Stokes profile analysis and vector magnetic fields. VI: Fine scale structure of a sunspot

Stokes profile analysis and vector magnetic fields. VI: Fine scale structure of a sunspot
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DOI：
10.1086/173450
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发表时间：
1993-12
期刊：
The Astrophysical Journal
影响因子：
--
通讯作者：
B. Lites;D. Elmore;P. Seagraves;A. Skumanich
B. Lites;D. Elmore;P. Seagraves;A. Skumanich
中科院分区：
其他
文献类型：
--
作者：
B. Lites;D. Elmore;P. Seagraves;A. Skumanich

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利用高海拔天文台/国家太阳天文台高级斯托克斯偏振仪(ASP)的数据，研究了一个非常接近圆盘中心的对称小黑子的矢量磁场结构。该仪器首次提供了高角度分辨率的太阳黑子光球矢量磁场的定量信息，这些信息是从630 nm处塞曼敏感的铁线对的全斯托克斯分布得到的
The vector magnetic field structure of a small, symmetric sunspot observed very close to disk center has been explored using data from the High Altitude Observatory/National Solar Observatory Advanced Stokes Polarimeter (ASP). This instrument provides, for the first time, quantitative information on sunspot photospheric vector magnetic fields with high angular resolution, as derived from full Stokes profiles of the Zeeman-sensitive Fe I line pair at 630 nm