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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
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 sciences |
| Research Field: | Solar physics |
| Objective Division: | Expanding Knowledge |
| Objective Group: | Expanding knowledge |
| Objective Field: | Expanding knowledge in the physical sciences |
| UTAS Author: | Cane, HV (Dr Hilary Cane) |
| ID Code: | 110771 |
| Year Published: | 2013 |
| Web of Science® Times Cited: | 3 |
| Deposited By: | Mathematics and Physics |
| Deposited On: | 2016-08-12 |
| Last Modified: | 2016-09-05 |
| Downloads: | 0 |
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