On the theory of the type III burst exciter

Details On the theory of the type III burst exciter On the theory of the type III burst exciter

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...46..515s&link_type=abstract

Solar Physics, vol. 46, Feb. 1976, p. 515-527.

Physics

24

Electron Beams, Plasma-Particle Interactions, Satellite Observation, Type 3 Bursts, Wave Excitation, Coupled Modes, Distribution Functions, High Energy Electrons, Magnetohydrodynamic Stability, Saturation, Solar Electrons, Velocity Distribution

Scientific paper

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 of 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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