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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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