Flat-Fielding of Solar Magnetograph Observations Using Relatively Shifted Images

Physics

Scientific paper

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Scientific paper

I present a method to correct solar magnetograms for a non-uniform
detector pattern that depends on the sense of light polarization. The
application to Big Bear Solar Observatory magnetograph observations
demonstrates that the determination of a flat pattern can be done at an
accuracy imposed by the photon noise in the raw magnetograms.

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