Radio method of mapping large-scale coronal magnetic fields on active stars

Details Radio method of mapping large-scale coronal magnetic fields on active stars Radio method of mapping large-scale coronal magnetic fields on active stars

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986natur.320..509s&link_type=abstract

Nature (ISSN 0028-0836), vol. 320, April 10, 1986, p. 509, 510.

Other

Late Stars, Solar Magnetic Field, Stellar Atmospheres, Stellar Magnetic Fields, Circular Polarization, Magnetic Storms, Radio Stars, Stellar Activity

Scientific paper

The author describes a radio method which measures the longitudinal magnetic sector structure of the solar corona by observing the Sun 'as a star' and monitoring the sense of circular polarization of metre-wavelength emission as a function of rotational phase. The method is tested by comparing synoptic plots of solar radio-noise-storm polarities derived from high- and low-resolution observations over a period of four years at Culgoora. This method may be applied to the measurement of large-scale coronal fields on other active stars.

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