Nordita Astrophysics Seminars

CANCELED because of ILLNESS: A mean field dynamo from negative eddy diffusivity

by Dr Ebru Devlen (NORDITA)

Europe/Stockholm
122:026

122:026

Description
Using direct numerical simulations, we verify that "flow IV" of Roberts (1972) exhibits dynamo action dominated by horizontally averaged large-scale magnetic field. With the test-field method we compute the turbulent magnetic diffusivity and find that it is negative and overcomes the molecular diffusivity, thus explaining quantitatively the large-scale dynamo for magnetic Reynolds numbers above ~8. As expected for a dynamo of this type, but contrary to alpha-effect dynamos, the two horizontal field components grow independently of each other and have arbitrary amplitude ratios and phase differences. Small length scales of the mean magnetic field are shown to be stabilized by the turbulent magnetic diffusivity becoming positive at wavenumbers larger than twice the characteristic wavenumber of the flow. For magnetic Reynolds numbers below ~0.5 the turbulent magnetic diffusivity is confirmed to be positive, as expected for all incompressible flows. Earlier claims of a dynamo driven by a modified Taylor-Green flow through negative eddy diffusivity could not be confirmed.

arxiv:1212.2626