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...

Full description

Saved in:
Bibliographic Details
Published inThe European physical journal. ST, Special topics Vol. 174; no. 1; pp. 219 - 225
Main Authors Balasis, G., Eftaxias, K.
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer-Verlag 01.07.2009
Subjects
Online AccessGet full text
ISSN1951-6355
1951-6401
DOI10.1140/epjst/e2009-01102-y

Cover

More Information
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.
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