A new denoising method extends the Brunt technique to recover 3D turbulent density dispersions from noisy 2D column-density maps with <15% error for SNR≥1.
and Schmidt, Wolfram, year = 2009, month = feb
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A model based on Chandrasekhar's 1951 time-invariant quantity quantitatively explains the Mach-number dependence of the density power spectrum slope in isothermal supersonic turbulence and demonstrates that the slope cannot reliably determine the Mach number.
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From 2D to 3D: Recovering Turbulent Density Dispersions from Noisy Data
A new denoising method extends the Brunt technique to recover 3D turbulent density dispersions from noisy 2D column-density maps with <15% error for SNR≥1.
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The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence
A model based on Chandrasekhar's 1951 time-invariant quantity quantitatively explains the Mach-number dependence of the density power spectrum slope in isothermal supersonic turbulence and demonstrates that the slope cannot reliably determine the Mach number.