Simulations show the Strouhal number of supernova-driven interstellar turbulence is approximately 0.25, with St reaching 1 only at about 12-13% of the outer scale near the cooling radius of remnants.
We find projected median val- ues St≈0.2–0.25 in both galaxy models, implying that the measured correlation time is substantially shorter than the outer-scale turnover time
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What is the Strouhal number of turbulence driven by supernovae?
Simulations show the Strouhal number of supernova-driven interstellar turbulence is approximately 0.25, with St reaching 1 only at about 12-13% of the outer scale near the cooling radius of remnants.