Author： Sorriso-Valvo Luca Carbone Vincenzo Bruno Roberto
Publisher： Springer Publishing Company
ISSN： 0038-6308
Source： Space Science Reviews, Vol.121, Iss.1-4, 2005-11, pp. : 49-53
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Abstract
We briefly discuss the strong intermittent nature of the interplanetary magnetic field, observing that similarity between its statistical properties and the passive scalar ones exists, and may arise from different dynamical mechanisms.
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