A study of non-extensivity in the Earth’s magnetosphere
Magnetic storms are undoubtedly among the most important phenomena in space physics and also a central subject of space weather. The non-extensive Tsallis entropy has been recently introduced, as an effective complexity measure for the analysis of the geomagnetic activity D st index. Tsallis entropy...
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| Published in | The European physical journal. ST, Special topics Vol. 174; no. 1; pp. 219 - 225 |
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| Main Authors | , |
| Format | Journal Article |
| Language | English |
| Published |
Berlin/Heidelberg
Springer-Verlag
01.07.2009
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| Subjects | |
| Online Access | Get full text |
| ISSN | 1951-6355 1951-6401 |
| DOI | 10.1140/epjst/e2009-01102-y |
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| Summary: | Magnetic storms are undoubtedly among the most important phenomena in space physics and also a central subject of space weather. The non-extensive Tsallis entropy has been recently introduced, as an effective complexity measure for the analysis of the geomagnetic activity
D
st
index. Tsallis entropy has been shown to sensitively detect the complexity dissimilarity between pre-storm activity and intense magnetic storms in the Earth’s magnetosphere. Here, we show that the
D
st
time series obey a modified form of the Gutenberg-Richter law for the case of non-extensive statistics, thus providing evidence for universality in magnetic storm and earthquake occurrence. |
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| Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
| ISSN: | 1951-6355 1951-6401 |
| DOI: | 10.1140/epjst/e2009-01102-y |