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Kappa-distributions and Temperature Structure of the Prominence-Corona Transition Region
Published online by Cambridge University Press: 06 January 2014
Abstract
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The influence of the electron κ - distributions on the differential emission measure (DEM) of the prominence-corona transition region (PCTR) derived from observed line intensities has been investigated. An important consequence of the κ - distribution is formation of the emission lines in much wider temperature ranges. The implications for the formation temperature of the observed SDO/AIA band emissions are shown.
Keywords
- 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. 408 - 409
- Copyright
- Copyright © International Astronomical Union 2013
References
Dere, K. P., Landi, E., Young, P. R., Del Zanna, G., Landini, M., & Mason, H. E., 2009, A&A, 498, 915Google Scholar
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