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Eruptive Prominences and Long-Delay Geomagnetic Storms

Published online by Cambridge University Press:  25 April 2016

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

Information

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 2 , 1983 , pp. 198 - 202
Copyright
Copyright © Astronomical Society of Australia 1983

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References

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