Coronal magnetic field structure derived
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K. Kai; K. V. Sheridan
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Article
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1974
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Springer
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English
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An exceptional variety of positions and polarizations was found for two type I storms and numerous sporadic bursts observed during 15 consecutive days with the Culgoora radioheliograph at 80 and 160 MHz. The radio data are combined with optical data to derive a model of the coronal magnetic field st