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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5118
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dc.contributor.authorSampoorna, M-
dc.date.accessioned2010-05-19T17:06:34Z-
dc.date.available2010-05-19T17:06:34Z-
dc.date.issued2010-
dc.identifier.citationHasan, S. S and Rutten, R. T., eds., Magnetic coupling between the interior and atmosphere of the Sun, Proceedings of the conference "Centenary commemoration of the discovery of the Evershed effect" Dec, 2 - 5, 2008, Indian Institute of Astrophysics, Bangalore, India, pp. 141 – 149en
dc.identifier.issn978-3-642-02858-8-
dc.identifier.urihttp://hdl.handle.net/2248/5118-
dc.descriptionOpen Access-
dc.description.abstractNumerical simulations of magneto-convection and analysis of solar magnetogram data provide empirical probability density functions (PDFs) for the line-of-sight component of the magnetic field. In this paper, we theoretically explore effects of several types of PDFs on polarized Zeeman line formation. We also propose composite PDFs to account for randomness in both field strength and orientation. Such PDFs can possibly mimic random fields at the solar surface.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesAstrophysics and Space Science Proceedings;-
dc.relation.urihttp://arxiv.org/abs/0903.1911en
dc.relation.urihttp://dx.doi.org/10.1007/978-3-642-02859-5_10en
dc.rights© Springeren
dc.titleProbability density functions to represent magnetic fields at the solar surfaceen
dc.typeArticleen
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