Radial evolution of solar wind intermittency in the inner heliosphere

We analyzed intermittency in the solar wind, as observed on the ecliptic plane, looking at magnetic field and velocity fluctuations between 0.3 and 1 AU, for both fast and slow wind and for compressive and directional fluctuations. Our analysis focused on the property that probability distribution f...

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Veröffentlicht in:	Journal of Geophysical Research. A. Space Physics 2003-03, Vol.108 (A3), p.n/a
Hauptverfasser:	Bruno, R., Carbone, V., Sorriso-Valvo, L., Bavassano, B.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy coherent structures Earth, ocean, space Exact sciences and technology intermittency interplanetary fluctuations Interplanetary space Solar system Solar wind plasma stochastic F1
Online-Zugang:	Volltext
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