The spectrum of whistler turbulence in the interplanetary plasma

Details The spectrum of whistler turbulence in the interplanetary plasma The spectrum of whistler turbulence in the interplanetary plasma

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..385c&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, May-June 1983, p. 385-389. In Russian.

Computer Science

2

Interplanetary Magnetic Fields, Plasma Turbulence, Solar Wind, Whistlers, Cyclotron Resonance, Energy Spectra, Low Turbulence, Magnetic Flux, Plasma Frequencies, Plasma Spectra, Plasma Waves, Plasma-Electromagnetic Interaction, Space Plasmas, Wave Interaction

Scientific paper

The spatial and temporal spectra of whistler turbulence in the interplanetary plasma are investigated theoretically for the small-scale spectral range confined between the ion and electron cyclotron resonances, k = 10 to the -7th to 10 to the -5th per cm. Theoretical results are compared with experimental data on high-frequency fluctuations of the magnetic field in the interplanetary plasma.

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