“…The development of a helical core is related to the linear stability of (m, n) = (1, 1) internal-kink modes [19][20][21], so that the magnetic shear at the q = 1 surface suppresses the formation while the pressure gradient enhances it [16,21,22,[24][25][26]. The enhancement of the distortion, by increasing the triangularity [17], is consistent with the shape dependence of the linear stability of internal-kink modes [21,25]. A direct link between a helical equilibrium state and linear stabilities is demonstrated by nonlinear MHD simulations [23,24].…”