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Emergence of intermittent structures and reconnection in MHD turbulence

Published online by Cambridge University Press:  08 June 2011

Antonella Greco ,
Sergio Servidio ,
William H. Matthaeus  and
Pablo Dmitruk
Antonella Greco
Affiliation:
Dipartimento di Fisica Università della Calabria, Rende (CS), Italy email: [email protected]
Sergio Servidio
Affiliation:
Dipartimento di Fisica Università della Calabria, Rende (CS), Italy email: [email protected]
William H. Matthaeus
Affiliation:
Bartol Research Institute, University of Delaware, Newark DE, United States
Pablo Dmitruk
Affiliation:
Departamento de Física (FCEN-UBA), Buenos Aires, Argentina
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Abstract

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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.

Keywords

(magnetohydrodynamics:) MHDturbulence(Sun:) solar windmethods: numerical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 116 - 119
Copyright
Copyright © International Astronomical Union 2011

References

Borovsky, J. 2008, J. Geophys Res., 113, A08110.Google Scholar
Burlaga, L. F. 1968, Solar Physics, 4, 67.CrossRefGoogle Scholar
Greco, A., Chuychai, P., Matthaeus, W. H., Servidio, S., & Dmitruk, P. 2008, Geophys. Res. Lett., 35, L19111, 2008GL035454.CrossRefGoogle Scholar
Greco, A., Matthaeus, W. H., Servidio, S., Chuychai, P. & Dmitruk, P. 2009, Astrophys. J., 691, L111.CrossRefGoogle Scholar
Greco, A., Matthaeus, W. H., Servidio, S., & Dmitruk, P. 2009, Phys. Rev. E, 80, 046401.CrossRefGoogle Scholar
Matthaeus, W. H., & Lamkin, S. L. 1986, Physics of Fluids, 29, 2513.CrossRefGoogle Scholar
Servidio, S., Matthaeus, W. H., Shay, M. A., Cassak, P. A., & Dmitruk, P. 2009, Phys. Rev. Lett., 102, 115003.CrossRefGoogle Scholar
Servidio, S., Matthaeus, W. H., Shay, M. A., Dmitruk, P., Cassak, P. A., & Wan, M. 2010, Phys. Plasmas, 17, 032315.CrossRefGoogle Scholar
Tsurutani, B. T. & Smith, E. J. 1979, J. Geophys. Res., 84, 2773.CrossRefGoogle Scholar