Physics
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...1e..52m&link_type=abstract
Cosmic Particle Acceleration, 26th meeting of the IAU, Joint Discussion 1, 16-17 August, 2006, Prague, Czech Republic, JD01, #52
Physics
Scientific paper
Nowadays Type III-like bursts with high frequency drift rates at decameter wavelengths were observed. Particularly, they can be connected with relativistic electron beams. In this paper the properties of relativistic electron propagation in coronal plasma with taking into account of Langmuir waves generation and waves interaction with electrons are studied. The consideration is conducted in the framework of weak turbulence theory when quasi-linear time is essentially smaller than flyaway time. We make going from kinetic description to gas-dynamic one, obtain a set of gas dynamic equations and solve the propagation problem of mono-energetic electron beams. It is shown that electron beams propagate in the form of relativistic beam-plasma structure with constant velocity. We discuss a possible interpretation of Type III-like bursts using developed theory of nonlinear interaction of relativistic electron beams with plasma.
Mel'nik Valentin N.
Rutkevych B. P.
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