Propagation of a Monoenergetic Electron Beam in the Solar Corona

Details Propagation of a Monoenergetic Electron Beam in the Solar Corona Propagation of a Monoenergetic Electron Beam in the Solar Corona

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999soph..184..353m&link_type=abstract

Solar Physics, v. 184, Issue 2, p. 353-362 (1999).

Physics

28

Scientific paper

The dynamics of an electron beam is considered when the initial electron distribution is localized in a space region. Analysis is conducted for the parameters of the beam and plasma that give radio emission. We demonstrate both numerically and analytically that beam electrons propagate as a beam-plasma structure at large distances. The speed of the beam-plasma structure is equal to half of the maximum velocity of the electrons involved in this structure. The structure conserves the shape of the initial spatial distribution of electrons. A plateau with a constant maximum velocity is formed at the electron distribution function in each spatial point.

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