A study of Type V solar radio bursts. II - A theoretical model

Details A study of Type V solar radio bursts. II - A theoretical model A study of Type V solar radio bursts. II - A theoretical model

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...56..405r&link_type=abstract

Solar Physics, vol. 56, Feb. 1978, p. 405-416.

Physics

4

Electron Beams, Type 5 Bursts, Circular Polarization, Coulomb Collisions, Electron Distribution, Plasma Waves, Polarization Characteristics, Type 3 Bursts, Wave Interaction, Wave Scattering

Scientific paper

According to the proposed model of the solar Type V event, the main difference between Type III and Type V bursts involves the evolution of the electron beam. In a Type V event the beam elongates rapidly so that it takes progressively longer times to pass higher plasma levels. Topics discussed include the effects of beam spreading, beam elongation by a velocity spread in a one-dimensional streaming electron distribution, effects of pitch angle scattering, and the lack of polarization. The roles played by Coulomb collisions, nonlinear interactions with Langmuir waves, and wave-particle scattering from various hydromagnetic wave modes are considered. The model is compared with earlier models and with observations.

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