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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

Jack Carlyle ,
David Williams ,
Lidia van Driel-Gesztelyi  and
Davina Innes
Jack Carlyle
Affiliation:
UCL-Mullard Space Science Laboratory, UK email: j.carlyle@ucl.ac.uk Max Planck Institute for Solar System Research, Germany
David Williams
Affiliation:
UCL-Mullard Space Science Laboratory, UK email: j.carlyle@ucl.ac.uk
Lidia van Driel-Gesztelyi
Affiliation:
UCL-Mullard Space Science Laboratory, UK email: j.carlyle@ucl.ac.uk Observatoire de Paris, LESIA, UMR 8109 (CNRS), France Konkoly Observatory, Budapest, Hungary
Davina Innes
Affiliation:
Max Planck Institute for Solar System Research, Germany
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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
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Williams, D. R., Baker, D., & van Driel-Gesztelyi, L., 2013, ApJ, 764, 165Google Scholar