Interplanetary magnetic Taylor microscale and implications for plasma dissipation

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The Taylor microscale, a measure of mean square spatial derivatives, is evaluated for interplanetary magnetic field fluctuations from single- and multiple-point data using Cluster and ACE spacecraft data. The Taylor scale is compared to the measured inner scale, which for hydrodynamics would corresp...

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Detalles Bibliográficos
Autores principales: Matthaeus, W.H., Weygand, J.M., Chuychai, P., Dasso, S., Smith, C.W., Kivelson, M.G.
Formato: Artículo publishedVersion
Publicado: 2008
Materias:
Interplanetary medium
Magnetic fields
Methods: data analysis
Plasmas
Solar wind
Turbulence
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v678_n2PART2_pL141_Matthaeus
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0004637X_v678_n2PART2_pL141_Matthaeus_oai
Aporte de:
Repositorio Digital de la Universidad de Buenos Aires (UBA) de Universidad de Buenos Aires

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