In fluid simulations of interchange turbulence, modes change from interchange to tearing parity via cubic nonlinearities; the small islands formed then coalesce into large-scale turbulence-driven islands, catalyzed by zonal flow and inhibited by zonal current.
Three-dimensional magnetic reconnection and its application to solar flares
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Zonal fields as catalysts and inhibitors of turbulence-driven magnetic islands
In fluid simulations of interchange turbulence, modes change from interchange to tearing parity via cubic nonlinearities; the small islands formed then coalesce into large-scale turbulence-driven islands, catalyzed by zonal flow and inhibited by zonal current.