Density fluctuations in the solar wind based on type III radio bursts
Type III bursts are among the strongest radio signals routinely observed by both space-borne and ground-based instruments. They are generated via the plasma emission mechanism, when beams of suprathermal electrons interact with the ambient plasma, triggering radio emissions at the plasma frequency (the fundamental emission) or at its second harmonic (the harmonic emission). As the electron beams propagate outward from the sun, radio emissions are generated at progressively lower frequencies corresponding to a decreasing ambient solar wind plasma density. Type III bursts can be simultaneously detected over a broad range of longitudes, and their radio sources lie at considerably larger radial distances than predicted by electron density models.
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2020-04-01
