Non-Gaussian probability distributions of solar wind fluctuations

The probability distributions of field differences &#x2206;<i>x</i>(&#x03C4;)=<i>x</i>(<i>t</i>+&#x03C4;)-<i>x</i>(<i>t</i>), where the variable <i>x</i>(<i>t</i>) may denote any solar wind scalar field...

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Bibliographic Details
Main Authors: E. Marsch, C. Y. Tu
Format: Article
Language:English
Published: Copernicus Publications 1994-12-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/12/1127/1994/angeo-12-1127-1994.pdf

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