On the Polarization Degree of the Inner White Light Corona on March 29, 2006

Details On the Polarization Degree of the Inner White Light Corona on March 29, 2006 On the Polarization Degree of the Inner White Light Corona on March 29, 2006

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..405..435p&link_type=abstract

Solar Polarization 5: In Honor of Jan Stenflo ASP Conference Series, Vol. 405, proceedings of the conference held 17-21 Septembe

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Results of the preliminary data reduction of the eclipse white-light corona polarimetry by a portable low-scattered light coronagraph are presented. Broad-band RGB polarization recordings (movies) were obtained in the range 1.05--1.5 solar radii. A special algorithm for data reduction was used to get the 2D distributions of the linear polarization degree in the green and in the red spectral intervals with an accuracy of 1%. Polar plumes are evidently traced in the polarization patterns. Everywhere in the corona the polarization degree in the red is 5-25% lower than in the green.

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