Despite the importance of the magnetorotational instability (MRI) as a fundamental mechanism for angular momentum transport in magnetized accretion disks, it has yet to be demonstrated in the laboratory. A liquid sodium αω dynamo experiment at the New ...
CITATION STYLE
Noguchi, K., Pariev, V. I., Colgate, S. A., Beckley, H. F., & Nordhaus, J. (2002). Magnetorotational Instability in Liquid Metal Couette Flow. The Astrophysical Journal, 575(2), 1151–1162. https://doi.org/10.1086/341502
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