The most sophisticated attempts to model the convection zone have yielded results in which the angular velocity increases outwards and the largest scales of convection take the form of 'banana cells' aligned with the rotation axis. However, not only does the sign of the angular velocity gradient pre
β¦ LIBER β¦
The statistical stability of convection dynamos
β Scribed by Willem V.R. Malkus
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 473 KB
- Volume
- 97
- Category
- Article
- ISSN
- 0167-2789
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## Abstract We summarize the current state of the long term discussion about the saturation mechanisms associated with rapid growth of smallβscale magnetic field, that operate in largeβscale galactic dynamos, and related problems with magnetic helicity conservation. Our general conclusion is that,