Small-scale turbulence of the interplanetary plasma

Details Small-scale turbulence of the interplanetary plasma Small-scale turbulence of the interplanetary plasma

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..210c&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Mar.-Apr. 1989, p. 210-215. In Russian.

Computer Science

Interplanetary Medium, Plasma Turbulence, Space Plasmas, Energy Spectra, Ion Acoustic Waves, Plasma Spectra, Solar Wind, Whistlers

Scientific paper

The self-similar energy spectra of whistler and nonmagnetized ion-acoustic wave turbulence in a low-pressure magnetoplasma are determined on the basis of the frequency dependences of the probabilities of possible decay processes. A comparison with experimental data shows that the solar-wind turbulence in the wavenumber range from omega(pi)/c to omega(pe)/c, where omega(pi) is the ion plasma frequency, omega(pe) is the electron plasma frequency, and c is the speed of light, is connected mainly with whistlers; a major role here is played by waves propagating quasi-transversely with respect to the regular magnetic field.

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