tokens: We thank the anonymous referee for a very careful reading of our manuscript that has led to a marked improvement in the clarity of this paper. M.B.K. is grateful to the University of Sheffield and the Hungarian Academy of Sciences for the support received. M.B.K. also acknowledges the open research program of CAS Key Laboratory of Solar Activity, National Astronomical Observatories, No. KLSA201610. P.C. thanks the University of Sheffield for hospitality and support for a visit during which this work was initiated and the CAS PIFI project 2017VMC0002 and National Astronomical Observatories, Beijing, for support. The simulation was carried out on NASA’s Pleiades supercomputer under GID s1061. P.C. also acknowledges computing time awarded on the PARAM Yuva-II supercomputer at C-DAC, India, under the grant name Hydromagnetic-Turbulence-PR. We have used the 3D visualization software Paraview for volume rendering and field line plotting. R.E. is grateful to the Science and Technology Facilities Council (STFC; grant Nos. ST/L006316/1 and ST/M000826/1) UK and the Royal Society for their support. The authors also express their gratitude to Christopher J. Nelson and Michael S. Ruderman (both at University of Sheffield, UK) for a number of useful discussions and improving the manuscript.
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