Using $10,\!080^3$ grid simulations, we analyze scale-dependent alignment in driven, compressible, no net-flux magnetohydrodynamic turbulence. The plasma self-organizes into localized, strongly aligned regions. Alignment spans all primitive variables and their curls. Contrary to incompressible theory, velocity-magnetic alignment scales as $\theta(\lambda) \sim \lambda^{ 1/8}$, where $\lambda$ is the scale, suggesting a distinct three-dimensional eddy anisotropy and a much higher critical transition scale toward a reconnection-mediated cascade.
Categories: physics.plasm-ph astro-ph.GA nlin.CD physics.flu-dyn