The generation of type III solar radio bursts - The role of induced scattering of plasma waves by ions

Astronomy and Astrophysics – Astronomy

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Plasma Waves, Plasma-Particle Interactions, Type 3 Bursts, Wave Scattering, Astronomical Models, Decametric Waves, Ions, Noise Storms, Nonlinear Systems, Solar Corona

Scientific paper

A brief analysis of the induced scattering of plasma waves under typical conditions for the generation of type III solar radio bursts shows that the growth rate of the bursts will diminish if the source comes closer to the k = 0 spectral density region than the width of the kernel of the integral transform. During noise storms, the quasi-steady rise of the plasma-noise level in the region where the bursts are generated suggests the presence of a quasi-steady condensate, an intense level of plasma waves near the zero region of wave vector space. The proximity of the condensate to wave vectors of zero is determined by its intensity and by the values of the threshold for the onset of modulation instability. The agents exciting a burst would travel through the corona quasi-linearly at a velocity interval which lies at C/3.

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