Abstract
We present inversions based on two different flux-tube models, both of which reproduce the Stokes I and V profiles obtained in active region plages with high accuracy, including the V profile asymmetry. One model is almost identical to that employed by Bellot Rubio et al. (1997, 1999), and results in a significant downflow within the flux tube. The other, although similar in most respects, has mass conservation enforced inside the flux-tubes components.
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© 1999 Springer Science+Business Media Dordrecht
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Frutiger, C., Solanki, S.K., Fligge, M., Bruls, J.H.M.J. (1999). Inversion of Stokes Profiles. In: Nagendra, K.N., Stenflo, J.O. (eds) Solar Polarization. Astrophysics and Space Science Library, vol 243. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9329-8_22
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DOI: https://doi.org/10.1007/978-94-015-9329-8_22
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