On Self‐Similar and Multifractal Models for the Scaling of Extreme Bursty Fluctuations in Space Plasmas

This chapter contains sections titled: Introduction Motivation for a Self‐Similar, Stable, Description Data Sets Used General Consequences of any Self‐Similar Model Specific Consequences of a Particular Choice of Self‐Similar Model Limitations of the LFSM Model Conclusions

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Bibliographic Details
Published inExtreme Events and Natural Hazards: The Complexity Perspective pp. 299 - 313
Main Authors Watkins, N. W, Hnat, B, Chapman, S. C
Format Book Chapter
LanguageEnglish
Published Washington, D. C American Geophysical Union 01.01.2012
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ISBN0875904866
9780875904863
DOI10.1029/2011GM001084

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Summary:This chapter contains sections titled: Introduction Motivation for a Self‐Similar, Stable, Description Data Sets Used General Consequences of any Self‐Similar Model Specific Consequences of a Particular Choice of Self‐Similar Model Limitations of the LFSM Model Conclusions
ISBN:0875904866
9780875904863
DOI:10.1029/2011GM001084