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

✍ Scribed by Bernard V. Jackson; Randolph H. Levine

Publisher
Springer
Year
1981
Tongue
English
Weight
391 KB
Volume
73
Category
Article
ISSN
0038-0938

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✦ Synopsis

We compare evidence of coronal magnetic fields from polarized metric type III radio bursts with (a) global potential field models, (b) direct averages of the observed photospheric magnetic field, and (c) Ha 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 Ha synoptic charts.

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