Dissipation of long magnetoacoustic waves through interaction with cosmic rays

Details Dissipation of long magnetoacoustic waves through interaction with cosmic rays Dissipation of long magnetoacoustic waves through interaction with cosmic rays

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pazh....7...53p&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, Jan. 1981, p. 53-55.) Soviet Astronomy Letters, vol. 7, Jan.-Feb. 1981, p. 30, 31. T

Astronomy and Astrophysics

Astronomy

Cosmic Rays, Energy Dissipation, Interstellar Matter, Magnetoacoustic Waves, Magnetohydrodynamic Waves, Wave Interaction, Long Wave Radiation, Thermal Plasmas, Wave Propagation

Scientific paper

It is shown that the damping of magnetoacoustic waves by cosmic-ray diffusion will predominate in the interstellar medium for wavelengths not less than 1 pc or (for hot material with a temperature of 1,000,000 K and a density of 0.003 per cu cm) not less than 100 pc. It is also found that the dissipated wave energy will contribute to the acceleration of the cosmic rays.

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