Recurrent substorm activity during the passage of a corotating interaction region
Recurrent substorm activity during the passage of a corotating interaction region
Recent observations of magnetospheric dynamics driven by interaction with both high-speed solar wind streams (HSSs) and interplanetary coronal mass ejections (ICMEs) have shown periodic substorms to be common under strong driving, but with different periods of 4 and 2–3 h, respectively. However, it is unclear what causes these substorms and what determines their periodicity. Observations during the passage of a corotating interaction region preceding a high-speed stream are presented here and the observed enhancements in the AE index are shown to be a quasi-periodic sequence of substorms. The occurrence times of these substorms and the variation of the AL index are shown to be consistent with a simple loading–unloading model without the need for external triggers. A possible explanation is given for the lengthening of the inter-substorm period during HSS relative to that of sawtooth events during ICMEs.
magnetospheric substorms, corotating interaction regions, high-speed solar wind streams, space weather
1073-1081
Morley, S.K.
60f13cee-88bd-4c88-891b-09d239c7b03d
Rouillard, A.P.
54aa9107-0da0-4006-88cc-b7b0f7b2aa14
Freeman, M.P.
ca34cfc2-086e-4b43-9cb1-921ccbdadb10
July 2009
Morley, S.K.
60f13cee-88bd-4c88-891b-09d239c7b03d
Rouillard, A.P.
54aa9107-0da0-4006-88cc-b7b0f7b2aa14
Freeman, M.P.
ca34cfc2-086e-4b43-9cb1-921ccbdadb10
Morley, S.K., Rouillard, A.P. and Freeman, M.P.
(2009)
Recurrent substorm activity during the passage of a corotating interaction region.
Journal of Atmospheric and Solar-Terrestrial Physics, 71 (10-11), .
(doi:10.1016/j.jastp.2008.11.009).
Abstract
Recent observations of magnetospheric dynamics driven by interaction with both high-speed solar wind streams (HSSs) and interplanetary coronal mass ejections (ICMEs) have shown periodic substorms to be common under strong driving, but with different periods of 4 and 2–3 h, respectively. However, it is unclear what causes these substorms and what determines their periodicity. Observations during the passage of a corotating interaction region preceding a high-speed stream are presented here and the observed enhancements in the AE index are shown to be a quasi-periodic sequence of substorms. The occurrence times of these substorms and the variation of the AL index are shown to be consistent with a simple loading–unloading model without the need for external triggers. A possible explanation is given for the lengthening of the inter-substorm period during HSS relative to that of sawtooth events during ICMEs.
This record has no associated files available for download.
More information
Published date: July 2009
Keywords:
magnetospheric substorms, corotating interaction regions, high-speed solar wind streams, space weather
Identifiers
Local EPrints ID: 146831
URI: http://eprints.soton.ac.uk/id/eprint/146831
ISSN: 1364-6826
PURE UUID: 0b290c33-73e2-42ea-957e-7ddd85440da8
Catalogue record
Date deposited: 22 Apr 2010 14:11
Last modified: 14 Mar 2024 00:56
Export record
Altmetrics
Contributors
Author:
S.K. Morley
Author:
A.P. Rouillard
Author:
M.P. Freeman
Download statistics
Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.
View more statistics