anisotropic scaling features and complexity in magnetospheric-cusp: a case study

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ID: 179915
2005
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Abstract
Magnetospheric cusps are high-latitude regions characterized by a highly turbulent plasma, playing a special role in the solar wind-magnetosphere interaction. Here, using POLAR satellite magnetic field vector measurements we investigate the anisotropic scaling features of the magnetic field fluctuations in the northern cusp region. Our results seem to support the hypothesis of a 2D-MHD turbulent scenario which is consequence of a strong background magnetic field. The observed turbulent fluctuations reveal a high degree of complexity, which might be due to the interplay of many competing scales. A discussion of our findings in connection with the complex scenario proposed by Chang et al. (2004) is provided.
Reference Key
yordanova2005nonlinearanisotropic Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;E. Yordanova;E. Yordanova;J. Bergman;J. Bergman;G. Consolini;M. Kretzschmar;M. Materassi;M. Materassi;B. Popielawska;M. Roca-Sogorb;K. Stasiewicz;A. W. Wernik
Journal BMC research notes
Year 2005
DOI
DOI not found
URL
http://www.nonlin-processes-geophys.net/12/817/2005/npg-12-817-2005.pdf
Keywords
cosmic physics sciencephysicsgeophysics

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