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Polarization Model for the New Vacuum Solar Telescope
Yuan S(袁沭); Yuan, S (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming, Yunnan, Peoples R China.
会议录名称Astronomical Society of the Pacific (ASP) Conference Series - SOLAR POLARIZATION 7
2014-10
卷号489
页码297-304
产权排序第1完成单位
收录类别CPCI
会议名称7th Solar Polarization Workshop (SPW7)
会议日期2013-09-09
会议地点Kunming, PEOPLES R CHINA
摘要It is essential to properly calibrate the instrumental polarization for solar telescopes, if one wants to achieve a high spectro-polarimetric accuracy. Model fitting is an efficient calibration method for telescopes with alt-azimuth mount. We have constructed an ideal model for the New Vacuum Solar Telescope (NVST) which describes its pupil and time-dependent polarization properties. An integration of polarization raytracing in pupil is implemented for solving the net polarization of main optics. The time and season-dependent polarization of the Coude optics is calculated based on the NVST ´ geometry and complex refractive index of ideal Al film.
语种英语
学科领域Astronomy & Astrophysics
文章类型Proceedings Paper
出版者ASTRONOMICAL SOC PACIFIC
出版地390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
ISBN号978-1-58381-863-3; 978-1-58381-862-6
URL查看原文
归档日期2014-11-21
WOS记录号WOS:000370308600029
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
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文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9653
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通讯作者Yuan, S (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming, Yunnan, Peoples R China.
作者单位Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, China
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GB/T 7714
Yuan S,Yuan, S . Polarization Model for the New Vacuum Solar Telescope[C]. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2014:297-304.
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