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Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/5031

Authors: Consolini, G.*
Bavassano, B.*
De Michelis, P.*
Title: A probabilistic approach to heterogeneity in space plasmas: the case of magnetic field intensity in solar wind
Title of journal: Nonlinear Processes in Geophysics
Series/Report no.: / 16 (2009)
Publisher: EGU/AGU - Copernicus Publications
Issue Date: 7-Apr-2009
URL: http://www.nonlin-processes-geophys.net/16/265/2009/
Keywords: fluctuations in space plasmas
heterogeneity
statistical features
solar wind
Abstract: Since the early 90s it was shown that Probability Distribution Functions (PDFs) of small scale differences (fluctuations) of several quantities in space plasmas display significant departures from Gaussianity. The non-Gaussian shape of PDFs was ascribed to intermittency and discussed in the framework of intermittent MHD turbulence. Here, we put the attention to the PDF of magnetic field intensity instead of its differences showing how the PDF of such quantity in a quiet solar wind can be related with the occurrence of heterogeneity. In detail, we derive the shape of the PDFs by simple statistical considerations based on the concept of subordination in probability theory. An interpretation and a discussion in terms of existing coherent magnetic structures in a mechanical near-equilibrium state are also presented.
Appears in Collections:01.03.01. Interplanetary physics
01.03.05. Solar variability and solar wind
Papers Published / Papers in press

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