Scattering of magnetohydrodynamic waves by solar-wind turbulence

Details Scattering of magnetohydrodynamic waves by solar-wind turbulence Scattering of magnetohydrodynamic waves by solar-wind turbulence

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21..961c&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 21, Nov.-Dec. 1981, p. 961-967. In Russian.

Physics

6

Magnetohydrodynamic Waves, Plasma Turbulence, Solar Wind, Turbulence Effects, Wave Scattering, Extinction, Low Pressure, Magnetoacoustic Waves, Plasma Spectra

Scientific paper

Equations are derived that describe the propagation of Alfven and magnetoacoustic waves in a low-pressure magnetoplasma with weak low-frequency turbulence. Extinction coefficients for Alfven and magnetoacoustic waves are calculated, and it is shown that the MHD waves interact most efficiently with turbulent pulsations having scales of the order of the wavelength.

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