Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1712
Title: Turbulent magnetic field averages for the Zeeman effect
Authors: Frisch, H
Sampoorna, M
Nagendra, K. N
Keywords: Polarization;magnetic fields;radiative transfer;Sun: atmosphere
Issue Date: 2007
Publisher: Societa Astronomica Italiana
Citation: Mem. S.A.It. Vol. 78, pp. 142 - 147
Abstract: Stokes parameters measured in the Solar atmosphere are in general time or space averages over a magnetic field probability distribution function. Here we show how to write the Zeeman propagation matrix in a reference frame defined with respect to the direction of a mean magnetic field and how to average over a random magnetic field distribution. We concentrate on the case of a normal Zeeman triplet but indicate how to treat general Zeeman patterns. Numerical results are presented for Gaussian distributions having cylindrical symmetry about a mean field. Di erent models of probability distribution functions (PDF), are compared.
URI: http://hdl.handle.net/2248/1712
???metadata.dc.relation.uri???: http://sait.oat.ts.astro.it/MSAIt780107/PDF/2007MmSAI..78..142F.pdf
Appears in Collections:IIAP Publications

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