Removing instrumental polarization from infrared solar polarimetric observations

Removing instrumental polarization from infrared solar polarimetric observations
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DOI：
10.1007/bf00712497
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发表时间：
1994-08
期刊：
Solar Physics
影响因子：
2.8
通讯作者：
J. Kuhn;K. Balasubramaniam;G. Kopp;M. Penn;A. Dombard;H. Lin
J. Kuhn;K. Balasubramaniam;G. Kopp;M. Penn;A. Dombard;H. Lin
中科院分区：
物理与天体物理3区
文献类型：
--
作者：
J. Kuhn;K. Balasubramaniam;G. Kopp;M. Penn;A. Dombard;H. Lin

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Full Stokes polarimetry is obtained using the National Solar Observatory Vacuum Tower Telescope at Sacramento Peak while observing the magnetically sensitive infrared Feiline 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, andVline profiles.