• Title of article

    Turbulent magnetic Prandtl number and magnetic diffusivity quenching from simulations

  • Author/Authors

    Brandenburg، A. نويسنده , , Rudiger، G. نويسنده , , Yousef، T. A. نويسنده ,

  • Issue Information
    روزنامه با شماره پیاپی سال 2003
  • Pages
    -320
  • From page
    321
  • To page
    0
  • Abstract
    Forced turbulence simulations are used to determine the turbulent kinematic viscosity, v(t), from the decay rate of a large scale velocity field. Likewise, the turbulent magnetic diffusivity, ..., is determined from the decay of a large scale magnetic field. In the kinematic regime, when the field is weak, the turbulent magnetic Prandtl number, ..., is about unity. When the field is nonhelical, ...is quenched when magnetic and kinetic energies become comparable. For helical fields the quenching is stronger and can be described by a dynamical quenching formula.
  • Keywords
    turbulence , magnetohydrodynamics (MHD)
  • Journal title
    Astronomy and Astrophysics
  • Serial Year
    2003
  • Journal title
    Astronomy and Astrophysics
  • Record number

    77100