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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 9.

Time evolution of the magnetic flux Φ_B, calculated across the plane x = 0, for different magnetic Prandtl numbers. The two dashed black lines correspond to a constant reconnection rate of V_rec/V_A = −∂_tΦ_B = 0.05.

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