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Absolute versus convective helical magnetorotational instabilities in Taylor-Couette flows

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Figure

Figure 1. Stability boundaries in the (indicated. In each panel the black curves are the convective instability obtained forBHa, Re) plane, for Ωo/Ωi = 0.26 and 0.27 asc
Figure 2. Hovm¨oller plots showing the space-time evolution of ψ(z, t) at mid-gap,r = 1.5
Figure 4. Time-averaged axial power spectra of the solutions in fig. 2. The black linecorresponding to dissipative lengthscales much shorter than the typical Taylor vortex400
Figure 5. Linear eigenvalue calculations at Ωo/Ωi = 0.26, δ = 0.1, Ha = 120 andRe = 2500

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