Review Article

Modeling Kelvin–Helmholtz Instability in Soft X-Ray Solar Jets

Figure 10

(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 , 4.15, 4.1, 4.075, and 4.062. (b) The normalized growth rates for the same values of
(a)
(b)