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| Titel |
The extreme solar storm of May 1921: observations and a complex topological model |
| VerfasserIn |
H. Lundstedt, T. Persson, V. Andersson |
| Medientyp |
Artikel
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| Sprache |
Englisch
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| ISSN |
0992-7689
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| Digitales Dokument |
URL |
| Erschienen |
In: Annales Geophysicae ; 33, no. 1 ; Nr. 33, no. 1 (2015-01-27), S.109-116 |
| Datensatznummer |
250121154
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| Publikation (Nr.) |
 copernicus.org/angeo-33-109-2015.pdf |
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| Zusammenfassung |
| 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. |
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