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Scale-free texture of the fast solar wind

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Hnat, B., Chapman, Sandra C., Gogoberidze, G. and Wicks, R. T. (2011) Scale-free texture of the fast solar wind. Physical Review E, Volume 84 (Number 6). Article number 065401. doi:10.1103/PhysRevE.84.065401 ISSN 1539-3755.

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Official URL: http://dx.doi.org/10.1103/PhysRevE.84.065401

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Abstract

The higher-order statistics of magnetic field magnitude fluctuations in the fast quiet solar wind are quantified systematically, scale by scale. We find a single global non-Gaussian scale-free behavior from minutes to over 5 h. This spans the signature of an inertial range of magnetohydrodynamic turbulence and a ∼1/f range in magnetic field components. This global scaling in field magnitude fluctuations is an intrinsic component of the underlying texture of the solar wind and puts a strong constraint on any theory of solar corona and the heliosphere. Intriguingly, the magnetic field and velocity components show scale-dependent dynamic alignment outside of the inertial range.

Item Type: Journal Article
Divisions: Faculty of Science, Engineering and Medicine > Science > Physics
Journal or Publication Title: Physical Review E
Publisher: American Physical Society
ISSN: 1539-3755
Official Date: December 2011
Dates:
DateEvent
December 2011Published
Volume: Volume 84
Number: Number 6
Article Number: Article number 065401
DOI: 10.1103/PhysRevE.84.065401
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access

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