Interplanetary-magnetosphere coupling during intense geomagnetic storms at solar maximum

Main Article Content

W. D. González
A. L. Clua de González
B. T. Tsurutani

Abstract

During the interval of August 16. 1978 - December 28. 1979,90% of the intense geomagnetic storms CDst < -l00nD were preceded by the arrival of interplanetary fast forward shocks at 1AU. as identified with magnetic field and plasma data collected by the ISEE-3 spacecraft. For these events we discuss the interplanetary structures that are associated with the -large-amplitude and long-duration negative Bz fields that are thought to be the main cause of the intense storms. We also present a summary of the interplanetary-magnetosphere coupling functions, based on the magnetopause reconnection process. We end by an overview of the long-term evolution of intense geomagnetic storms such as those associated to the seasonal and solar cycle distributions.

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How to Cite
González, W. D., Clua de González, A. L., & Tsurutani, B. T. (1992). Interplanetary-magnetosphere coupling during intense geomagnetic storms at solar maximum. Geofisica Internacional, 31(1), 11–18. https://doi.org/10.22201/igeof.00167169p.1992.31.1.1299
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References

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