Computer Science
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..313b&link_type=abstract
Proceedings from the 18th International Cosmic Ray Conference, held in Bangalore, India, 22 August - 3 September, 1983. Volume
Computer Science
Scientific paper
Cosmic rays (CR) acceleration by large scale motion with account of effectively particles scattering by small scale turbulence, magnetic fields and shock waves is considered. Some features of particle acceleration by compressible and incompressible motions are discussed. It is shown that this acceleration mechanism plays an important role for CR acceleration problems in young and old supernova remnants.
Bykov Andrei M.
Toptygin Igor N.
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