The turbulent structure of the solar wind from observations in the decameter radio wavelength range

Details The turbulent structure of the solar wind from observations in the decameter radio wavelength range The turbulent structure of the solar wind from observations in the decameter radio wavelength range

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995azh....72..761b&link_type=abstract

Astronomicheskij Zhurnal, vol. 72, p. 761

Astronomy and Astrophysics

Astronomy

Solar Wind, Turbulent Flow, Solar Radio Emission, Wave Scattering, Electron Plasma, Solar Electrons, Radio Waves, Electron Density (Concentration), Radio Interferometers, Plasma Diagnostics

Scientific paper

Results of observations of scattering of the decameter radio emission of a compact object in the source 3C 144 on inhomogeneities in the electron density of the solar wind plasma over a wide range of elongation on the URAN-1 and URAN-4 radio interferometers with baselines 42.3 and 613 km are presented. The experimental relationships obtained are compared with calculations made for a power law inhomogeneity spectrum. Dependences of the results of the calculations on a number of solar wind plasma parameters are presented, and probable values for these parameters are estimated.

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