Access to the requested content is limited to institutions that have purchased or subscribe to SPIE eBooks.
You are receiving this notice because your organization may not have SPIE eBooks access.*
*Shibboleth/Open Athens users─please
sign in
to access your institution's subscriptions.
To obtain this item, you may purchase the complete book in print or electronic format on
SPIE.org.
Abstract
The reliability of a free-space optical communications (FSOC) system in atmospheric turbulence can be deduced from a mathematical model of the probability density function (PDF) of the irradiance (also called intensity). Scintillation can lead to power losses at the pupil plane of a receiver (Rx) and eventually to fading of the received signal below a specified threshold in the detector plane. Consequently, one of the goals in studying optical wave propagation through the atmosphere is the identification of a tractable PDF model for the irradiance under all irradiance fluctuation conditions. Over the years, an abundance of PDF models has been proposed with varying degrees of success. Of particular importance are (1) the accuracy of the PDF model in the low-intensity portion of the tail that leads to the probability of fade and (2) the bit error rate in the design of FSOC systems. Accuracy in the high-intensity portion of the tail is also important for eye-safety calculations and to recognize the potential for equipment damage through random surges.
Online access to SPIE eBooks is limited to subscribing institutions.