The small-scale turbulence of the interplanetary plasma.

Details The small-scale turbulence of the interplanetary plasma. The small-scale turbulence of the interplanetary plasma.

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..186c&link_type=abstract

Geomagn. Aeron., Vol. 29, No. 2, p. 186 - 190

Computer Science

Interplanetary Plasma: Turbulence

Scientific paper

Self-similar energy spectra of the turbulence of whistlers and unmagnetized ionosonic waves in a low-pressure magnetoactive plasma are found using the frequency-dependence of the probabilities of the possible decay processes. Comparison with the experimental data shows that solar-wind turbulence in the wave-number range ωpi/c ⪉ k ⪉ ωpe/c is primarily associated with whistlers, with waves propagating quasi-transversely with respect to the regular magnetic field playing a significant role.

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