Beam-plasma instability in the presence of low-frequency turbulence

Details Beam-plasma instability in the presence of low-frequency turbulence Beam-plasma instability in the presence of low-frequency turbulence

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phfl...25.1062g&link_type=abstract

Physics of Fluids, vol. 25, June 1982, p. 1062-1072. Research supported by the U.S. Department of Energy

Physics

38

Beam Interactions, Electron Plasma, Electrostatic Waves, Magnetohydrodynamic Stability, Plasma Turbulence, Type 3 Bursts, Plasma Density, Plasma Frequencies, Plasma Resonance, Solar Wind

Scientific paper

General equations are derived for a linear beam-plasma instability in the presence of low-frequency turbulence. Within a 'quasi-linear' statistical approximation, these equations contain Langmuir wave scattering, diffusion, resonant and nonresonant anomalous absorption, and a 'plasma laser' effect. It is proposed that naturally occurring density irregularities in the solar wind may stabilize the beam-unstable Langmuir waves which occur during type III solar emissions.

Affiliated with

Also associated with

No associations

Rating

Beam-plasma instability in the presence of low-frequency turbulence 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 Beam-plasma instability in the presence of low-frequency turbulence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Beam-plasma instability in the presence of low-frequency turbulence will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1355146