English

Observation of axisymmetric standard magnetorotational instability in the laboratory

Instrumentation and Methods for Astrophysics 2022-09-20 v1 High Energy Astrophysical Phenomena Fluid Dynamics

Abstract

We report the first direct evidence for the axisymmetric standard magnetorotational instability (SMRI) from a combined experimental and numerical study of a magnetized liquid-metal shear flow in a Taylor-Couette cell with independently rotating and electrically conducting end caps. When a uniform vertical magnetic field BiB_i is applied along the rotation axis, the measured radial magnetic field BrB_r on the inner cylinder increases linearly with a small magnetic Reynolds number RmRm due to the magnetization of the residue Ekman circulation. Onset of the axisymmetric SMRI is identified from the nonlinear increase of BrB_r beyond a critical RmRm in both experiments and nonlinear numerical simulations. The axisymmetric SMRI exists only at sufficiently large RmRm and intermediate BiB_i, a feature consistent with theoretical predictions. Our simulations further show that the axisymmetric SMRI causes the velocity and magnetic fields to contribute an outward flux of axial angular momentum in the bulk region, just as it should in accretion disks.

Keywords

Cite

@article{arxiv.2209.08457,
  title  = {Observation of axisymmetric standard magnetorotational instability in the laboratory},
  author = {Yin Wang and Erik P. Gilson and Fatima Ebrahimi and Jeremy Goodman and Hantao Ji},
  journal= {arXiv preprint arXiv:2209.08457},
  year   = {2022}
}

Comments

10 pages; 11 figures