Abstract
Full Stokes polarimetry is obtained using the National Solar Observatory Vacuum Tower Telescope at Sacramento Peak while observing the magnetically sensitive infrared Fei line at wavelength of 1.56μ. A technique is described which makes use of the high magnetic resolution in this spectral range to remove instrumental polarization from observed StokesQ, U, andV line profiles.
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Supported under a USAF/AFOSR research initiative.
Operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation.
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Kuhn, J.R., Balasubramaniam, K.S., Kopp, G. et al. Removing instrumental polarization from infrared solar polarimetric observations. Sol Phys 153, 143–155 (1994). https://doi.org/10.1007/BF00712497
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DOI: https://doi.org/10.1007/BF00712497