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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 20.

Time evolution of the magnetic flux (left) and the reconnection rate (right) for two different initial conditions, one with constant density (black) and the other with constant guide field, which is used in all simulated models of this work (orange). The physical parameters of both simulations are S = 105, β = 2.0, Prm = 50, Pinj = 0.1, and kinj = 128.

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