Magnetohydrodynamic Turbulence in the Cosmic Rays Confinement Regions of Galaxy

Details Magnetohydrodynamic Turbulence in the Cosmic Rays Confinement Regions of Galaxy Magnetohydrodynamic Turbulence in the Cosmic Rays Confinement Regions of Galaxy

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..247b&link_type=abstract

Proceedings from the 18th International Cosmic Ray Conference, held in Bangalore, India, 22 August - 3 September, 1983. Volume

Physics

Scientific paper

Observational data and theoretical models of magnetohydrodynamic
turbulence generation in the interstellar medium and supernova remnants
are considered. The role of shock waves and cosmic rays for turbulence
generation is discussed.

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