Spectropolarimetric studies of H alpha emission in "solar moustaches": Observations and calculation of the Stokes parameters

Details Spectropolarimetric studies of H alpha emission in "solar moustaches": Observations and calculation of the Stokes parameters Spectropolarimetric studies of H alpha emission in "solar moustaches": Observations and calculation of the Stokes parameters

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arep...42..702k&link_type=abstract

Astronomy Reports, Volume 42, Issue 5, September 1998, pp.702-706

Astronomy and Astrophysics

Astronomy

2

Scientific paper

The results of spectropolarimetric observations of three solar `moustaches' carried out on the Large Vacuum Solar Telescope of Baikal Observatory of the Institute of Solar-Terrestrial Physics are presented. The observed degree of polarization varies from 2-13%. The direction of the plane of polarization for a moustache with moderate intensity is tangential, and is radial for the weakest moustache. In the brightest moustache, the plane of polarization is close to radial at the line center, and is tangential in the wings.

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