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Eruptive Prominences and Long-Delay Geomagnetic Storms

Published online by Cambridge University Press:  25 April 2016

C. S. Wright*
Affiliation:
Ionospheric Prediction Service, Dept. of Science & Technology

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.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1983

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References

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