A spectroscopic method for the solution of the 180-deg azimuth ambiguity in magnetograms

Details A spectroscopic method for the solution of the 180-deg azimuth ambiguity in magnetograms A spectroscopic method for the solution of the 180-deg azimuth ambiguity in magnetograms

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...411l..49l&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 411, no. 1, p. L49-L52.

Astronomy and Astrophysics

Astrophysics

14

Astronomical Spectroscopy, Solar Magnetic Field, Integral Equations, Linear Polarization, Magnetic Field Configurations, Resonance Lines

Scientific paper

A spectroscopic method is proposed for removing the azimuth ambiguity intrinsically present in vector magnetograms. The method is based on the idea that the polarization observed in resonance lines (typically formed at the chromospheric level) depends not only on the magnetic field vector, but also on the anisotropy of the radiation field that is illuminating the scattering atoms. An observational scheme is proposed.

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