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IEEE Transactions on Antennas and Propagation
Volume 47 Number 1, January 1999
Table of Contents for this issue
Complete paper in PDF format
Frequency Dependence of Amplitude Scintillation
Max M. J. L. van de Kamp, Carlo Riva, Jouni K. Tervonen, and Erkki T. Salonen
Page 77.
Abstract:
In the prediction models of tropospheric scintillation on
earth-satellite paths from Karasawa, Yamada, and Allnutt and ITU-R, the
frequency dependence of scintillation is expressed as a power law with a
different exponent for each model. In this paper, this is verified using
a collection of measurement results from different satellite links in
Europe, the U.S., and Japan at frequencies from 4 to 50 GHz and
elevation angles from 2.5 to 52^{irc}. It shows that the
exponent of the power law varies widely among the results from the
different sites. Possible explanations of this are: 1) the frequency
dependence of scintillation due to cloudy turbulence is different from
that due to clear-sky turbulence and this kind of scintillation may be
present to different extents in the various databases due to climatic
differences and different clear-sky selection procedures or 2)
angle-of-arrival fluctuations due to turbulence have a different
frequency dependence and this effect may have some impact on the
measured scintillation at some of the sites.
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