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20 July 2010Utilization of redundant polarized solar spectra to infer the polarization properties of the new generation of large aperture solar telescopes
Spectro-polarimetry plays an important role in the study of solar magnetism and strongly influences the design of the
new generation of solar telescopes. Calibration of the polarization properties of the telescope is a critical requirement
needed to use these observations to infer solar magnetic fields. However, the large apertures of these new telescopes
make direct calibration with polarization calibration optics placed before all the telescope optical elements impractical.
It is therefore desirable to be able to infer the polarization properties of the telescope optical elements utilizing solar
observations themselves. Taking advantage of the fact that the un-polarized, linearly, and circularly polarized spectra
originating from the Sun are uncorrelated, we have developed techniques to utilize observations of solar spectra with
redundant combination of the polarization states measured at several different telescope configurations to infer the
polarization properties of the telescope as a whole and of its optical elements. We show results of these techniques
applied to spectro-plarimetric data obtained at the Dunn Solar Telescope.
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David F. Elmore, Haosheng Lin, Héctor Socas Navarro, Sarah A. Jaeggli, "Utilization of redundant polarized solar spectra to infer the polarization properties of the new generation of large aperture solar telescopes," Proc. SPIE 7735, Ground-based and Airborne Instrumentation for Astronomy III, 77354E (20 July 2010); https://doi.org/10.1117/12.857061