11
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: not found
      • Article: not found

      Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field

      ,
      Monthly Notices of the Royal Astronomical Society
      Wiley-Blackwell

      Read this article at

      ScienceOpenPublisher
      Bookmark
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Related collections

          Most cited references8

          • Record: found
          • Abstract: not found
          • Article: not found

          Non-linear amplification of a magnetic field driven by cosmic ray streaming

            Bookmark
            • Record: found
            • Abstract: not found
            • Article: not found

            The non-linear self-regulation of cosmic ray acceleration at shocks

            A. Bell (1987)
              Bookmark
              • Record: found
              • Abstract: not found
              • Article: not found

              The origins of high-energy cosmic rays

              W I Axford (1994)
                Bookmark

                Author and article information

                Journal
                Monthly Notices of the Royal Astronomical Society
                Monthly Notices of the Royal Astronomical Society
                Wiley-Blackwell
                0035-8711
                1365-2966
                March 01 2001
                March 01 2001
                : 321
                : 3
                : 433-438
                Article
                10.1046/j.1365-8711.2001.04063.x
                2e3d8c34-d4f2-4166-b21e-2c55cfc55574
                © 2001
                History

                Comments

                Comment on this article