arXiv:1001.2720 [astro-ph.SR]AbstractReferencesReviewsResources
On the Sensitivity of the H$α$ Scattering Polarization to Chromospheric Magnetism
Jiri Stepan, Javier Trujillo Bueno
Published 2010-01-15Version 1
A particularly interesting line for exploring the physical conditions of the quiet solar chromosphere is H$\alpha$, but its intensity profile is magnetically insensitive and the small circular polarization signatures produced by the longitudinal Zeeman effect come mainly from the underlying photosphere. Here we show that the Hanle effect in H$\alpha$ provides quantitative information on the magnetism of the quiet chromosphere. To this end, we calculate the response function of the emergent scattering polarization to perturbations in the magnetic field.
Comments: 4 pages, 4 figures, to appear in the proceedings of the 25th NSO Workshop "Chromospheric Structure and Dynamics. From Old Wisdom to New Insights", Memorie della Societa' Astronomica Italiana
Categories: astro-ph.SR
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