Reacceleration of cosmic rays in interstellar space has been studied in detail in order to examine the behavior of the ratios of secondary to primary nuclei in cosmic radiation. It is found that modest acceleration in a confinement region, where particles escape more freely at high energies, provides a better fit to the observed data. The effect of reacceleration on the spectral shape of proton and helium components of cosmic rays has been studied. The examination of two different models has shown that reacceleration provides a poor fit to the observed proton data.
Effect of re-acceleration on cosmic ray components
Advances in Space Research ; 9 , 12 1
1989-01-01
Sonstige
Keine Angabe
Englisch
Effect of re-acceleration on cosmic ray components
Elsevier | 1989
|Cosmic-ray acceleration by pulsars
Elsevier | 1984
|Cosmic ray acceleration by supernova shocks
Elsevier | 2007
|Cosmic ray acceleration by supernova shocks
Online Contents | 2008
|Injection mechanism for cosmic ray acceleration
Elsevier | 1989
|