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We have constructed an instrument to measure the polarization of light emitted by the solar corona in order to constrain the strength and orientation of coronal magnetic fields. We have constructed an instrument to measure the polarization of light emitted by the solar corona and prominences in order to constrain the strength and orientation of coronal magnetic fields. “the most striking aspect of the subject of magnetic fields in the corona is the frequency and variety of situations for which they are postulated, compared to the scarcity of any definite information concerning them.” from donald e
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It will measure the stokes parameters at the 1074.7 and 1079.8 fexiii coronal emission lines, and the 1083.0 nm hei chromospheric line.
