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Near-Earth solar wind flows and geomagnetic activity over more than four solar cycles (1963-2011)
conference contribution
posted on 2023-05-23, 11:18 authored by Richardson, IG, Hilary CaneUsing 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.
History
Publication title
Proceedings of the 13th International Solar Wind ConferenceEditors
GP ZankPagination
426-429ISSN
0094-243XDepartment/School
School of Natural SciencesPublisher
AIP PublishingPlace of publication
USAEvent title
13th International Solar Wind ConferenceEvent Venue
Hawaii, USADate of Event (Start Date)
2012-06-17Date of Event (End Date)
2012-06-22Rights statement
Copyright 2013 AIP PublishingRepository Status
- Restricted