Anisotropic scaling features and complexity in magnetospheric-cusp: a case study (Articolo in rivista)

Type
Label
  • Anisotropic scaling features and complexity in magnetospheric-cusp: a case study (Articolo in rivista) (literal)
Anno
  • 2005-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.5194/npg-12-817-2005 (literal)
Alternative label
  • Yordanova E.; Bergman J.; Consolini G.; Kretzschmar M.; Materassi M.; Popielawska B.; Roca-Sogorb M.; Stasiewicz K.; Wernik A.W. (2005)
    Anisotropic scaling features and complexity in magnetospheric-cusp: a case study
    in Nonlinear processes in geophysics
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Yordanova E.; Bergman J.; Consolini G.; Kretzschmar M.; Materassi M.; Popielawska B.; Roca-Sogorb M.; Stasiewicz K.; Wernik A.W. (literal)
Pagina inizio
  • 817 (literal)
Pagina fine
  • 825 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
  • http://www.nonlin-processes-geophys.net/12/817/2005/npg-12-817-2005.html (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 12(6) (literal)
Rivista
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#note
  • European Geosciences Union and the American Geophysical Union ; Authors - Creative Commons. Part of Special Issue “Nonlinear and multiscale phenomena in space plasmas”, eds: J. Büchner, S. Chapman, A. Chian, A. S. Sharma, D. Vassiliadis, and N. Watkins. (literal)
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • 1) Space Research Center, Polish Academy of Sciences, Warsaw, Poland 2) Space Research Institute, Bulgarian Academy of Sciences, Sofia, Bulgaria 3) Swedish Institute of Space Physics, Uppsala, Sweden 4) Istituto di Fisica dello Spazio Interplanetario, INAF, Roma, Italy 5) Istituto di Fisica dei Sistemi Complessi, CNR, Firenze, Italy (literal)
Titolo
  • Anisotropic scaling features and complexity in magnetospheric-cusp: a case study (literal)
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. (literal)
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