Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..74..491g&link_type=abstract
Astrophysics and Space Science, vol. 74, no. 2, Feb. 1981, p. 491-495.
Astronomy and Astrophysics
Astrophysics
1
Magnetohydrodynamic Waves, Plasma Conductivity, Plasma Oscillations, Plasma Turbulence, Wave Propagation, Electrical Resistivity, Energy Dissipation, Magnetosonic Resonance, Type 4 Bursts
Scientific paper
A theoretical study is presented of the propagation of nonlinear Alfven waves in a turbulent plasma with large but finite conductivity. The Alfven wave in such a medium is governed by the diffusion equation. It is shown that an initial periodic perturbation (for a constant magnetic field strength) while still being incompressive decays due to dissipation. The study indicates that the origin of type IV bursts is a magnetosonic wave, which, although accompanied by an Alfven wave, forms the shock wave in time intervals much longer than the time of Alfven wave decay.
No associations
LandOfFree
Nonlinear Alfven waves in a plasma with a finite conductivity 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 Nonlinear Alfven waves in a plasma with a finite conductivity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonlinear Alfven waves in a plasma with a finite conductivity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1407115