Physics
Scientific paper
Mar 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..119..207m&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 119, no. 1, 1989, p. 207-210. Research supported by Korea Institute of Technology and Korea
Physics
1
Electron Beams, Plasma Heating, Plasma-Particle Interactions, Solar Corona, Solar Flares, Beam Plasma Amplifiers, Chromosphere, Electric Fields
Scientific paper
Electron beam propagation in a fully ionized plasma has been studied using a one-dimensional particle simulation model. The electrostatic results show the essential features of beam-plasma interactions. It is found that the return currents are enhanced by the beam-plasma instability which accelerates ambient plasmas. The results also show the heating of ambient plasmas and the trapping of plasmas due to the locally generated electric field. The electromagnetic simulations show much the same results as the electrostatic simulations do. The results are discussed in context of the heating of coronal plasma during solar flares.
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