Lancaster EPrints

High-speed solar-wind streams and geospace interactions

Kavanagh, Andrew and Denton, Michael (2007) High-speed solar-wind streams and geospace interactions. Astronomy and Geophysics, 48 (6). 6.24-6.26. ISSN 1366-8781

Full text not available from this repository.

Abstract

High-speed solar-wind streams emanate from solar coronal holes; the fast wind interacts with upstream slow streams producing regions of enhanced magnetic field strength and particle density that are known as co-rotating interaction regions. Due to the recurring nature of coronal holes near solar minimum, this results in periodic driving of the magnetosphere that can last for several days and input as much energy as a storm driven by a coronal mass ejection.

Item Type: Article
Journal or Publication Title: Astronomy and Geophysics
Subjects: Q Science > QA Mathematics > QA75 Electronic computers. Computer science
Departments: Faculty of Science and Technology > School of Computing & Communications
Faculty of Science and Technology > Physics
ID Code: 6727
Deposited By: ep_importer_dcs
Deposited On: 03 Jul 2008 09:41
Refereed?: Yes
Published?: Published
Last Modified: 24 Oct 2013 11:06
Identification Number:
URI: http://eprints.lancs.ac.uk/id/eprint/6727

Actions (login required)

View Item