Characterization of intermittent structures in the solar wind

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, Maria Soledad, Ruiz, Maria Emilia, Dasso, Sergio Ricardo
Publicado:	2013
Materias:	Intermittency Magnetohydrodynamic turbulence Solar Wind
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v8_nS300_p485_Nakwacki http://hdl.handle.net/20.500.12110/paper_17439213_v8_nS300_p485_Nakwacki
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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