  The objective of this work is to understand how the characteristics of
relativistic MHD turbulence may differ from those of nonrelativistic MHD
turbulence. We accomplish this by studying the ideal invariants in the
relativistic case and comparing them to what we know of nonrelativistic
turbulence. Although much work has been done to understand the dynamics of
nonrelativistic systems (mostly for ideal incompressible fluids), there is
minimal literature explicitly describing the dynamics of relativistic MHD
turbulence using numerical simulations. Many researchers simply assume that
relativistic turbulence has the same invariants and obeys the same dynamics as
non-relativistic systems our results show that this assumption may be
incorrect.
