Polarisation of type III bursts between 164 and 435 MHz - Structure and variation with frequency

Details Polarisation of type III bursts between 164 and 435 MHz - Structure and variation with frequency Polarisation of type III bursts between 164 and 435 MHz - Structure and variation with frequency

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..130..119m&link_type=abstract

(Committee of European Radio Astronomers, SNSF, URSI, et al., Workshop on Particle Beams in the Solar Atmosphere, Braunwald, Swi

Physics

7

Polarization (Waves), Solar Corona, Type 3 Bursts, Circular Polarization, Harmonics, Solar Magnetic Field, Spatial Resolution, Very High Frequencies

Scientific paper

The first observations of circular polarization in type III bursts with spatial resolution in the range 164-435 MHz are presented. The degree of polarization is in general neither constant nor uniform over burst extent, and increases with frequency. Observations are discussed and it is proposed that they give access to the inhomogeneity of the coronal magnetic field and its variation with height.

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