On the long-term behaviour of the circular polarization from coronal condensation radio emission at 4.3 cm wavelength

Details On the long-term behaviour of the circular polarization from coronal condensation radio emission at 4.3 cm wavelength On the long-term behaviour of the circular polarization from coronal condensation radio emission at 4.3 cm wavelength

Nov 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972soph...27..203d&link_type=abstract

Solar Physics, Volume 27, Issue 1, pp.203-207

Physics

1

Scientific paper

The circular polarization from coronal condensations at λ = 4.3 cm correspond to the extraordinary mode of propagation, due to the contribution of preceding spots' polarities, being usually left-handed. The fewer cases of right-handed polarization are normally associated to an excess of sunspot plages in the southern hemisphere, thus making it difficult to give evidence for magnetoionic coupling phenomena as a general rule.

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