tokens: ACKNOWLEDGEMENTS I acknowledge computing time awarded at CDAC National Param supercomputing facility, India, under the grant ‘Hydromagnetic-Turbulence-PR’ and the use of ‘Nova’ cluster at IIA. I also thank the Science and Engineering Research Board (SERB) of the Department of Science Technology (DST), Government of India, for support through research grant ECR/2017/001535. It is a pleasure to thank Kandaswamy Subramanian for insightful discussions on decaying (M)HD turbulence and for his comments on the manuscript. I also thank the anonymous referee for a timely and and constructive report that helped to improve the quality of the paper. The software used in this work was in part developed by the DOE NNSA-ASC OASCR Flash Center at the University of Chicago.
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