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Recurrent substorm activity during the passage of a corotating interaction region

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
1364-6826
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
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), 1073-1081. (doi:10.1016/j.jastp.2008.11.009).

Record type: Article

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.

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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

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Date deposited: 22 Apr 2010 14:11
Last modified: 14 Mar 2024 00:56

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Contributors

Author: S.K. Morley
Author: A.P. Rouillard
Author: M.P. Freeman

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