Anisotropy of interplanetary plasma irregularities

Details Anisotropy of interplanetary plasma irregularities Anisotropy of interplanetary plasma irregularities

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..665c&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Dec. 1979, p. 665-668.) Soviet Astronomy Letters, vol. 5, Nov.-Dec. 1979, p. 356, 35

Astronomy and Astrophysics

Astronomy

1

Anisotropy, Cosmic Plasma, Interplanetary Gas, Magnetoacoustic Waves, Plasma Turbulence, Radio Waves, Wave Scattering, Interplanetary Magnetic Fields, Irregularities, Radio Sources (Astronomy), Refractivity, Solar Wind Velocity, Turbulence Models

Scientific paper

An analysis is made of the anisotropy in the scattering angle of radiation from a distant radio source passing through interplanetary plasma with magneto-acoustic turbulence. Comparison of theory and experiment shows that the observed scattering anisotropy agrees very well with the magneto-acoustic turbulence model. At distances R = 20-30 solar radii from the sun the magnetic field is nearly radial. In the zone R less than 10 solar radii either the radial field is replaced by an azimuthal field, or there is an additional isotropic turbulence which is absent at R greater than 20 solar radii.

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