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Signal structure in diffuse refraction from the ionosphere
Authors:S. A. Namazov
Abstract:Conclusions Thus, our investigations with 10-mgrsec resolution have shown that a diffuse signal usually consisted of several discrete pulses among which there is a well-defined peak pulse. The time extent of a diffuse pulse group was 40–80 mgrsec for vertical sounding and 100–150 mgrsec for oblique sounding. The most probable shift between adjacent pulses was 15–20 mgrsec. For oblique sounding, and for vertical sounding at frequencies ohgr>0.8ohgrc, individual diffuse-signal pulses fluctuated in amplitude and delay time. For vertical sounding at frequencies ohgr<0.8ohgrc, the pulses fluctuated in amplitude and had stable time shifts over a 2-min observation run.For a vertical sounding, the effect prevailing among the four possible mechanisms considered for generation of diffuse reflections in the plane of the meridian at mid- and low latitudes is scattering by magnetically oriented inhomogeneities, while in the latitude plane it is the partial-reflection mechanism.The diffuse-signal structure for oblique sounding may be explained satisfactorily by the mechanism of forward scattering by discrete irregularities of a layer. In this case, the scattering and reception angles prove to be related in single-valued fashion to the group delay time for known average layer parameters. This makes it possible to determine the scattering indicatrix of an irregularity and the angular spectrum of the waves.Institute of Radio Engineering and Electronics, Academy of Sciences of the USSR. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 18, No. 9, pp. 1355–1364, September, 1975.
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