OF THE WORKSHOP : MECHANISMS FOR SOLAR TYPE lII RADIO BURSTS
نویسندگان
چکیده
In situ satellite observations of type III burst exciters at 1 AU show that the beam does not evolve into a plateau in velocity space, contrary to the prediction quasilinear theory. The observations can be explained by a theory that includes mode coupling effects due to excitation of the parametric oscillating two-stream instability and its saturation by anomalous resistivity. The time evolution of the beam velocity distribution is included in the analysis.
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تاریخ انتشار 2004