On the scaling properties of anisotropy of interplanetary magnetic turbulent fluctuations

The anisotropic character of interplanetary magnetic-field turbulence has been studied through the analysis of Cluster data. The full tensor of the mixed second-order structure functions has been used to quatitatively measure the degree of anisotropy and its effect on small-scale turbulence. Three different regions of the near-Earth space have been studied, namely the solar wind, the Earth’s foreshock and magnetosheath. While in the undisturbed solar wind the observed strong anisotropy is mainly due to the large-scale magnetic field, near the magnetosphere other sources of anisotropy influence the magnetic-field properties.

On the scaling properties of anisotropy of interplanetary magnetic turbulent fluctuations / SORRISO VALVO, L; Yordanova, E; Carbone, Vincenzo. - In: EUROPHYSICS LETTERS. - ISSN 0295-5075. - 90(2010), p. 59001.



Titolo: On the scaling properties of anisotropy of interplanetary magnetic turbulent fluctuations
Autori: 
CARBONE, Vincenzo
mostra contributor esterni 
Data di pubblicazione: 2010
Rivista: 
EUROPHYSICS LETTERS  
Citazione: On the scaling properties of anisotropy of interplanetary magnetic turbulent fluctuations / SORRISO VALVO, L; Yordanova, E; Carbone, Vincenzo. - In: EUROPHYSICS LETTERS. - ISSN 0295-5075. - 90(2010), p. 59001.
Handle: http://hdl.handle.net/20.500.11770/134915
Appare nelle tipologie:1.1 Articolo in rivista

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http://hdl.handle.net/20.500.11770/134915
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