Review Article
Modeling Kelvin–Helmholtz Instability in Soft X-Ray Solar Jets
Figure 11
(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 , 4.1, 4.109, and 4.125. (b) The normalized growth rates for the same values of
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