Magnetostrophic MRI in the earth's outer core
We show that a simple, modified version of the Magnetorotational Instability (MRI) can develop in the outer liquid core of the Earth, in the presence of a background shear. It requires either thermal wind, or a primary instability, such as convection, to drive a weak differential rotation within the...
| Päätekijät: | , , |
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| Aineistotyyppi: | Journal article |
| Kieli: | English |
| Julkaistu: |
2008
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