Abstract
The preliminary results of a classical spectroscopic analysis of a facular region at μ = 0.78 of ~ 100″×50″ are presented. The variation with magnetic activity of several spectroscopic parameters has been studied, showing clear evidence that granulation properties are modified.
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© 1999 Springer Science+Business Media Dordrecht
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Sainz, R.M., Hidalgo, I.R., Collados, M. (1999). Quiet and Active Granulation Properties. 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_8
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DOI: https://doi.org/10.1007/978-94-015-9331-1_8
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5151-6
Online ISBN: 978-94-015-9331-1
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