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首页> 外文期刊>PASJ: Publications of the Astronomical Society of Japan >The Tandem Etalon Magnetograph of the Solar Magnetic Activity Research Telescope (SMART) at Hida Observatory
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The Tandem Etalon Magnetograph of the Solar Magnetic Activity Research Telescope (SMART) at Hida Observatory

机译:飞ida天文台太阳磁活动研究望远镜(SMART)的串联标准具磁力仪

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摘要

The imaging photospheric magnetograph using tandem Fabry–Perot filters is newly installed in the Solar Magnetic Activity Research Telescope (SMART) of Hida Observatory, Kyoto University. The instrument, Tandem Etalon Magnetograph (TEM), consists of a rotating wave plate, tandem Fabry–Perot filters which scan the Fe I 6302.5 ? line with ~130 m? bandwidth, a polarizing beam splitter, and two CCD cameras simultaneously taking orthogonally polarized light with a frame rate of 30 frames per second. We have confirmed that the Stokes vector map deduced from 20 s integration achieves a polarimetric sensitivity of ~5 × 10~(?4) for all polarization states at one wavelength, which is higher than is achieved with a space instrument such as the Spectro-Polarimeter aboard Hinode or the Helioseismic and Magnetic Imager aboard the Solar Dynamic Observatory (SDO). We expect the complementary observations by SMART/TEM, Hinode, and SDO can shed new light on the trigger and energy storage mechanism of solar flares.
机译:使用串联法布里-珀罗滤光片的成像光球磁力仪是新安装在京都大学飞ida天文台的太阳磁活动研究望远镜(SMART)中。串联式Etalon磁力仪(TEM)由旋转波片,串联法布里-珀罗滤波器组成,可扫描Fe I 6302.5? 〜130 m?带宽,一个偏振分束器和两个CCD摄像机同时以每秒30帧的帧速率拍摄正交偏振光。我们已经确认,通过20 s积分推导的斯托克斯矢量图对于一个波长下的所有偏振态均实现约5×10〜(?4)的偏振灵敏度,这比使用诸如Spectro- Hinode上的旋光仪或太阳动态天文台(SDO)上的日震和磁成像仪。我们期望SMART / TEM,Hinode和SDO的补充观测可以为太阳耀斑的触发和能量存储机制提供新的思路。

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