Abstract
A simple experimental method for comparison of the line formation heights in the solar photosphere is presented. Several Fe I lines are used to test the method.
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© 1999 Springer Science+Business Media Dordrecht
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Kučera, A., Rybák, J., Wöhl, H. (1999). Correlation of Velocity Fields at Different Heights in the Solar Photosphere. 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_13
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DOI: https://doi.org/10.1007/978-94-015-9331-1_13
Publisher Name: Springer, Dordrecht
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