Self-consistent shock structure in the presence of cosmic rays and Alfven waves

Details Self-consistent shock structure in the presence of cosmic rays and Alfven waves Self-consistent shock structure in the presence of cosmic rays and Alfven waves

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981icrc....9..242m&link_type=abstract

Proceedings of the 17th International Cosmic Ray Conference, held in Paris, France. Volume 9., p.242

Physics

Convective Flow, Cosmic Rays, Magnetohydrodynamic Flow, Magnetohydrodynamic Waves, Plasma Diffusion, Shock Waves, Adiabatic Conditions, Differential Equations, Integral Equations

Scientific paper

The structure of a parallel shock including the back reaction from cosmic rays and Alfven waves generated by the streaming instability were investigated. An integral of the wave growth equation which describes how the wave magnetic pressure is amplified by both adiabatic and instability effects is obtained. The results imply that the overall efficiency of the conversion of flow energy to cosmic ray energy may only become high provided that the wave power is saturated at some modest level by nonlinear effects.

Affiliated with

Also associated with

No associations

Rating

Self-consistent shock structure in the presence of cosmic rays and Alfven waves 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 Self-consistent shock structure in the presence of cosmic rays and Alfven waves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Self-consistent shock structure in the presence of cosmic rays and Alfven waves will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-744326