Stray light and polarimetry considerations for the COSMO K-Coronagraph
2012
The COSMO K-Coronagraph is scheduled to replace the aging Mk4 K-Coronameter at the Mauna Loa Solar
Observatory of the National Center for Atmospheric Research in 2013. We present briefly the science objectives and
derived requirements, and the optical design. We single out two topics for more in-depth discussion: stray light, and
performance of the camera and polarimeter.
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