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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 11.

Power spectra of the vorticity field in the x−z plane (current sheet midplane) at different time steps of the simulation with S = 105, β = 2.0, and Prm = 50. The black dashed lines represents the 2D Kolmogorov turbulent power spectrum of ﹩{ \mathcal P }(k)\propto {k}^{-2/3}﹩.

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