The multi-component field topology of sunspot penumbrae : A diagnostic tool for spectropolarimetric measurements

• Published in: Astronomy and astrophysics (Berlin) Vol. 460; no. 3; pp. 925 - 933
• Main Authors: MÜLLER, D. A. N, SCHLICHENMAIER, R, FRITZ, G, BECK, C
• Format: Journal Article
• Language: English
• Published: Les Ulis EDP Sciences 01.12.2006
• Subjects: Astronomy; Earth, ocean, space; Exact sciences and technology; Discontinuity; Atmosphere model; Circular polarization; Flux tubes; Flow pattern; Sun: photosphere; Topology; Penumbra; Sun; Geometrical model; Sun: atmosphere; Three dimensional model; Physical parameter; Sun: magnetic fields; Sun: sunspots; Magnetic structure; Modelling; Radiative transfer; Magnetic fields; Sunspots; Sun: infrared; Spectropolarimetry
• ISSN: 0004-6361; 1432-0746
• DOI: 10.1051/0004-6361:20066062

Context. Sunspot penumbrae harbor highly structured magnetic fields and flows. The moving flux tube model offers an explanation for several observed phenomena, e.g. the Evershed effect and bright penumbral grains. Aims. A wealth of information can be extracted from spectropolarimetric observations. In order to deduce the structure of the magnetic field in sunspot penumbrae, detailed forward modeling is necessary. On the one hand, it gives insight into the sensitivity of various spectral lines to different physical scenarios. On the other hand, it is a very useful tool to guide inversion techniques. In this work, we present a generalized 3D geometrical model that embeds an arbitrarily shaped flux tube in a stratified magnetized atmosphere. Methods. The new semi-analytical geometric model serves as a frontend for a polarized radiative transfer code. The advantage of this model is that it preserves the discontinuities of the physical parameters across the flux tube boundaries. This is important for the detailed shape of the emerging Stokes Profiles and the resulting net circular polarization (NCP). Results. (a) The inclination of downflows in the outer penumbra must be shallower than approximately 15 logical or circ; (b) observing the limb-side NCP of sunspots in the \ion{1} 1564.8 nm line offers a promising way to identify a reduced magnetic field strength in flow channels; (c) the choice of the background atmosphere can significantly influence the shape of the Stokes profiles, but does not change the global characteristics of the resulting NCP curves for the tested atmospheric models.