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Nonlinear Processes in Geophysics 2009

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. [PUBLICATION ABSTRACT]

Details

Title
A probabilistic approach to heterogeneity in space plasmas: the case of magnetic field intensity in solar wind
Author
Consolini, G.; Bavassano, B.; De Michelis, P.
Pages
265
Publication year
2009
Publication date
2009
Publisher
Copernicus GmbH
ISSN
1023-5809
e-ISSN
1607-7946
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
519651002
Copyright
Nonlinear Processes in Geophysics 2009