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- W2017681925 abstract "The spontaneous fast reconnection model is applied to the plasmoid dynamics, and computer simulations are performed for a wide range of parameters. According to the fast reconnection development, the resulting strong (Alfvénic) plasma jet drives a large-scale plasmoid to swell and propagate. Once the plasmoid fully develops, the propagation speed Vp becomes almost constant. It is the J×B force, not the pressure-gradient force, that plays the dominant role on the plasmoid propagation. It is estimated that Vp∼0.8VA l0, where VA l0 is the Alfvén velocity measured in the magnetic field region ahead of the plasmoid. Along the backward-half plasmoid boundary a strong slow (almost switch-off) shock is formed, whereas along the forward-half boundary a rather weak slow shock stands. The plasma pressure is largely enhanced in the middle of the plasmoid, and the magnetic energy just outside the plasmoid is notably enhanced in the forward half because of the generator effect and is then distinctly reduced in the backward half by the strong motor effect. For the uniform resistivity model, any distinct plasmoid cannot be set up. It is argued that the spontaneous fast reconnection mechanism should be most applicable to catastrophic events observed in space plasmas." @default.
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- W2017681925 date "1995-09-01" @default.
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- W2017681925 title "Computer studies on plasmoid dynamics associated with the spontaneous fast reconnection mechanism" @default.
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- W2017681925 doi "https://doi.org/10.1063/1.871165" @default.
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