By P. H. Diamond
Turbulence pervades the dynamics of either laboratory and astrophysi- cal plasmas. Turbulent shipping and its linked confinement degrada- tion are the most stumbling blocks to attaining ignition in magnetically limited plasma (i.e., for magnetic confinement fusion (MCF) research), whereas trans- port bifurcations and self-generated shear flows are the main capacity for controlling such waft wave turbulence.
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