Abstract
The recently introduced class of Multi-Gaussian Schell-model [MGSM] beams is investigated via simulations and experiments with regards to its intensity fluctuations on propagation in atmospheric turbulence. The results indicate that the scintillation index of the MGSM beam is reduced for high values of the summation index, in agreement with previous theoretical results.
| Original language | English (US) |
|---|---|
| Title of host publication | Laser Communication and Propagation Through the Atmosphere and Oceans III |
| Publisher | SPIE |
| Volume | 9224 |
| ISBN (Print) | 9781628412512 |
| DOIs | |
| State | Published - 2015 |
| Event | Laser Communication and Propagation Through the Atmosphere and Oceans III - San Diego, United States Duration: Aug 17 2014 → Aug 19 2014 |
Other
| Other | Laser Communication and Propagation Through the Atmosphere and Oceans III |
|---|---|
| Country | United States |
| City | San Diego |
| Period | 8/17/14 → 8/19/14 |
Keywords
- Atmospheric turbulence
- random beams
- scintillation
ASJC Scopus subject areas
- Applied Mathematics
- Computer Science Applications
- Electrical and Electronic Engineering
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
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Korotkova, O., Avramov-Zamurovic, S., Nelson, C., Malek-Madani, R., Gu, Y., & Gbur, G. (2015). Scintillation reduction in multi-Gaussian Schell-model beams propagating in atmospheric turbulence. In Laser Communication and Propagation Through the Atmosphere and Oceans III (Vol. 9224). [92240M] SPIE. https://doi.org/10.1117/12.2062601