Peng Songwu, Ye Yizhong, Wei Fei, Yang Zuhua, Guo Yihong, Sun Tianran
Opt Express. 2018 Jun 11;26(12):15138-15152. doi: 10.1364/OE.26.015138.
Solar wind magnetosphere ionosphere link explorer (SMILE) scientific satellite is dedicated to observe solar wind-magnetosphere coupling. The key payload, soft X-ray imager (SXI), is designed to map the location, shape, and motion of dayside magnetospheric boundaries by Angel-type lobster-eye optical system. Contrast to traditional Wolter-type X-ray telescope with very narrow field-of-view, the lobster-eye-type optics has a unique capability of providing wide field of view for panoramic imaging with moderate spatial resolution in soft X-ray band. Since the lobster-eye optics focus X-ray by reflecting of the inner walls of the micro-channel array shaped in spherical surface, traditional optical design tools can't well match to the requirements of simulation for SXI. In this paper, a 3D Angel-type lobster-eye model is designed for simulation of lobster-eye optics and its capability is demonstrated for the applying scenarios including the imaging of point light source, surface light source with uniform and non-uniform intensity distribution. The simulation results are well consistent with those of theoretical estimate.
太阳风-磁层-电离层连接探测器(SMILE)科学卫星致力于观测太阳风-磁层耦合。关键载荷软X射线成像仪(SXI)旨在通过安吉尔型龙虾眼光学系统绘制日侧磁层边界的位置、形状和运动。与传统的具有非常窄视场的沃尔特型X射线望远镜不同,龙虾眼型光学器件具有独特的能力,能够在软X射线波段以中等空间分辨率提供宽视场进行全景成像。由于龙虾眼光学器件通过反射球形微通道阵列的内壁来聚焦X射线,传统的光学设计工具无法很好地满足SXI模拟的要求。本文设计了一个三维安吉尔型龙虾眼模型,用于模拟龙虾眼光学器件,并展示了其在包括点光源成像、强度分布均匀和不均匀的面光源成像等应用场景中的能力。模拟结果与理论估计结果高度一致。