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Non-LTE Modeling and Observations of Oscillating Prominences
Published online by Cambridge University Press: 06 January 2014
Abstract
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Prominence oscillations have been mostly detected using Doppler velocity, although there are also claimed detections by means of the periodic variations of half-width or line intensity. Our main aim here is to explore the relationship between spectral indicators such as Doppler shift, line intensity and line half-width and the linear perturbations excited in a simple prominence model.
- 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. 52 - 55
- Copyright
- Copyright © International Astronomical Union 2013
References
Labrosse, N., Heinzel, P., Vial, J.-C., Kucera, T., Parenti, S., Gunár, S., & Schmieder, B. and Kilper, G. 1993, Space Sci. Revs, 151, 243Google Scholar
Oliver, R., Ballester, J. L., & Hood, A. W. and Priest, E. R. 1993, ApJ, 400, 369CrossRefGoogle Scholar
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