Influence of the Hall effect and electron inertia in collisionless magnetic reconnection

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We study the role of the Hall current and electron inertia in collisionless magnetic reconnection within the framework of full two-fluid MHD. At spatial scales smaller than the electron inertial length, a topological change of magnetic field lines exclusively due to the electron inertia becomes poss...

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Autor principal: Andrés, Nahuel
Otros Autores: Dmitruk, P., Gómez, D.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: American Institute of Physics Inc. 2016
Acceso en línea:Registro en Scopus
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100 1 |a Andrés, Nahuel 
245 1 0 |a Influence of the Hall effect and electron inertia in collisionless magnetic reconnection 
260 |b American Institute of Physics Inc.  |c 2016 
270 1 0 |m Andrés, N.; Instituto de Astronomía y Física Del Espacio (CONICET-UBA), Ciudad Autónoma de Buenos AiresArgentina; email: nandres@iafe.uba.ar 
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506 |2 openaire  |e Política editorial 
520 3 |a We study the role of the Hall current and electron inertia in collisionless magnetic reconnection within the framework of full two-fluid MHD. At spatial scales smaller than the electron inertial length, a topological change of magnetic field lines exclusively due to the electron inertia becomes possible. Assuming stationary conditions, we derive a theoretical scaling for the reconnection rate, which is simply proportional to the Hall parameter. Using a pseudo-spectral code with no dissipative effects, our numerical results confirm this theoretical scaling. In particular, for a sequence of different Hall parameter values, our numerical results show that the width of the current sheet is independent of the Hall parameter, while its thickness is of the order of the electron inertial range, thus confirming that the stationary reconnection rate is proportional to the Hall parameter. © 2016 AIP Publishing LLC.  |l eng 
593 |a Instituto de Astronomía y Física Del Espacio (CONICET-UBA), Ciudad Autónoma de Buenos Aires, Argentina 
593 |a Departamento de Física (FCEN, UBA) Nahuel Andrés, Argentina 
690 1 0 |a ELECTRONS 
690 1 0 |a MAGNETISM 
690 1 0 |a PLASMA SIMULATION 
690 1 0 |a DISSIPATIVE EFFECTS 
690 1 0 |a ELECTRON INERTIA 
690 1 0 |a MAGNETIC FIELD LINE 
690 1 0 |a MAGNETIC RECONNECTIONS 
690 1 0 |a NUMERICAL RESULTS 
690 1 0 |a RECONNECTION RATE 
690 1 0 |a STATIONARY CONDITIONS 
690 1 0 |a TOPOLOGICAL CHANGES 
690 1 0 |a MAGNETOHYDRODYNAMICS 
700 1 |a Dmitruk, P. 
700 1 |a Gómez, D. 
773 0 |d American Institute of Physics Inc., 2016  |g v. 23  |k n. 2  |p Phys. Plasmas  |x 1070664X  |w (AR-BaUEN)CENRE-6479  |t Physics of Plasmas 
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