Solar Physics

, Volume 184, Issue 2, pp 353–362

Propagation of a Monoenergetic Electron Beam in the Solar Corona

  • V.N. Mel'nik
  • V. Lapshin
  • E. Kontar
Article

DOI: 10.1023/A:1005191910544

Cite this article as:
Mel'nik, V., Lapshin, V. & Kontar, E. Solar Physics (1999) 184: 353. doi:10.1023/A:1005191910544

Abstract

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.

Copyright information

© Kluwer Academic Publishers 1999

Authors and Affiliations

  • V.N. Mel'nik
    • 1
  • V. Lapshin
    • 2
  • E. Kontar
    • 3
  1. 1.Institute of Radio Astronomy of National Academy of SciencesKharkovUkraine
  2. 2.National Science Center 'Institute of Physics & Technology'KharkovUkraine
  3. 3.Kharkov State UniversityKharkovUkraine