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Near-Earth solar wind flows and geomagnetic activity over more than four solar cycles (1963-2011)

Citation

Richardson, IG and Cane, HV, Near-Earth solar wind flows and geomagnetic activity over more than four solar cycles (1963-2011), Proceedings of the 13th International Solar Wind Conference, 17-22 June 2012, Hawaii, USA, pp. 426-429. ISSN 0094-243X (2013) [Refereed Conference Paper]


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Copyright Statement

Copyright 2013 AIP Publishing

Official URL: http://dx.doi.org/10.1063/1.4811076

DOI: doi:10.1063/1.4811075

Abstract

Using observations of solar wind plasma and magnetic field parameters and additional data (e.g., geomagnetic indicies, energetic particle and cosmic ray observations), we have classified the near-Earth solar wind during 1963 to 2011 into three basic flow types: high-speed streams associatedwith coronal holes at the Sun, slow, inter-stream flows, and transient ("CME-related") flows. We discuss the cycle-to-cycle variations in solar wind parameters and structures, and geomagnetic activity, over this period, encompassingmore than four solar cycles.

Item Details

Item Type:Refereed Conference Paper
Keywords:Solar wind, interplanetary magnetic field, geomagnetic activity, 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:110771
Year Published:2013
Deposited By:Mathematics and Physics
Deposited On:2016-08-12
Last Modified:2016-09-05
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