Physics
Scientific paper
Oct 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..129..325k&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 129, Oct. 1990, p. 325-341. Research supported by SERC and British Council.
Physics
20
Electron Beams, Electron Energy, Solar Corona, Solar Flares, Atmospheric Models, Computerized Simulation, Power Spectra, Solar Atmosphere
Scientific paper
The one-dimensional particle simulation of return current and direct collisional effects is presently used to study the evolution of a pulse of truncated power-law spectrum nonthermal electrons injected into a uniformly dense coronal plasma, deliberately ignoring quasi-linear relaxation of the beam in order to isolate the modification of return-current effects by the pulsed injection. A marked difference is noted, in the energetic electron trajectories over parameter conditions where return current losses dominate, between the pulsed injection case and the continuous injection case (for the same beam current at injection). Energy losses to return-current dissipation are lower in the pulsed case, due to the rapid fall in the local beam current as the pulse disperses in space.
Alexander Dave
Brown John C.
Karlicky Marian
MacKinnon Alexander L.
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