Dynamics of electron beams in the inhomogeneous solar corona plasma

Details Dynamics of electron beams in the inhomogeneous solar corona plasma Dynamics of electron beams in the inhomogeneous solar corona plasma

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001soph..202..131k&link_type=abstract

Solar Physics, v. 202, Issue 1, p. 131-149 (2001).

Physics

23

Scientific paper

Dynamics of a spatially-limited electron beam in the inhomogeneous solar corona plasma is considered in the framework of weak turbulence theory when the temperature of the beam significantly exceeds that of surrounding plasma. The numerical solution of kinetic equations manifests that generally the beam accompanied by Langmuir waves propagates as a beam-plasma structure with a decreasing velocity. Unlike the uniform plasma case the structure propagates with the energy losses in the form of Langmuir waves. The results obtained are compared with the results of observations of type III bursts. It is shown that the deceleration of type III sources can be explained by corona inhomogeneity. The frequency drift rates of the type III sources are found to be in good agreement with the numerical results of beam dynamics.

Affiliated with

Also associated with

No associations

Rating

Dynamics of electron beams in the inhomogeneous solar corona plasma does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dynamics of electron beams in the inhomogeneous solar corona plasma, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of electron beams in the inhomogeneous solar corona plasma will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-819683