A comparison of Type III metric radio bursts and global solar potential field models

Details A comparison of Type III metric radio bursts and global solar potential field models A comparison of Type III metric radio bursts and global solar potential field models

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...73..183j&link_type=abstract

Solar Physics, vol. 73, Sept. 1981, p. 183-190.

Physics

3

Polarized Radiation, Potential Fields, Solar Corona, Solar Magnetic Field, Solar Radiation, Type 3 Bursts, Circular Polarization, H Alpha Line, Photosphere

Scientific paper

Evidence of coronal magnetic fields from polarized metric type III radio bursts is compared with (1) global potential field models, (2) direct averages of the observed photospheric magnetic field, and (3) H-alpha synoptic charts. The comparison clearly indicates both that the principal aspects of type III burst radiation are understood and that global potential field models are a significantly more accurate representation of coronal magnetic field structure than either the large-scale photospheric field or H-alpha synoptic charts.

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