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arXiv · 1101.0370

Fluid and Magnetofluid Modeling of Relativistic Magnetic Reconnection

Seiji Zenitani·Michael Hesse·Alex Klimas
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Abstract

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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Seiji Zenitani, Michael Hesse, Alex Klimas. 2011-10-13. Fluid and Magnetofluid Modeling of Relativistic Magnetic Reconnection. https://doi.org/10.1063/1.3625599

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