Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2009-04-13
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
To appear in "Second Hinode Science Meeting, Beyond Discovery -- Toward Understanding", eds. B. Lites, M. Cheung, K. Reeves, J
Scientific paper
Three-dimensional magnetohydrodynamic simulations of the surface layers of the Sun intrinsically produce a predominantly horizontal magnetic field in the photosphere. This is a robust result in the sense that it arises from simulations with largely different initial and boundary conditions for the magnetic field. While the disk-center synthetic circular and linear polarization signals agree with measurements from Hinode, their center-to-limb variation sensitively depends on the height variation of the horizontal and the vertical field component and they seem to be at variance with the observed behavior.
Rezaei Rashid
Schaffenberger Werner
Schlichenmaier Rolf
Steiner Oskar
Wedemeyer-Böhm Sven
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