Physics
Scientific paper
Nov 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...55..211m&link_type=abstract
Solar Physics, vol. 55, Nov. 1977, p. 211-240. NSF-supported research.
Physics
61
Electron Beams, Solar Atmosphere, Type 3 Bursts, Boundary Value Problems, Magnetic Effects, Plasma-Particle Interactions, Solar Magnetic Field, Solar Physics, Solar Wind
Scientific paper
Electron streams with type III burst characteristics are numerically modeled. The electron-plasma wave quasilinear interaction is assumed to be the dominant velocity diffusion process. The quasilinear equations with the addition of spontaneous emission, magnetic and collisional effects are numerically solved as an initial value and a half-space boundary value problem with time, distance and velocity as the independent variables for a solar-type background plasma and a type-III-like stream. Background density and temperature coordinate structure, spontaneous emission, magnetic fields, electron-ion collisions, stream reabsorption and wave pileup are shown to affect propagation and are incorporated into a physical description of the stream motion. The calculated electron flux-time profiles at the earth suggest scatter-free propagation and compare well with type III stream observations.
Magelssen G. R.
Smith Donelson F.
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