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

Anticoagulants

收養(yǎng)

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

jagged

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.

舉止粗野的人

http://image.papertrans.cn/m/image/621226.jpg

GEM

FOLLY

ARCH

fatty-streak

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