Inverse energy transfer in decaying MHD turbulence: A shell-to-shell analysis
This paper utilizes shell-to-shell transfer functions to demonstrate that inverse energy transfer in decaying magnetohydrodynamic turbulence arises from non-local, self-similar growth driven by the merging of local magnetic islands with equal-signed helicity, a mechanism consistent with Hosking integral conservation that operates independently of net-helicity and within individual helical sectors.