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The extreme solar s...
The extreme solar storm of May 1921: observations and a complex topological model
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Lundstedt, H. (author)
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- Persson, Tomas (author)
- Lund University,Lunds universitet,Dynamiska system,Forskargrupper vid Lunds universitet,Matematik LTH,Matematikcentrum,Institutioner vid LTH,Lunds Tekniska Högskola,Dynamical systems,Lund University Research Groups,Mathematics (Faculty of Engineering),Centre for Mathematical Sciences,Departments at LTH,Faculty of Engineering, LTH
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Andersson, V. (author)
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(creator_code:org_t)
- 2015-01-27
- 2015
- English.
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In: Annales Geophysicae. - : Copernicus GmbH. - 1432-0576. ; 33:1, s. 109-116
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Abstract
Subject headings
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- A complex solid torus model was developed in order to be able to study an extreme solar storm, the so-called "Great Storm" or "New York Railroad Storm" of May 1921, when neither high spatial and time resolution magnetic field measurements, solar flare nor coronal mass ejection observations were available. We suggest that a topological change happened in connection with the occurrence of the extreme solar storm. The solar storm caused one of the most severe space weather effects ever.
Subject headings
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- Solar physics astrophysics and astronomy
- magnetic fields
Publication and Content Type
- art (subject category)
- ref (subject category)
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