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Eruptive Prominences and Long-Delay Geomagnetic Storms
Published online by Cambridge University Press: 25 April 2016
Extract
During recent years a firm relationship has been established between disappearing solar fragments and geomagnetic disturbances (Joselyn and McIntosh 1981; McNamara and Wright 1982; Wright and McNamara 1983). Wright and McNamara (1983) showed that the average magnitude and delay of the geomagnetic disturbance depended upon the size of the filament.
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- Copyright © Astronomical Society of Australia 1983
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