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Dependence of Solar Line Bisectors on Equivalent Widths

Published online by Cambridge University Press:  27 September 2017

A. Hanslmeier ,
W. Mattig  and
A. Nesis
A. Hanslmeier
Affiliation:
Inst. f. Astronomie, Graz, Austria
W. Mattig
Affiliation:
Kiepenheuer Inst., Freiburg, F.R.G.
A. Nesis
Affiliation:
Kiepenheuer Inst., Freiburg, F.R.G.

Abstract

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Spectroscopic highly resolved solar granulation observations lead to intense line asymmetries for rising and sinking elements. In order to average several granules it is better to use equivalent widths than continuum intensities.

Type
Session II: Solar Flares
Information
International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 251 - 254
Copyright
Copyright © Kluwer 1989

References

Dravins, D.: 1982, Ann.Rev.Astron.Astrophys. 20, 61 CrossRefGoogle Scholar
Kavetsky, A., O'Mara, B.J.: 1984, Solar Phys. 92, 47 CrossRefGoogle Scholar
Keil, S.L., Yackovich, F.H.: 1981, Solar Phys. 69, 213 CrossRefGoogle Scholar
Musmann, S.: 1969, Solar Phys. 7, 178 Google Scholar
Schröter, E.H.: 1957, Z.Astrophys. 41, 141 Google Scholar
Steffen, M.: 1987, in “The Role of Fine-Scale Magnetic Fields on the Structure of the Solar Atmosphere”, ed. Schröter, E.H., Vazquez, M., Wyller, A.A., 47 Google Scholar
Voigt, H.H.: 1956, Z.Astrophys. 40, 157 Google Scholar