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Solar wind drivers of geomagnetic storms over more than four solar cycles

Citation

Richardson, IG and Cane, HV, Solar wind drivers of geomagnetic storms over more than four solar cycles, Proceedings of the 13th International Solar Wind Conference, 17-22 June 2012, Hawaii, USA, pp. 422-425. ISSN 0094-243X (2013) [Refereed Conference Paper]


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Copyright Statement

Copyright 2013 AIP Publishing

DOI: doi:10.1063/1.4811075

Abstract

Using a classification of near-Earth solar wind flows into corotating high-speed streams, slow interstream solar wind, and transients originating with coronal mass ejections at the Sun, we determine the drivers of geomagnetic storms of various sizes from 1964 to 2011 based on the Kp index, encompassing more than four solar cycles. We also briefly discuss storm occurrence rates since the beginning of Kp in 1932.

Item Details

Item Type:Refereed Conference Paper
Keywords:Solar wind, interplanetary magnetic field, geomagnetic storms, solar cycle variation
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Space and Solar Physics
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:Cane, HV (Dr Hilary Cane)
ID Code:110770
Year Published:2013
Deposited By:Mathematics and Physics
Deposited On:2016-08-12
Last Modified:2016-09-05
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