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MODEL OF RECONNECTION OF WEAKLY STOCHASTIC MAGNETIC FIELD AND ITS IMPLICATIONS

We discuss the model of magnetic eld reconnection in the presence of turbulence introduced by us ten years ago. The model does not require any plasma e ects to be involved in order to make the reconnection fast. In fact, it shows that the degree of magnetic eld stochasticity controls the reconnectio...

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Publié dans:Revista Mexicana de Astronomía y Astrofísica
Auteurs principaux: A. Lazarian, E. Vishniac
Format: Artigo
Langue:Inglês
Publié: Universidad Nacional Autónoma de México 2009
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Accès en ligne:https://www.redalyc.org/articulo.oa?id=57115743013
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