Construct · 1 fields · 1 citations

magnetorotational instability: a standalone construct

One name. One construct. A landmark on the map.

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magnetorotationalinstability1 CONSTRUCTMagnetorotationalBALBUS · ASTROPHYSICS

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Astrophysics

an instability of weakly magnetized, differentially rotating disks that drives turbulence and outward angular momentum transport in accretion disks.

In astrophysics, magnetorotational instability refers to an instability of weakly magnetized, differentially rotating disks that drives turbulence and outward angular momentum transport in accretion disks. This meaning comes from Balbus (1991) in The Astrophysical Journal.[1]

Unit
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Measured by

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Nearby constructs

accretion3 fields · 6 citationsjingle · one word, three constructsinstability3 fields · 3 citationsjingle · one word, three constructsmomentum7 fields · 14 citationsjingle · one name, six constructs

References

  1. Balbus, S. A., & Hawley, J. F. (1991). A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution. The Astrophysical Journal, 376, 214. https://doi.org/10.1086/170270

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