Figure 4 from Tearing Instability and Periodic Density Perturbations in the Slow Solar Wind

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Tearing Instability and Periodic Density Perturbations in the Slow Solar Wind

Authors: Victor Réville, Marco Velli, Alexis P. Rouillard, Benoit Lavraud, Anna Tenerani, Chen Shi, and Antoine Strugarek

2020 The Astrophysical Journal Letters 895 L20.

Provider: AAS Journals

Caption: Figure 4.

Top panel: fastest growing mode k_m as a function of the Lundquist number S. The asymptotic regime k_m ∝ S^1/6 is shown by the black dashed line. The corresponding growth rate, normalized by t_A = L/v_A, is shown in the bottom panel.

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