A statistical analysis of 167 Galactic molecular clouds finds 60% of velocity structure functions are power-laws whose relative exponents match the Boldyrev 2002 intermittent turbulence model.
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Examining Turbulence in Galactic Molecular Clouds -- I: A Statistical Analysis of Velocity Structures
A statistical analysis of 167 Galactic molecular clouds finds 60% of velocity structure functions are power-laws whose relative exponents match the Boldyrev 2002 intermittent turbulence model.