“…For weak stochasticity, even small perpendicular current associated with the plasma inertia, can produce significant modulation in λ along the magnetic field line due to the Pfirsch-Schlüter effect [8]. As the MHD instabilities die down and the flux surfaces reheal, like those in laboratory confinement experiments with reversed field pinch [9], spheromaks [10], spherical tokamak [11,12,13], and tokamak disruptions [14], or in the solar corona [15] and radio lobes [16], one can end up with a force-free plasma with λ(ψ) a function of the flux surface label ψ, also know as a nonlinear force-free magnetic field [17,18,19,20], which despite the deviation from the constant λ Taylor state, retains the key feature of magnetic self-organization via a resonant coupling between the helicity injection source and global magnetic configuration [21,22,23]. Further evolution of such a nonlinear force-free plasma, for example, a post-thermal-quench tokamak plasma undergoing a cold vertical displacement event (VDE), is governed by the slow transport process, namely the resistive decay of the plasma current.…”