Statistics – Computation
Scientific paper
Apr 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.132..353r&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 132, no. 2, April 1987, p. 353-386.
Statistics
Computation
3
Computational Astrophysics, Particle Acceleration, Pulsar Magnetospheres, Pulsars, Stellar Models, Chaos, Electron Acceleration, Lorentz Transformations, Magnetic Field Configurations, Particle Production, Radio Emission
Scientific paper
The present computer simulation of the electron acceleration within a pulsar magnetosphere's outflow channel, for the spherically-symmetric case, notes the stationary motion of electrons to be unstable in the case where the parameter for the inhomogeneity of the background charge is greater than its critical value. The nonstationary motion of electrons thus generated forms electron bunches that move chaotically. Attention is given to the parameter mean value distributions over the height of the magnetosphere. The results of numerical investigations of the spherically-symmetric model are used for estimation of the electron energy and of the electron flux in the case of the more realistic model, and radio emission loss is estimated.
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