The fine structure of the solar wind velocity in the model of the power spectrum of inhomogeneities

Details The fine structure of the solar wind velocity in the model of the power spectrum of inhomogeneities The fine structure of the solar wind velocity in the model of the power spectrum of inhomogeneities

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ge%26ae..15..769l&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 15, Sept.-Oct. 1975, p. 769-776. In Russian.

Physics

3

Power Spectra, Scintillation, Solar Wind Velocity, Wave Dispersion, Cross Correlation, Energy Dissipation, Fine Structure, Velocity Distribution

Scientific paper

A model of the solar wind with a power spectrum of inhomogeneities is used to study the dispersion dependence of the scintillation pattern velocity. The dispersion dependence is obtained for various velocity fine structure models, including for a medium with two characteristic velocities, an extended medium and a medium with an arbitrary velocity distribution. It is shown that the difference in dispersion dependence for Gaussian and power spectra is small.

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