Abstract
Solar flare energy release mechanisms often neglect the role played by viscous effects. Here we perform incompressible planar reconnection simulations, driven by the Orszag–Tang vortex, for both classical and Braginskii forms of the viscosity. We show that strongly driven “saturated” flux pile-up current layers, which lead to weak reconnection rates at small resistivities, are accompanied by invariant global viscous losses. These results support the notion that viscous dissipation in flaring plasmas can account for a significant fraction of the flare energy release.
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Armstrong, C.K., Craig, I.J.D. Visco-Resistive Dissipation in Strongly Driven Transient Reconnection. Sol Phys 289, 869–877 (2014). https://doi.org/10.1007/s11207-013-0363-z
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DOI: https://doi.org/10.1007/s11207-013-0363-z