Höhn D H
Astronomisches Institut der Universität, Tübingen, Germany.
Appl Opt. 1966 Sep 1;5(9):1433-6. doi: 10.1364/AO.5.001433.
The frequency spectra of light intensity fluctuations of a laser beam by atmospheric turbulence were investigated using a He-Ne gas laser at 6328 A with a beam diameter of about 3.5 mm and optical path length of L = 4.5 km and 14.5 km. The normalized spectra U(f) were not systematically affected by different receiving aperture diameters 5 mm <or= D <or= 80 mm, probably because of the small diameter of the output aperture of the source. The theoretical relation f(c) L(-1/2), where f(c) is a characteristic frequency of U(f), does not appear to hold empirically.