
Analyzing the efficiency of a practical heterodyne lidar in the turbulent atmosphere: telescope parameters
Author(s) -
Aniceto Belmonte
Publication year - 2003
Publication title -
optics express
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.394
H-Index - 271
ISSN - 1094-4087
DOI - 10.1364/oe.11.002041
Subject(s) - optics , heterodyne (poetry) , lidar , telescope , physics , atmospheric turbulence , aperture (computer memory) , atmospheric optics , heterodyne detection , wavelength , turbulence , transmitter , remote sensing , superheterodyne receiver , free space optical communication , huygens–fresnel principle , optical communication , laser , meteorology , computer science , telecommunications , acoustics , geology , channel (broadcasting) , quantum mechanics , microwave
The simulation of beam propagation permits examination of the signal degradation in a heterodyne receiver caused by refractive turbulence under general atmospheric conditions and at arbitrary transmitter and receiver configurations. At shorter wavelengths, an understanding of turbulence effects is essential for deciding the optimal telescope parameters, i.e., focal length and aperture diameter, of a practical heterodyne lidar.