Image Details

Choose export citation format:

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 2.

Dependence of the reconnection rate Vrec on the Lundquist number S for simulations without forcing at early times, and for different values of plasma−β. The dashed black line represents the Sweet–Parker scaling of Vrec ∝ S−1/2. Some circles and squares are overlapped. This is the case for intermediate values of β, between 2 and 18, for both S = 103 and 104.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse