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Polarization control at the microscopic and electronic structure observatory

机译:显微和电子结构天文台的偏振控制

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The new Microscopic and Electronic Structure Observatory (MAESTRO) at the Advanced Light Source (ALS) Berkeley in provides X-rays of variable polarization, produced by an elliptically polarized undulator (EPU), for angle resolved photoemission (ARPES) and photoemission electron microscopy (PEEM) experiments. The interpretation of photoemission data, in particular of dichroism effects in ARPES, requires the precise knowledge of the exact polarization state. Numerical simulations show that the first harmonics of the EPU at MAESTRO provides soft X-rays of almost 100% on axis polarization. However, the higher harmonics as well as the downstream optical elements of the beamline, have a considerable impact on the polarization of the light delivered to the experimental end-station. Employing a simple reflective polarimeter, the polarization is characterized for variable EPU and beamline settings and the overall degree of polarization in the MAESTRO end-stations is estimated to be on the order of 83%.
机译:位于伯克利先进光源(ALS)的新型显微电子结构天文台(MAESTRO)提供由椭圆偏振波荡器(EPU)产生的可变偏振X射线,用于角度分辨光发射(ARPES)和光发射电子显微镜( PEEM)实验。解释光发射数据,特别是ARPES中的二色性效应,需要对确切的偏振态有确切的了解。数值模拟表明,MAESTRO的EPU的一次谐波提供了几乎100%的轴偏振软X射线。但是,光束线的高次谐波以及下游光学元件对传递到实验终端的光的偏振有相当大的影响。使用简单的反射偏振仪,可对可变的EPU和光束线设置进行偏振表征,而MAESTRO终端站的总体偏振度估计约为83%。

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