3D-Numerical Simulations of Magnetic Field Evolution in the Turbulent Interstellar Gas
نویسندگان
چکیده
منابع مشابه
Numerical simulations of compressively driven interstellar turbulence: I. Isothermal gas
Context. Supersonic turbulence is ubiquitous in the interstellar medium and plays an important role in contemporary star formation. Aims. To perform a high-resolution numerical simulation of supersonic isothermal turbulence driven by compressive large-scale forcing and to analyse various statistical properties. Methods. The compressible Euler equations with an external stochastic force field do...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1993
ISSN: 0074-1809
DOI: 10.1017/s0074180900174510