Park J, Brown G V, Schneider M B, Baldis H A, Beiersdorfer P, Cone K V, Kelley R L, Kilbourne C A, Magee E W, May M J, Porter F S
Lawrence Livermore National Laboratory, P.O. Box 808, Livermore, California 94551-0808, USA.
Rev Sci Instrum. 2010 Oct;81(10):10E319. doi: 10.1063/1.3495790.
We have calibrated the x-ray response of a variable line spaced grating spectrometer, known as the VSG, at the Fusion and Astrophysics Data and Diagnostic Calibration Facility at the Lawrence Livermore National Laboratory (LLNL). The VSG has been developed to diagnose laser produced plasmas, such as those created at the Jupiter Laser Facility and the National Ignition Facility at LLNL and at both the Omega and Omega EP lasers at the University of Rochester's Laboratory for Laser Energetics. The bandwidth of the VSG spans the range of ∼6-60 Å. The calibration results presented here include the VSG's dispersion and quantum efficiency. The dispersion is determined by measuring the x rays emitted from the hydrogenlike and heliumlike ions of carbon, nitrogen, oxygen, neon, and aluminum. The quantum efficiency is calibrated to an accuracy of 30% or better by normalizing the x-ray intensities recorded by the VSG to those simultaneously recorded by an x-ray microcalorimeter spectrometer.
我们在劳伦斯利弗莫尔国家实验室(LLNL)的聚变与天体物理数据及诊断校准设施中,对一种名为可变线间距光栅光谱仪(VSG)的X射线响应进行了校准。VSG是为诊断激光产生的等离子体而开发的,比如在LLNL的木星激光设施和国家点火设施以及罗切斯特大学激光能量学实验室的欧米茄和欧米茄EP激光器上产生的等离子体。VSG的带宽范围约为6 - 60埃。这里给出的校准结果包括VSG的色散和量子效率。色散是通过测量碳、氮、氧、氖和铝的类氢离子和类氦离子发射的X射线来确定的。通过将VSG记录的X射线强度与X射线微热量计光谱仪同时记录的强度进行归一化,将量子效率校准到30%或更高的精度。