Solar Surface Magneto-Convection
We review the properties of solar magneto-convection in the top half of the convection zones scale heights (from 20 Mm below the visible surface to the surface, and then through the photosphere to the temperature minimum). Convection is a highly non-linear and non-local process, so it is best studie...
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| Format: | Article |
| Language: | English |
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SpringerOpen
2012-07-01
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| Series: | Living Reviews in Solar Physics |
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| Online Access: | http://www.livingreviews.org/lrsp-2012-4 |