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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
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 |
| Deposited By: | Mathematics and Physics |
| Deposited On: | 2016-08-12 |
| Last Modified: | 2022-06-29 |
| Downloads: | 0 |
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