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A New Approach of Linear Theory of Tearing Instability in Uniform Resistivity

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arxiv 2209.00149 v1 pith:FGFHGZ7P submitted 2022-08-31 physics.plasm-ph astro-ph.SR

classification physics.plasm-phastro-ph.SR
keywords instabilityresistivitytheoryuniformlinearoutertearingacceptable
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The linear perturbation equation of the tearing instability derived in LSC theory (Loureiro, Schekochihin, and Cowley, PoP2007) is numerically examined as an initial value problem, where the inner and outer regions are seamlessly solved under uniform resistivity. Hence, all regions are solved as the resistive MHD (magnetohydrodynamics). To comprehensively study physically acceptable perturbation solutions, the behaviors of the local maximum points required for physically acceptable solutions and zero-crossing points, at which \phi=0 and \psi=0, are examined. Eventually, the uniform resistivity assumed in the outer region is shown to play an important role in improving some conclusions derived from the theory. In conclusion, the upper limit \lambda_{up} of the growth rate obtained in the improved (modified) LSC theory is shown to be regulated by the Alfven speed measured in the outer region. It is also shown to be partially consistent with the growth rate in the linear developing stage of the impulsive tearing instability observed in the compressible MHD simulation of the plasmoid instability (PI) based on uniform resistivity.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dynamics and Energetics of Resistive, Thermally Conductive, and Radiative Plasma in Coronal Current Sheets due to Asymmetric External Perturbation

    astro-ph.SR 2024-12 conditional novelty 5.0 of 10

    In 2.5D MHD simulations, thermal conduction hastens current-sheet fragmentation and speeds reconnection, while radiative cooling delays fragmentation, altering plasmoid speeds and energy release.

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