Cosmic-ray electrons in the diffusion-convection model of particle propagation

Details Cosmic-ray electrons in the diffusion-convection model of particle propagation Cosmic-ray electrons in the diffusion-convection model of particle propagation

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..696d&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Nov.-Dec. 1980, p. 696-699.) Soviet Astronomy Letters, vol. 6, Nov.-Dec. 1980, p. 36

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Cosmic Rays, High Energy Electrons, Milky Way Galaxy, Particle Diffusion, Convective Flow, Emission Spectra, Halos, Particle Motion, Radio Emission

Scientific paper

Electron and radio emission spectra are calculated within the framework of a simple diffusion-convection model of cosmic ray propagation with allowance for convective escape of cosmic rays and adiabatic losses. Comparison of the calculations with the observed spectra suggests that the propagation of electrons through the galactic halo is realized by diffusion. Analysis of data on the proton-nucleon component of cosmic rays in terms of a pure diffusion model indicates that the size of the halo should be of order 5-10 kpc.

Affiliated with

Also associated with

No associations

Rating

Cosmic-ray electrons in the diffusion-convection model of particle propagation 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 Cosmic-ray electrons in the diffusion-convection model of particle propagation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmic-ray electrons in the diffusion-convection model of particle propagation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-757869