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.
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References
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© 1999 Springer Science+Business Media Dordrecht
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Puschmann, K., Hanslmeier, A., Solanki, S.K. (1999). Solar Line Bisectors in the Infrared. In: Hanslmeier, A., Messerotti, M. (eds) Motions in the Solar Atmosphere. Astrophysics and Space Science Library, vol 239. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9331-1_15
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DOI: https://doi.org/10.1007/978-94-015-9331-1_15
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5151-6
Online ISBN: 978-94-015-9331-1
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