Isolated supernova remnants drive incompressible turbulence through baroclinic vorticity at corrugated contact discontinuities, producing a k^{3/4} spectrum that can imprint on kiloparsec scales via inverse cascade.
I plotP B(k) in the bottom panel of Figure 4, averaged and normalized in the same way as the previous spectra
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Supernovae drive large-scale, incompressible turbulence through small-scale instabilities
Isolated supernova remnants drive incompressible turbulence through baroclinic vorticity at corrugated contact discontinuities, producing a k^{3/4} spectrum that can imprint on kiloparsec scales via inverse cascade.