On the strong phase screen theory of ionospheric scintillations

Details On the strong phase screen theory of ionospheric scintillations On the strong phase screen theory of ionospheric scintillations

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976rasc...11..459t&link_type=abstract

Radio Science, vol. 11, May 1976, p. 459-463.

Physics

Atmospheric Models, Ionospheric Propagation, Radio Scattering, Scintillation, Turbulence Effects, Atmospheric Turbulence, Kolmogoroff Theory, Phase Shift, Turbulence Models, Wave Excitation

Scientific paper

The problem of ionospheric scintillations is considered. It is shown that the result obtained using an ionospheric turbulence model with a single-scale length parameter, predicting modulation indices much larger than unity, is not valid for a two-parameter model of the Kolmogoroff type unless the rms phase variation for the wave exiting the ionosphere is larger than the ratio of the outer scale to the inner scale of turbulence.

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