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Flares and non-potentiality of AR 11158
Published online by Cambridge University Press: 18 July 2013
Abstract
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Five non-potential parameters are calculated to investigate the temporal and spatial variations of vector magnetic field in active region 11158. An area that had evident changes of the azimuth of the vector magnetic field was found. The sunspot rotation may lead to an increase of the non-potentiality. Rapid and prominent increases are found in the variations of unsigned helicity.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 573 - 574
- Copyright
- Copyright © International Astronomical Union 2013
References
Song, Q., Zhang, J., Yang, S., & Liu, Y.
2012, Research in Astronomy and Astrophysics, accepted, arXiv:1209.6192Google Scholar
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