Magnetic reconnection in two-dimensional magnetohydrodynamic turbulence

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Systematic analysis of numerical simulations of two-dimensional magnetohydrodynamic turbulence reveals the presence of a large number of X-type neutral points where magnetic reconnection occurs. We examine the statistical properties of this ensemble of reconnection events that are spontaneously gene...

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Detalles Bibliográficos
Autor principal: Servidio, S.
Otros Autores: Matthaeus, W.H, Shay, M.A, Cassak, P.A, Dmitruk, P.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2009
Acceso en línea:Registro en Scopus
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Biblioteca Central Dr. Luis F. Leloir (FCEN) de Universidad de Buenos Aires
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100 1 |a Servidio, S. 
245 1 0 |a Magnetic reconnection in two-dimensional magnetohydrodynamic turbulence 
260 |c 2009 
270 1 0 |m Servidio, S.; Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, United States 
506 |2 openaire  |e Política editorial 
504 |a Sweet, P.A., (1958) Electromagnetic Phenomena in Cosmical Physics, , Cambridge University Press, New York 
504 |a Parker, E.N., (1957) J. Geophys. Res., 62, p. 509. , JGREA2 0148-0227 10.1029/JZ062i004p00509 
504 |a Sonnerup, B.U.O., (1984) Solar Terrestrial Physics-Present and Future, , edited by D.M. Butler and K. Papadopoulos, NASA Reference Publication 1120 (NASA, Washington, DC 
504 |a Schindler, K., (1988) J. Geophys. Res., 93, p. 5547. , JGREA2 0148-0227 10.1029/JA093iA06p05547 
504 |a Vasyliunas, V.M., (1975) Rev. Geophys. Space Phys., 13, p. 303. , RGPSBL 0034-6853 10.1029/RG013i001p00303 
504 |a Parker, E.N., (1979) Cosmical Magnetic Fields, , Oxford Univ. Press, New York 
504 |a Taylor, J.B., (1986) Rev. Mod. Phys., 58, p. 741. , RMPHAT 0034-6861 10.1103/RevModPhys.58.741 
504 |a Sato, T., (1978) Phys. Rev. Lett., 41, p. 1548. , PRLTAO 0031-9007 10.1103/PhysRevLett.41.1548 
504 |a Birn, J., (2001) J. Geophys. Res., 106, p. 3715. , JGREA2 0148-0227 10.1029/1999JA900449 
504 |a Matthaeus, W.H., Montgomery, D., (1980) Ann. N.Y. Acad. Sci., 357, p. 203. , ANYAA9 0077-8923 10.1111/j.1749-6632.1980.tb29687.x 
504 |a Matthaeus, W.H., Lamkin, S.L., (1986) Phys. Fluids, 29, p. 2513. , PFLDAS 0031-9171 10.1063/1.866004 
504 |a Strauss, H.R., (1988) Astrophys. J., 326, p. 412. , ASJOAB 0004-637X 10.1086/166104 
504 |a Carbone, V., (1990) Phys. Fluids A, 2, p. 1487. , PFADEB 0899-8213 10.1063/1.857598 
504 |a Malara, F., (1992) Phys. Fluids B, 4, p. 3070. , PFBPEI 0899-8221 10.1063/1.860477 
504 |a Lapenta, G., (2008) Phys. Rev. Lett., 100, p. 235001. , PRLTAO 0031-9007 10.1103/PhysRevLett.100.235001 
504 |a Biskamp, D., (1986) Phys. Fluids, 29, p. 1520. , PFLDAS 0031-9171 10.1063/1.865670 
504 |a Biskamp, D., (2000) Magnetic Reconnection in Plasmas, , Cambridge Univ. Press, Cambridge 
504 |a Ghosh, S., (1993) Comput. Phys. Commun., 74, p. 18. , CPHCBZ 0010-4655 10.1016/0010-4655(93)90103-J 
504 |a Rana, S., (2004) Surface Topological Data Structures, , John Wiley and Sons, Chichester, England 
504 |a Kraichnan, R.H., Panda, R., (1988) Phys. Fluids, 31, p. 2395. , PFLDAS 0031-9171 10.1063/1.866591 
504 |a Arzner, K., Vlahos, L., (2004) Astrophys. J., 605, p. 69. , ASJOAB 0004-637X 10.1086/392506 
504 |a Craig, J.D., Watson, P.G., (1999) Astrophys. J., 516, p. 924. , ASJOAB 0004-637X 10.1086/307135 
504 |a Dorelli, J.C., Birn, J., (2003) J. Geophys. Res., 108, p. 1183. , JGREA2 0148-0227 10.1029/2002JA009659 
504 |a Borovsky, J.E., Hesse, M., (2007) Phys. Plasmas, 14, p. 102309. , PHPAEN 1070-664X 10.1063/1.2772619 
504 |a Cassak, P.A., Shay, M.A., (2007) Phys. Plasmas, 14, p. 102114. , PHPAEN 1070-664X 10.1063/1.2795630 
504 |a Orszag, S.A., (1977) Fluid Dynamics, p. 235. , edited by R. Ballian and J.-L. Puebe (Gordon & Breach, N.Y 
504 |a Retinò, A., (2007) Nature Phys., 3, p. 235. , NPAHAX 1745-2481 10.1038/nphys574 
504 |a Gosling, J., Szabo, A., (2008) J. Geophys. Res., 113, p. 10103. , JGREA2 0148-0227 10.1029/2008JA013473 
520 3 |a Systematic analysis of numerical simulations of two-dimensional magnetohydrodynamic turbulence reveals the presence of a large number of X-type neutral points where magnetic reconnection occurs. We examine the statistical properties of this ensemble of reconnection events that are spontaneously generated by turbulence. The associated reconnection rates are distributed over a wide range of values and scales with the geometry of the diffusion region. Locally, these events can be described through a variant of the Sweet-Parker model, in which the parameters are externally controlled by turbulence. This new perspective on reconnection is relevant in space and astrophysical contexts, where plasma is generally in a fully turbulent regime. © 2009 The American Physical Society.  |l eng 
593 |a Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, United States 
593 |a Department of Physics, West Virginia University, Morgantown, WV 26506, United States 
593 |a Departmento de Física, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, 1428, Buenos Aires, Argentina 
690 1 0 |a ASTROPHYSICS 
690 1 0 |a FLUID DYNAMICS 
690 1 0 |a GEOPHYSICS 
690 1 0 |a MAGNETOHYDRODYNAMICS 
690 1 0 |a TWO DIMENSIONAL 
690 1 0 |a DIFFUSION REGIONS 
690 1 0 |a MAGNETIC RECONNECTIONS 
690 1 0 |a MAGNETOHYDRODYNAMIC TURBULENCES 
690 1 0 |a NUMERICAL SIMULATIONS 
690 1 0 |a RECONNECTION RATES 
690 1 0 |a STATISTICAL PROPERTIES 
690 1 0 |a SWEET-PARKER MODELS 
690 1 0 |a SYSTEMATIC ANALYSIS 
690 1 0 |a TURBULENT REGIMES 
690 1 0 |a X-TYPE NEUTRAL POINTS 
690 1 0 |a TURBULENCE 
700 1 |a Matthaeus, W.H. 
700 1 |a Shay, M.A. 
700 1 |a Cassak, P.A. 
700 1 |a Dmitruk, P. 
773 0 |d 2009  |g v. 102  |k n. 11  |p Phys Rev Lett  |x 00319007  |w (AR-BaUEN)CENRE-386  |t Physical Review Letters 
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856 4 0 |u https://doi.org/10.1103/PhysRevLett.102.115003  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_00319007_v102_n11_p_Servidio  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00319007_v102_n11_p_Servidio  |y Registro en la Biblioteca Digital 
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