Is there a common explanation for scattering of type III radio bursts and solar radar

Details Is there a common explanation for scattering of type III radio bursts and solar radar Is there a common explanation for scattering of type III radio bursts and solar radar

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...79..375w&link_type=abstract

Solar Physics, vol. 79, Aug. 1982, p. 375-377. NSF-supported research.

Physics

3

Radar Scattering, Solar Corona, Solar Radar Echoes, Type 3 Bursts, Polarized Radiation, Solar Magnetic Field, Wave Scattering

Scientific paper

The fundamental and harmonic components of type III radio bursts appear to originate from the same source in the corona. A common source of scattering is also suggested by the observed decrease of polarization toward the limb in both components. The apparent source heights of type III bursts and of the strong radar echoes can both be explained by scattering at the coronal level, where the frequency/plasma frequency ratio is in the 2-5 range. The ducting indicated by the type III harmonic/fundamental frequency ratios corresponds to the density gradients required for the lower-hybrid waves that can cause the scattering.

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