Characterization of intermittent structures in the solar wind

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The solar wind (SW) is a suitable natural scenario to study the intermittent nature of magnetohydrodynamic (MHD) turbulence for systems with low dissipation rate. In particular, nonlinear wave-wave interactions can be characterized by the degree of phase correlation and by departures from Gaussianit...

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Detalles Bibliográficos
Autores principales:	Nakwacki, M.S., Ruiz, M.E., Dasso, S.
Formato:	Artículo publishedVersion
Publicado:	2013
Materias:	Intermittency Magnetohydrodynamic turbulence Solar Wind
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_17439213_v8_nS300_p485_Nakwacki https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_17439213_v8_nS300_p485_Nakwacki_oai
Aporte de:	Repositorio Digital de la Universidad de Buenos Aires (UBA) de Universidad de Buenos Aires

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