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 variable <i>x</i>(<i>t</i>) may denote any solar wind scalar field...
Main Authors: | E. Marsch, C. Y. Tu |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
1994-12-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/12/1127/1994/angeo-12-1127-1994.pdf |
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