3D-Numerical Simulations of Magnetic Field Evolution in the Turbulent Interstellar Gas

نویسندگان
چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

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...

متن کامل

Numerical Study of turbulent free convection of liquid metal with constant and variable properties in the presence of magnetic field

In this research, turbulent MHD convection of liquid metal with constant and variable properties is investigated numerically. The finite volume method is applied to model the fluid flow and natural convection heat transfer in a square cavity. The fluid flow and heat transfer were simulated and compared for two cases constant and variable properties. It is observed that for the case variable pro...

متن کامل

Numerical Control of 3D Turbulent Premixed Flame Simulations

One of the well-known properties of turbulent, premixed flames is that their speed of propagtion is correlated to the intensity of the turbulence they encounter. A simple consequence is that these types of flames are inherently unstable. Given a source of turbulence, if the flame is propagating faster than the mean flow, it will drift upstream and encounter increased turbulent intensities that ...

متن کامل

The Role of Helicity in Magnetic Reconnection: 3D Numerical Simulations

We demonstrate that conservation of global helicity plays only a minor role in determining the nature and consequences of magnetic reconnection in the solar atmosphere. First, we show that observations of the solar coronal magnetic field are in direct conflict with Taylor’s theory. Next, we present results from three-dimensional MHD simulations of the shearing of bipolar and multi-polar coronal...

متن کامل

Direct Numerical Simulations of Magnetic Field Effects on Turbulent Duct Flows

Magnetic fields are crucial in controlling flow in various physical processes of significance. Magnetic fields are frequently used to pump, stir and stabilize liquid metal flows non-intrusively. One of these processes, which has significant application of a magnetic field, is continuous casting of steel, where different magnetic field configurations are used to control the turbulent steel flow ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Symposium - International Astronomical Union

سال: 1993

ISSN: 0074-1809

DOI: 10.1017/s0074180900174510