Signal structure in diffuse refraction from the ionosphere

Conclusions

Thus, our investigations with 10-μsec 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 μsec for vertical sounding and 100–150 μsec for oblique sounding. The most probable shift between adjacent pulses was 15–20 μsec. For oblique sounding, and for vertical sounding at frequencies ω>0.8ω_c, individual diffuse-signal pulses fluctuated in amplitude and delay time. For vertical sounding at frequencies ω<0.8ω_c, 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.