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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 22.

Time evolution of the magnetic flux (left) and the reconnection rate (right) for two different resolutions, with grid size h = 1/1024 (black) and h = 1/2048 (orange). The initial parameters of both simulations are S = 105, β = 2.0, Prm = 50, Bz = 0.5 (constant), Pinj = 0.1, and kinj = 128.

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