Results 201 to 210 of about 4,329,863 (238)
Some of the next articles are maybe not open access.
Direct observation of turbulent magnetic reconnection in the solar wind
Nature Astronomy, 2022Rongsheng Wang +5 more
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Reconnection rates in driven magnetic reconnection
Physics of Plasmas, 2007Using resistive magnetohydrodynamic simulations, we investigate the influence of various parameters on the reconnection rate in two scenarios of magnetic reconnection. The first scenario consists of the “Newton Challenge” problem [Birn et al., Geophys. Res. Lett. 32, L06105 (2005)].
J. Birn, M. Hesse
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Nonlinear collisionless magnetic reconnection
Physical Review Letters, 1993Collisionless magnetic reconnection in regimes where the mode structure is characterized by global convection cells is found to exhibit a quasiexplosive time behavior in the early nonlinear stage where the fluid displacement is smaller than the equilibrium scale length. This process is accompanied by the formation of a current density sublayer narrower
M. OTTAVIANI, PORCELLI, Francesco
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Physics Reports, 1994
This lecture deals with the concept of magnetic field lines and with the conservation of magnetic flux. In high temperature fusion devices like tokamaks flux conservation can be violated and reconnection can occur at closed magnetic field lines. Reconnection processes lead to changes in the global topology of the magnetic field.
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This lecture deals with the concept of magnetic field lines and with the conservation of magnetic flux. In high temperature fusion devices like tokamaks flux conservation can be violated and reconnection can occur at closed magnetic field lines. Reconnection processes lead to changes in the global topology of the magnetic field.
openaire +3 more sources
Hall Magnetic Reconnection Rate
Physical Review Letters, 2004Two-dimensional Hall magnetohydrodynamic simulations are used to determine the magnetic reconnection rate in the Hall limit. The simulations are run until a steady state is achieved for four initial current sheet thicknesses: L=1,5,10, and 20c/omega(pi), where c/omega(pi) is the ion inertial length.
J D, Huba, L I, Rudakov
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Impacts of Ionospheric Ions on Magnetic Reconnection and Earth's Magnetosphere Dynamics
Reviews of Geophysics, 2021Benoit Lavraud +2 more
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Energy Budgets From Collisionless Magnetic Reconnection Site to Reconnection Front
Journal of Geophysical Research: Space Physics, 2021San Lu, Quanming Lu, Yukang Shu
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