Physics
Scientific paper
Dec 1969
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969phrv..188.1994b&link_type=abstract
Physical Review, vol. 188, Issue 5, pp. 1994-2010
Physics
20
Scientific paper
We consider the modulating of the energy spectrum of cosmic-ray electrons as they propagate in interstellar space. The effects of spatial propagation, energy loss, boundary conditions, and the spatial distribution and energy spectrum of the electrons injected into interstellar space by the sources are all taken into account. Two models for spatial propagation are considered: isotropic diffusion and convection diffusion. In the latter, the particle motion parallel to the disk plane is characterized by diffusion, while particles are transported perpendicular to the disk plane by convection, caused by the outward expansion of the field lines. Examples are worked out for several source distributions. It is shown that the high-energy electron distribution (in both energy and space) is determined by the source distribution, rather than the properties of the confinement region (i.e., the propagation model). In order to illustrate how one can use the observable quantities (the electron spectrum and positron fraction at Earth, and the background Galactic radio and γ radiation) to determine the properties of the injection spectrum, we have considered the construction of a model of primary cosmic-ray electron sources in some detail. It is found that a combination of a source with a disk distribution and a source concentrated at the Galactic center may be necessary to explain the observed disk γ rays.
Berkey G. B.
Shen Shih-Chi
No associations
LandOfFree
Origin and Propagation of Cosmic-Ray Electrons 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 Origin and Propagation of Cosmic-Ray Electrons, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Origin and Propagation of Cosmic-Ray Electrons will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1748150