The Horizontal Magnetic Field of the Quiet Sun: Numerical Simulations in Comparison to Observations with Hinode

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dc.creatorSteiner, O.
dc.creatorRezaei, R.
dc.creatorSchlichenmaier, R.
dc.creatorSchaffenberger, W.
dc.creatorWedemeyer-Böhm, S.
dc.date2009-04-13
dc.date.accessioned2026-07-07T13:03:40Z
dc.date.available2026-07-07T13:03:40Z
dc.descriptionThree-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.
dc.descriptionTo appear in "Second Hinode Science Meeting, Beyond Discovery -- Toward Understanding", eds. B. Lites, M. Cheung, K. Reeves, J. Mariska, and T. Magara ASP Conference Series xxx, 2009
dc.identifierhttps://arxiv.org/abs/0904.2030
dc.identifierhttp://arxiv.org/abs/0904.2030
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/226888
dc.subjectSolar and Stellar Astrophysics
dc.titleThe Horizontal Magnetic Field of the Quiet Sun: Numerical Simulations in Comparison to Observations with Hinode
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