Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16.1123b&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, Dec. 1990, p. 1123-1132. In Russian. In Russian.
Astronomy and Astrophysics
Astronomy
Magnetoacoustic Waves, Magnetohydrodynamic Waves, Solar Cosmic Rays, Solar Wind, Space Plasmas, Wave Generation, Cosmic Rays, Heliosphere, Plasma Turbulence
Scientific paper
The rate of growth of magnetoacoustic waves excited in the solar wind by
solar cosmic ray streams is calculated. Calculation results suggest that
this process plays an important role in the generation of MHD turbulence
in the inner heliosphere.
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