Titlebook: Magnetic Fields and Star Formation; Theory Versus Observ A. I. Gómez Castro,M. Heyer,R. E. Pudritz Book 2004 Springer Science+Business Medi

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Scaling Relations of Supersonic Turbulence in Molecular Cloudsis highly intermittent; we describe its statistical properties by obtaining scaling of velocity-difference structure functions. This scaling was analytically predicted in Boldyrev (2002), confirmed in numerical simulations by Boldyrev et al. (2002), and discovered in observations by Padoan et al. (2003).

ZEST

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Structure of Molecular Cloudsnnection with the diffuse medium, their multi-fractal characteristics and the diversity of their small-scale structure, where cold and dense gas may coexist with dilute and warm gas. Stuctures of essentially pure velocity origin are uncovered and seen as a possible signature of the intermittency of turbulence dissipation.

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Monocle

High-Resolution Simulations of Nonhelical MHD Turbulencere function exponent that is found to be .. = 0.70, suggesting a .. spectrum. The third-order structure function scaling exponent is very close to unity,—in agreement with Goldreich—Sridhar theory..Adding an imposed field tends to suppress the small-scale magnetic field. We find that at large scales