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Investigating Turbulence Effects on Magnetic Reconnection Rates through 3D Resistive Magnetohydrodynamic Simulations

  • Authors: Giovani H. Vicentin, Grzegorz Kowal, Elisabete M. de Gouveia Dal Pino, Alex Lazarian

Giovani H. Vicentin et al 2025 The Astrophysical Journal 987 .

  • Provider: AAS Journals

Caption: Figure 15.

Left: average thickness 〈δ〉 of the current layer extracted from the FWHM of the current density magnitude profile for the turbulent (solid) and tearing instability (dashed) cases. Right: an estimate of the reconnection rate for these two simulations, as measured from the ratio 〈δ〉/〈L〉. The models are the same as those in Figure 14.

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