Transport and acceleration of cosmic rays in the Galactic disk and halo by strong turbulence

Details Transport and acceleration of cosmic rays in the Galactic disk and halo by strong turbulence Transport and acceleration of cosmic rays in the Galactic disk and halo by strong turbulence

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.2056b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, Russia, Nov. 1-3, 1990, Materialy. A92-40776 16-93) Akademiia Nauk

Physics

Galactic Cosmic Rays, Galactic Halos, Interstellar Space, Magnetohydrodynamic Turbulence, Particle Acceleration, Radiative Transfer, Massive Stars, Stellar Evolution

Scientific paper

The interaction of cosmic rays with large-scale strong turbulence in the Galactic disk and halo is investigated. Kinetic coefficients which describe the spatial transfer and effects of particle acceleration are calculated within the framework of renormalization theory. An analysis of possible diffusion regimes of strongly magnetized particles, which are caused by turbulent motions, across a regular magnetic field, is given.

Affiliated with

Also associated with

No associations

Rating

Transport and acceleration of cosmic rays in the Galactic disk and halo by strong 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 Transport and acceleration of cosmic rays in the Galactic disk and halo by strong turbulence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Transport and acceleration of cosmic rays in the Galactic disk and halo by strong turbulence will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1876354