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Density evolution of in-falling prominence material from the 7th June 2011 CME
Published online by Cambridge University Press: 06 January 2014
Abstract
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This work investigates the density of in-falling prominence material following the 7th June 2011 eruption. Both the evolution and the distribution of the density is analysed in five discreet “blobs” of material. The density appears to be remarkably uniform, both spatially within the blobs, and temporally over the course of the descent of each, although a slight concentration of material towards the leading edge is noted in some cases. Online material is available at bit.ly/jackblob
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 401 - 402
- Copyright
- Copyright © International Astronomical Union 2013
References
Carlyle, J., Williams, D., van Driel-Gesztelyi, L., Innes, D., Hillier, A., Matthews, S., 2013, ApJ, submittedGoogle Scholar
Innes, D. E., Cameron, R. H., Fletcher, L., Inhester, B., & Solanki, S. K., 2012, A&A 540, L10Google Scholar
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