The Hanle effect as diagnostic tool for turbulent magnetic fields

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DC Field	Value	Language
dc.contributor.author	Anusha, L. S	-
dc.contributor.author	Sampoorna, M	-
dc.contributor.author	Frisch, H	-
dc.contributor.author	Nagendra, K. N	-
dc.date.accessioned	2010-05-19T17:13:46Z	-
dc.date.available	2010-05-19T17:13:46Z	-
dc.date.issued	2010	-
dc.identifier.citation	Hasan, 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. 390 – 394	en
dc.identifier.isbn	978-3-642-02858-8	-
dc.identifier.uri	http://hdl.handle.net/2248/5120	-
dc.description	Open Access	-
dc.description.abstract	The Hanle effect is calculated for a random magnetic field characterized by a finite correlation length and a probability density function of the magnetic field vector. It is shown that linear polarization is essentially independent of the magnetic field correlation length, but strongly depends on the distribution of the field strength.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.ispartofseries	Astrophysics and Space Science Proceedings;	-
dc.relation.uri	http://www.springerlink.com/content/p1301351068134v8/	en
dc.rights	© Springer	en
dc.title	The Hanle effect as diagnostic tool for turbulent magnetic fields	en
dc.type	Article	en
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