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Space-resolving flat-field extreme ultraviolet spectrograph system and its aberration analysis with wave-front aberration

机译:空间分辨平场极紫外光谱仪系统及其波前像差的像差分析

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摘要

The Nam aberration of a fiat-field extreme ultraviolet spectrograph system, composed of a varied line-spacing concave grating and a toroidal mirror, was analyzed by calculating the wave-front aberration with respect to an astigmatic reference surface. The toroidal mirror was used to compensate for the astigmatism that was due to the grazing incidence of light at the concave grating. The spectrograph system could form a space-resolved spectrum along the sagittal direction. The spectral and spatial resolutions of the spectrograph system were estimated from the root-mean-square spot size. The actual spectral resolution of the spectrograph system was measured from extreme ultraviolet spectra obtained from plasmas produced by an iodine laser having an energy of 0.5 J in a 4-ns duration, and it was compared with the calculated value, # 1997 Optical Society of America
机译:通过计算相对于像散参考面的波前像差,分析了由可变行距凹面光栅和环形镜组成的平场极紫外光谱仪系统的南像差。环形反射镜用于补偿由于光在凹面光栅上的掠入射而引起的像散。光谱仪系统可以沿着矢状方向形成空间分辨光谱。光谱仪系统的光谱和空间分辨率是根据均方根光斑大小估算的。光谱仪系统的实际光谱分辨率是通过在4-ns的持续时间内从具有0.5 J能量的碘激光器产生的等离子体中获得的极端紫外光谱中测得的,并与计算值进行比较(美国1997年光学学会)

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