Diagnosis of Faraday Rotation with the Video Vector Magnetograph at Huairou

Details Diagnosis of Faraday Rotation with the Video Vector Magnetograph at Huairou Diagnosis of Faraday Rotation with the Video Vector Magnetograph at Huairou

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hia....13..139s&link_type=abstract

Highlights of Astronomy, Vol. 13, as presented at the XXVth General Assembly of the IAU - 2003 [Sydney, Australia, 13 - 26 July

Astronomy and Astrophysics

Astronomy

Scientific paper

In this paper we present results of the inversion of Stokes polarization profiles to recover the vector magnetic field parameters of the spectral line forming region using the FeI 5324.19A spectral line using a nonlinear least-squares itting. At the same time curves of the observed variation of azimuth with wavelength were fitted with model calculations for the azimuth at each position of the line profile as derived the inverse Zeeman effect modified by Faraday rotation. The results show that Faraday rotation seem to be insignificant in observation taken near the center of the Fe I 5324.19A spectral line.

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