It is shown that ambipolar diffusion as a useful model for nonlinearity lea
ds to similar behaviour of large scale turbulent dynamos as full MHD. This
is demonstrated using both direct simulations in a periodic box and a closu
re model for the magnetic correlation functions applicable to infinite spac
e. Large scale fields develop via a nonlocal inverse cascade as described b
y 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 inc
reases with magnetic Reynolds number.