Topological Methods for the Analysis of Solar Magnetic Fields
The solar coronal magnetic field is anchored to a complex distribution of photospheric flux consisting of sunspots and magnetic elements. Coronal activity such as flares, eruptions and general heating is often attributed to the manner in which the coronal field responds to photospheric motions. A nu...
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| Format: | Article |
| Language: | English |
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SpringerOpen
2005-11-01
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| Series: | Living Reviews in Solar Physics |
| Online Access: | http://www.livingreviews.org/lrsp-2005-7 |