Large scale dynamos with ambipolar diffusion nonlinearity

Jul, 2000
4 pages
Published in:
  • Astron.Astrophys. 361 (2000) L33
e-Print:

Citations per year

20002003200620092012012345
Abstract: (arXiv)
It is shown that ambipolar diffusion as a toy nonlinearity leads to very similar behaviour of large scale turbulent dynamos as full MHD. This is demonstrated using both direct simulations in a periodic box and a closure model for the magnetic correlation functions applicable to infinite space. Large scale fields develop via a nonlocal inverse cascade as described by the alpha-effect. However, because magnetic helicity can only change on a resistive timescale, the time it takes to organize the field into large scales increases with magnetic Reynolds number.