1) Simulations were conducted of the decay of various helical and non-helical magnetic knot configurations, including trefoil knots, IUCAA knots, and Borromean rings. 2) The decay was slower for configurations with higher magnetic helicity, as these knots were more strongly packed. This led to different decay slopes for different configurations. 3) Reconnection events transformed magnetic self-linking into twisting, approximately conserving magnetic helicity over time. Isolated helical structures that formed also inhibited energy decay.