Artículo
Emergence of intermittent structures and reconnection in MHD turbulence
Fecha de publicación:
09/2010
Editorial:
CUP
Revista:
Proceedings of the International Astronomical Union
ISSN:
1743-9221
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
In recent analyses of numerical simulation and solar wind dataset, the idea that the magnetic discontinuities may be related to intermittent structures that appear spontaneously in MHD turbulence has been explored in details. These studies are consistent with the hypothesis that discontinuity events founds in the solar wind might be of local origin as well, i.e. a by-product of the turbulent evolution of magnetic fluctuations. Using simulations of 2D MHD turbulence, we are exploring a possible link between tangential discontinuities and magnetic reconnection. The goal is to develop numerical algorithms that may be useful for solar wind applications. © 2011 International Astronomical Union.
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Articulos(IFIBA)
Articulos de INST.DE FISICA DE BUENOS AIRES
Articulos de INST.DE FISICA DE BUENOS AIRES
Citación
Greco, Antonella; Servidio, Sergio; Matthaeus, William H.; Dmitruk, Pablo Ariel; Emergence of intermittent structures and reconnection in MHD turbulence; CUP; Proceedings of the International Astronomical Union; 6; S274; 9-2010; 116-119
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