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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 21.

Time evolution of the magnetic flux (left) and the reconnection rate (right) for two different injection powers of the initial perturbation, of Pinj = 0.1 (blue) and 0.5 (red). The other parameters of the simulation are S = 105, β = 2.0, Prm = 1, and kinj = 128.

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