Carregant...
Carregant...

Vés al contingut (premeu Retorn)

Exponentiated Weibull model for the irradiance probability density function of a laser beam propagating through atmospheric turbulence

Autor
Barrios, R.; Dios, V.
Tipus d'activitat
Article en revista
Revista
Optics and laser technology
Data de publicació
2013-02
Volum
45
Número
1
Pàgina inicial
13
Pàgina final
20
DOI
https://doi.org/10.1016/j.optlastec.2012.08.004 Obrir en finestra nova
Repositori
http://hdl.handle.net/2117/19582 Obrir en finestra nova
URL
http://www.sciencedirect.com/science/article/pii/S0030399212003556# Obrir en finestra nova
Resum
Many distributions have been proposed to model the probability density function of irradiance fluctuations. The most widespread models nowadays are the Lognormal (LN) and Gamma–Gamma (GG) distributions. Albeit these models comply with the actual PDF data most of the time, neither of them works in all scenarios and, depending on the conditions, one of the two have to be chosen. In this paper, a new model is presented resulting in the exponentiated Weibull (EW) distribution, along with a physica...
Citació
Barrios, R.; Dios, V. Exponentiated Weibull model for the irradiance probability density function of a laser beam propagating through atmospheric turbulence. "Optics and laser technology", Febrer 2013, vol. 45, núm. 1, p. 13-20.
Paraules clau
Atmospheric Turbulence, Channel Model, Exponentiated Weibull
Grup de recerca
RSLAB - Grup de Recerca en Teledetecció

Participants