Review Article
Modeling Kelvin–Helmholtz Instability in Soft X-Ray Solar Jets
Figure 9
(a) Dispersion curves of unstable () MHD mode propagating in a moving twisted flux tube of incompressible plasma (modeling jet #11) at the same parameters as in Figure 8 and for , (green curve), (purple curve), and 4.02. (b) The normalized growth rates for the same values of
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