Fluid and Magnetofluid Modeling of Relativistic Magnetic Reconnection
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🌌 astro-ph.HE
keywords
relativisticmagneticreconnectionevolutionmagnetofluidmodelssimulationstwo-fluid
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The fluid-scale evolution of relativistic magnetic reconnection is investigated by using two-fluid and magnetofluid simulation models. Relativistic two-fluid simulations demonstrate the meso-scale evolution beyond the kinetic scales, and exhibit quasi-steady Petschek-type reconnection. Resistive relativistic MHD simulations further show new shock structures in and around the downstream magnetic island (plasmoid). General discussions on these models are presented.
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