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On the scaling properties of anisotropy of interplanetary magnetic turbulent fluctuations
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Swedish Institute of Space Physics, Uppsala Division.
2010 (English)In: Europhysics letters, ISSN 0295-5075, E-ISSN 1286-4854, Vol. 90, no 5, 59001- p.Article in journal (Refereed) Published
Abstract [en]

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.

Place, publisher, year, edition, pages
2010. Vol. 90, no 5, 59001- p.
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:uu:diva-147197DOI: 10.1209/0295-5075/90/59001ISI: 000280061500032OAI: oai:DiVA.org:uu-147197DiVA: diva2:400301
Available from: 2011-02-25 Created: 2011-02-24 Last updated: 2017-12-11Bibliographically approved

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