A mechanism for generating the turbulence spectrum of interplanetary plasma

Details A mechanism for generating the turbulence spectrum of interplanetary plasma A mechanism for generating the turbulence spectrum of interplanetary plasma

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pazh....7..500c&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, Aug. 1981, p. 500-504.) Soviet Astronomy Letters, vol. 7, July-Aug. 1981, p. 276-278

Astronomy and Astrophysics

Astronomy

1

Interplanetary Gas, Plasma Dynamics, Plasma Turbulence, Solar Wind, Magnetohydrodynamic Waves, Power Spectra, Wave Interaction

Scientific paper

It is contended that solar wind turbulence will maintain a stationary spectrum owing to a balance near the outer scale. The balance is between the relative intensification of the turbulence due to irregularities in the medium and the transfer of energy toward higher frequencies due to nonlinear interactions. The ramifications of the model discussed here are found to agree closely with experimental results

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