VLF, magnetic and Pi2 substorm signatures
We carried out a superposed epoch analysis, using a database of substorm chorus events observed at Halley, Antarctica, within an hour of magnetic midnight, to define a set of 123 substorm expansion phase onsets. The method is applied to the 3-component ground magnetic field variations and Pi2 pulsat...
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2000
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ftnerc:oai:nora.nerc.ac.uk:502406 2024-02-04T09:55:49+01:00 VLF, magnetic and Pi2 substorm signatures Smith, A.J. Freeman, M.P. Hunter, S. Wilson, A. 2000 http://nora.nerc.ac.uk/id/eprint/502406/ unknown European Space Agency Smith, A.J.; Freeman, M.P. orcid:0000-0002-8653-8279 Hunter, S. 2000 VLF, magnetic and Pi2 substorm signatures. In: Wilson, A., (ed.) Proceedings of the Fifth International Conference on Substorms, St. Petersburg, Russia, May 2000. European Space Agency, 577-578. (European Space Agency Special Paper, 443). Atmospheric Sciences Publication - Book Section PeerReviewed 2000 ftnerc 2024-01-05T00:03:05Z We carried out a superposed epoch analysis, using a database of substorm chorus events observed at Halley, Antarctica, within an hour of magnetic midnight, to define a set of 123 substorm expansion phase onsets. The method is applied to the 3-component ground magnetic field variations and Pi2 pulsation power. The results may be considered in some sense the "typical" substorm signature at the station when located close to the substorm current wedge. Book Part Antarc* Antarctica Natural Environment Research Council: NERC Open Research Archive |
institution |
Open Polar |
collection |
Natural Environment Research Council: NERC Open Research Archive |
op_collection_id |
ftnerc |
language |
unknown |
topic |
Atmospheric Sciences |
spellingShingle |
Atmospheric Sciences Smith, A.J. Freeman, M.P. Hunter, S. VLF, magnetic and Pi2 substorm signatures |
topic_facet |
Atmospheric Sciences |
description |
We carried out a superposed epoch analysis, using a database of substorm chorus events observed at Halley, Antarctica, within an hour of magnetic midnight, to define a set of 123 substorm expansion phase onsets. The method is applied to the 3-component ground magnetic field variations and Pi2 pulsation power. The results may be considered in some sense the "typical" substorm signature at the station when located close to the substorm current wedge. |
author2 |
Wilson, A. |
format |
Book Part |
author |
Smith, A.J. Freeman, M.P. Hunter, S. |
author_facet |
Smith, A.J. Freeman, M.P. Hunter, S. |
author_sort |
Smith, A.J. |
title |
VLF, magnetic and Pi2 substorm signatures |
title_short |
VLF, magnetic and Pi2 substorm signatures |
title_full |
VLF, magnetic and Pi2 substorm signatures |
title_fullStr |
VLF, magnetic and Pi2 substorm signatures |
title_full_unstemmed |
VLF, magnetic and Pi2 substorm signatures |
title_sort |
vlf, magnetic and pi2 substorm signatures |
publisher |
European Space Agency |
publishDate |
2000 |
url |
http://nora.nerc.ac.uk/id/eprint/502406/ |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_relation |
Smith, A.J.; Freeman, M.P. orcid:0000-0002-8653-8279 Hunter, S. 2000 VLF, magnetic and Pi2 substorm signatures. In: Wilson, A., (ed.) Proceedings of the Fifth International Conference on Substorms, St. Petersburg, Russia, May 2000. European Space Agency, 577-578. (European Space Agency Special Paper, 443). |
_version_ |
1789959986674139136 |