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A Statistical Investigation of Prominence Fine Structure in the EUV

Published online by Cambridge University Press:  12 April 2016

S. Pojoga ,
A.G. Nikoghossian  and
Z. Mouradian
S. Pojoga
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon Cedex, France
A.G. Nikoghossian
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon Cedex, France
Z. Mouradian
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon Cedex, France

Abstract

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A statistical approach is proposed for the study of the prominence fine structure. Intensity variations in several EUV lines are measured in different regions of prominences. The expected number of fine structural elements is derived.

Type
Filaments and Their Environment
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 59 - 62
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Engvold, O., Jensen, E., Zhang, Y. and Brynildsen, N. 1989, Hvar Obs. Bull., 13(1), 205 Google Scholar
Nikoghossian, A.G., Pojoga, S. and Mouradian, Z. 1997, A&A, 325, 813 Google Scholar
Orrall, F.Q. and Schmahl, E.J. 1980, ApJ, 240, 908 CrossRefGoogle Scholar
Pojoga, S., Nikoghossian, A.G. and Mouradian, Z. 1998, A&A, to be submittedGoogle Scholar
Zirker, J.B. and Koutchmy, S. 1990, Sol. Phys., 127, 109 CrossRefGoogle Scholar