Non-Gaussian probability distributions of solar wind fluctuations

The probability distributions of field differences ∆<i>x</i>(τ)=<i>x</i>(<i>t</i>+τ)-<i>x</i>(<i>t</i>), where the...

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Bibliographic Details
Main Authors: E. Marsch, C. Y. Tu
Format: Article
Language:English
Published: Copernicus Publications
Series:Annales Geophysicae
Online Access:http://www.ann-geophys.net/12/1127/1994/angeo-12-1127-1994.html