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Non-LTE Modeling and Observations of Oscillating Prominences

Published online by Cambridge University Press:  06 January 2014

M. Zapiór ,
P. Heinzel ,
R. Oliver ,
J. L. Ballester  and
P. Kotrč
M. Zapiór
Affiliation:
Departament de Física, Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain email: [email protected]; [email protected]; [email protected] Astronomical Institute, Academy of Sciences, 25165 Ondřejov, Czech Republic email: [email protected]; [email protected]
P. Heinzel
Affiliation:
Astronomical Institute, Academy of Sciences, 25165 Ondřejov, Czech Republic email: [email protected]; [email protected]
R. Oliver
Affiliation:
Departament de Física, Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain email: [email protected]; [email protected]; [email protected]
J. L. Ballester
Affiliation:
Departament de Física, Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain email: [email protected]; [email protected]; [email protected]
P. Kotrč
Affiliation:
Astronomical Institute, Academy of Sciences, 25165 Ondřejov, Czech Republic email: [email protected]; [email protected]
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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.

Keywords

Sun: oscillationsSun: filamentsSun: prominences
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

Heinzel, P. 1995, A&A, 299, 563Google Scholar
Kotrč, P. 2009, Central European Astrophysical Bulletin, 33, 327Google Scholar
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