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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 14.

Comparison of the mean current density magnitude profile along the y-axis between the model with initial external perturbation where turbulence develops (solid) and the one without it, where tearing instability develops (dashed line). Both simulations have S = 105, β = 2.0, and Prm = 1.

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