Motions in the Solar Atmosphere pp 227-230 | Cite as
Solar Line Bisectors in the Infrared
Conference paper
Abstract
In the present work we made some analysis with respect to shifts and asymmetries of infrared solar spectral lines to get information about vertical velocity fields in the deep layers of the Solar Photosphere. For the analysis of shifts and asymmetries of bisectors were used. We averaged bisectors belonging to a group of similar line parameter. Therefore it was possible, to analyse correlations between asymmetries and line shifts and corresponding vertical velocities with line parameters and to discuss the results with other literature.
Keywords
Wavelength Shift Equivalent Width Line Shift Line Parameter Line Core
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References
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© Springer Science+Business Media Dordrecht 1999