Magnetized decaying turbulence in the weakly compressible Taylor-Green vortex

Magnetohydrodynamic turbulence affects both terrestrial and astrophysical plasmas. The properties of magnetized must be better understood to more accurately characterize these systems. This work presents ideal MHD simulations the compressible Taylor-Green vortex under a range initial sub-sonic Mach numbers magnetic field strengths. We find that regardless strength, energy becomes dominant over kinetic on all scales after at most several dynamical times. spectral indices spectra become shallower than $k^{-5/3}$ time generally fluctuate. Using shell-to-shell transfer analysis framework, we fields facilitate significant amount flux cascade is suppressed. Moreover, observe nonlocal from large scale intermediate small via tension. conclude even in intermittently or singularly driven weakly systems, effects cannot neglected.