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Published by: Physics of Plasmas Published on: 04/2013
YEAR: 2013   DOI: 10.1063/1.4802985
Parker Data Used; magnetic reconnection; plasma magnetohydrodynamics; plasma simulation; plasma turbulence; 52.30.Cv; 52.35.Ra; 52.35.Vd; 52.65.-y; Magnetohydrodynamics; plasma turbulence; magnetic reconnection; plasma simulation
Published by: Physics of Plasmas Published on: 01/2013
YEAR: 2013   DOI: 10.1063/1.4789606
Parker Data Used; plasma fluctuations; plasma magnetohydrodynamics; plasma simulation; plasma transport processes; plasma turbulence; random processes; Solar corona; stochastic processes; 52.25.Fi; 05.40.Fb; 52.30.Cv; 52.35.Ra; 52.65.Kj; 52.25.Gj; Transport properties; Random walks and Levy flights; Magnetohydrodynamics; plasma turbulence; Magnetohydrodynamic and fluid equation; Fluctuation and chaos phenomena
Magnetic field reconnection is often invoked to explain electromagnetic energy conversion in planetary magnetospheres, stellar coronae, and other astrophysical objects. Because of the huge dynamic range of magnetic fields in these bodies, it is important to understand energy conversion as a function of magnetic field strength and related parameters. It is conjectured theoretically and shown experimentally that the energy conversion rate per unit area in reconnection scales as the cube of an appropriately weighted magnetic ...
Published by: Physics of Plasmas Published on: 10/2010
YEAR: 2010   DOI: 10.1063/1.3504224