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Lookup NU author(s): Professor Axel Brandenburg,
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It is shown that ambipolar diffusion as a useful model for nonlinearity leads to 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 ct-effect. However, magnetic helicity can only change on a resistive timescale, so the time it takes to organize the field into large scales increases with magnetic Reynolds number.
Author(s): Brandenburg A, Subramanian K
Publication type: Letter
Publication status: Published
Journal: Astronomy and Astrophysics