Magnetorotational instability in Taylor-Couette flows between cylinders with finite electrical conductivity
Abstract
The nonaxisymmetric azimuthal magnetorotational instability is studied for hydromagnetic Taylor-Couette flows between cylinders of finite electrical conductivity. We find that the magnetic Prandtl number ? determines whether perfectly conducting or insulating boundary conditions lead to lower Hartmann numbers for the onset of instability. Regardless of the imposed rotation profile, for small ? the solutions for perfectly conducting cylinders become unstable for weaker magnetic fields than the solutions for insulating cylinders. The critical Hartmann and Reynolds numbers form monotonic functions of the ratio ? of the electrical conductivities of the cylinders and the fluid, such that ? provides a very good approximation to perfectly conducting cylinders, and ? a very good approximation to insulating cylinders. These results are of particular relevance for the super-rotating case where the outer cylinder rotates faster than the inner one; in this case the critical onset values are substantially different for perfectly conducting versus insulating boundary conditions. An experimental realisation of the super-rotating instability, with liquid sodium as the fluid and cylinders made of copper, would need an electric current of at least 33.5 kA running along the central axis.
- Publication:
-
Geophysical and Astrophysical Fluid Dynamics
- Pub Date:
- July 2018
- DOI:
- arXiv:
- arXiv:1804.01501
- Bibcode:
- 2018GApFD.112..301R
- Keywords:
-
- Astrophysical fluid dynamics;
- Taylor-Couette flow;
- magnetic boundary conditions;
- Physics - Fluid Dynamics
- E-Print:
- 18 pages with 15 figures