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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.

Information

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

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