Modification of Projected Velocity Power Spectra by Density Inhomogeneities in Compressible Supersonic Turbulence

Details Modification of Projected Velocity Power Spectra by Density Inhomogeneities in Compressible Supersonic Turbulence Modification of Projected Velocity Power Spectra by Density Inhomogeneities in Compressible Supersonic Turbulence

2003-11-19

arxiv.org/abs/astro-ph/0311461v1

Astrophys.J. 604 (2004) 196-212

Astronomy and Astrophysics

Astrophysics

28 pages total, 20 figures, accepted for publication in ApJ

Scientific paper

10.1086/381648

(Modified) The scaling of velocity fluctuation, dv, as a function of spatial scale L in molecular clouds can be measured from size-linewidth relations, principal component analysis, or line centroid variation. Differing values of the power law index of the scaling relation dv = L^(g3D) in 3D are given by these different methods: the first two give g3D=0.5, while line centroid analysis gives g3D=0. This discrepancy has previously not been fully appreciated, as the variation of projected velocity line centroid fluctuations (dv_{lc} = L^(g2D)) is indeed described, in 2D, by g2D=0.5. However, if projection smoothing is accounted for, this implies that g3D=0. We suggest that a resolution of this discrepancy can be achieved by accounting for the effect of density inhomogeneity on the observed g2D obtained from velocity line centroid analysis. Numerical simulations of compressible turbulence are used to show that the effect of density inhomogeneity statistically reverses the effect of projection smoothing in the case of driven turbulence so that velocity line centroid analysis does indeed predict that g2D=g3D=0.5. Using our numerical results we can restore consistency between line centroid analysis, principal component analysis and size-linewidth relations, and we derive g3D=0.5, corresponding to shock-dominated (Burgers) turbulence. We find that this consistency requires that molecular clouds are continually driven on large scales or are only recently formed.

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