This review describes the basic theory of cosmic ray acceleration by shocks including the plasma instabilities confining cosmic rays near the shock, the effect of the magnetic field orientation, the maximum cosmic ray energy and the shape of the cosmic ray spectrum. Attention is directed mainly towards Galactic cosmic rays accelerated by supernova remnants. © 2012 Elsevier B.V. All rights reserved
Abstract One century ago Viktor Hess carried out several balloon flights that led him to conclude th...
We evaluate the current status of supernova remnants as the sources of Galactic cosmic rays. We summ...
We investigate the appearance of magnetic field amplification resulting from a cosmic ray escape cur...
Supernova remnants (SNR) are the most likely source of galactic cosmic rays (CRs) up to the 'knee' i...
Supernova remnants (SNR) are the most likely source of galactic cosmic rays (CRs) up to the 'knee' i...
The problem of the origin of cosmic rays is considered in an astronomical context and the current ob...
It is well known that electrons and probably cosmic rays are accelerated in supernova remnants. To m...
It is well known that electrons and probably cosmic rays are accelerated in supernova remnants. To m...
It is well known that electrons and probably cosmic rays are accelerated in supernova remnants. To m...
Cosmic ray acceleration may occur at a supernova shock expanding into a circumstellar wind sustainin...
Cosmic ray acceleration may occur at a supernova shock expanding into a circumstellar wind sustainin...
International audienceWe give a brief review of the origin and acceleration of cosmic rays (CRs), em...
International audienceWe give a brief review of the origin and acceleration of cosmic rays (CRs), em...
We review the theory of cosmic ray transport and acceleration with an emphasis on the underlying pla...
We review the theory of cosmic ray transport and acceleration with an emphasis on the underlying pla...
Abstract One century ago Viktor Hess carried out several balloon flights that led him to conclude th...
We evaluate the current status of supernova remnants as the sources of Galactic cosmic rays. We summ...
We investigate the appearance of magnetic field amplification resulting from a cosmic ray escape cur...
Supernova remnants (SNR) are the most likely source of galactic cosmic rays (CRs) up to the 'knee' i...
Supernova remnants (SNR) are the most likely source of galactic cosmic rays (CRs) up to the 'knee' i...
The problem of the origin of cosmic rays is considered in an astronomical context and the current ob...
It is well known that electrons and probably cosmic rays are accelerated in supernova remnants. To m...
It is well known that electrons and probably cosmic rays are accelerated in supernova remnants. To m...
It is well known that electrons and probably cosmic rays are accelerated in supernova remnants. To m...
Cosmic ray acceleration may occur at a supernova shock expanding into a circumstellar wind sustainin...
Cosmic ray acceleration may occur at a supernova shock expanding into a circumstellar wind sustainin...
International audienceWe give a brief review of the origin and acceleration of cosmic rays (CRs), em...
International audienceWe give a brief review of the origin and acceleration of cosmic rays (CRs), em...
We review the theory of cosmic ray transport and acceleration with an emphasis on the underlying pla...
We review the theory of cosmic ray transport and acceleration with an emphasis on the underlying pla...
Abstract One century ago Viktor Hess carried out several balloon flights that led him to conclude th...
We evaluate the current status of supernova remnants as the sources of Galactic cosmic rays. We summ...
We investigate the appearance of magnetic field amplification resulting from a cosmic ray escape cur...
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