AbstractReacceleration of cosmic rays produced by galactic sources on the galactic wind termination shock is considered. The problem of the cosmic ray spectrum continuity is investigated. Numeric results are presented and discussed. We found that a smooth spectral transition from the galactic cosmic rays to the cosmic rays reaccelerated at the galactic wind termination shock is difficult to produce, if the maximum energy of accelerated particles is the same throughout the surface of the termination shock. The possible solution of this problem is the non-spherical termination shock with different maximum energies at different places of the shock.
Cosmic ray reacceleration on the galactic wind termination shock
Advances in Space Research ; 37 , 10 ; 1923-1927
2005-06-10
5 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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