of stochastic electromagnetic beams, such as the spectral composition and the states of coherence and polarization. We suggest a detailed survey on how these properties evolve on propagation of beams generated by electromagnetic Gaussian Schell-model sources, depending on the fractal constant α of the atmospheric power spectrum.
UR - http://www.scopus.com/inward/record.url?scp=77952727617&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=77952727617&partnerID=8YFLogxK
U2 - 10.1364/OE.18.010650
DO - 10.1364/OE.18.010650
M3 - Article
C2 - 20588917
AN - SCOPUS:77952727617
VL - 18
SP - 10650
EP - 10658
JO - Optics Express
JF - Optics Express
SN - 1094-4087
IS - 10
ER -