Nonlinear perturbation theory for cosmic ray propagation in random magnetic fields

1973 ◽  
Vol 25 (2) ◽  
pp. 471-490 ◽  
Author(s):  
Heinrich J. V�lk
1970 ◽  
Vol 39 ◽  
pp. 168-183
Author(s):  
E. N. Parker

The topic of this presentation is the origin and dynamical behavior of the magnetic field and cosmic-ray gas in the disk of the Galaxy. In the space available I can do no more than mention the ideas that have been developed, with but little explanation and discussion. To make up for this inadequacy I have tried to give a complete list of references in the written text, so that the interested reader can pursue the points in depth (in particular see the review articles Parker, 1968a, 1969a, 1970). My purpose here is twofold, to outline for you the calculations and ideas that have developed thus far, and to indicate the uncertainties that remain. The basic ideas are sound, I think, but, when we come to the details, there are so many theoretical alternatives that need yet to be explored and so much that is not yet made clear by observations.


1993 ◽  
Vol 199 (1) ◽  
pp. 125-132 ◽  
Author(s):  
K. Kudela ◽  
M. Slivka ◽  
M. Stehl�k ◽  
A. Geranios

2017 ◽  
Vol 469 (2) ◽  
pp. 1849-1860 ◽  
Author(s):  
J. H. Matthews ◽  
A. R. Bell ◽  
K. M. Blundell ◽  
A. T. Araudo

1976 ◽  
Vol 17 (1) ◽  
pp. 121-140 ◽  
Author(s):  
Charles R. Eminhizer ◽  
Robert H. G. Helleman ◽  
Elliott W. Montroll

1997 ◽  
Vol 477 (2) ◽  
pp. 560-567 ◽  
Author(s):  
Torsten A. Ensslin ◽  
Peter L. Biermann ◽  
Philipp P. Kronberg ◽  
Xiang‐Ping Wu

2009 ◽  
Vol 5 (H15) ◽  
pp. 251-253
Author(s):  
Vitor de Souza ◽  
Peter L. s Biermman

AbstractIn this paper we briefly discuss the present status of the cosmic ray astrophysics under the light of the new data from the Pierre Auger Observatory. The measured energy spectrum is used to test the scenario of production in nearby radio galaxies. Within this framework the AGN correlation would require that most of the cosmic rays are heavy nuclei and are widely scattered by intergalactic magnetic fields.


1984 ◽  
Vol 30 (5) ◽  
pp. 2227-2233 ◽  
Author(s):  
Sergio A. Maluendes ◽  
Francisco M. Fernández ◽  
Alejandro M. Mesón ◽  
Eduardo A. Castro

2009 ◽  
Vol 395 (2) ◽  
pp. 895-906 ◽  
Author(s):  
D. Caprioli ◽  
P. Blasi ◽  
E. Amato ◽  
M. Vietri
Keyword(s):  

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