Investigation of recovery of stellar magnetic field geometries from simulated spectropolarimetric data
Powerful remote sensing techniques can covert time variability of polarization profiles of stellar spectral lines into vector magnetic fields maps of stellar surfaces. These techniques are widely applied to interpret observations but have been tested using only simplistic tests. It would be of inter...
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| Format: | Others |
| Language: | English |
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Uppsala universitet, Institutionen för fysik och astronomi
2017
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| Online Access: | http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-316290 |