Properties of coronal Alfven waves from polarized radio occultation experiments

Details Properties of coronal Alfven waves from polarized radio occultation experiments Properties of coronal Alfven waves from polarized radio occultation experiments

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20...65a&link_type=abstract

Advances in Space Research, vol. 20, p. 65

Computer Science

Sound

2

Solar Corona, Magnetohydrodynamic Waves, Radio Occultation, Linear Polarization, Radio Probing, Helios Satellites, Spectrum Analysis, Faraday Effect, Solar Diameter

Scientific paper

A spectral analysis is conducted of polarization angle measurements from coronal radio-sounding experiments using the linearly-polarized Helios signals. The level of Faraday rotation fluctuations, at 1 to 15 min characteristic periods, are determined for heliocentric distances of 3 and 16 solar radii; magnetic field amplitudes generated by Alfven waves are then derived from the fluctuations by a new technique.

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