Department of Physics, University of Alabama at Birmingham, Birmingham, Alabama 35294.
J Xray Sci Technol. 1989 Jan 1;1(2):190-206. doi: 10.3233/XST-1989-1207.
Normal incidence multilayer Cassegrain x-ray telescopes were flown on the Stanford/MSFC Rocket X-Ray Spectroheliograph. These instruments produced high spatial resolution images of the Sun and conclusively demonstrated that doubly reflecting multilayer x-ray optical systems are feasible. The images indicated that aplanatic imaging soft x-ray /EUV microscopes should be achievable using multilayer optics technology. We have designed a doubly reflecting normal incidence multilayer imaging x-ray microscope based on the Schwarzschild configuration. The Schwarzschild microscope utilizes two spherical mirrors with concentric radii of curvature which are chosen such that the third-order spherical aberration and coma are minimized. We discuss the design of the microscope and the results of the optical system ray trace analysis which indicates that diffraction-limited performance with 600 Å spatial resolution should be obtainable over a 1 mm field of view at a wavelength of 100 Å. Fabrication of several imaging soft x-ray microscopes based upon these designs, for use in conjunction with x-ray telescopes and laser fusion research, is now in progress. High resolution aplanatic imaging x-ray microscopes using normal incidence multilayer x-ray mirrors should have many important applications in advanced x-ray astronomical instrumentation, x-ray lithography, biological, biomedical, metallurgical, and laser fusion research.
常规入射角多层卡塞格林 X 射线望远镜曾搭载于斯坦福大学/马歇尔太空飞行中心的火箭 X 射线分光日冕仪上。这些仪器拍摄了高空间分辨率的太阳图像,明确证实了双层反射多层 X 射线光学系统是可行的。这些图像表明,使用多层光学技术可以实现消像差成像软 X 射线/EUV 显微镜。我们基于施瓦西(Schwarzschild)配置设计了一种双层反射常规入射角多层成像 X 射线显微镜。施瓦西显微镜采用两个同心曲率半径的球形反射镜,其选择方式使得第三阶球差和彗差最小化。我们讨论了显微镜的设计以及光学系统光线追踪分析的结果,该结果表明,在 100 Å 波长下,600 Å 空间分辨率的衍射极限性能应该可以在 1 毫米视场中获得。目前正在根据这些设计制作几个用于与 X 射线望远镜和激光聚变研究相结合的软 X 射线成像显微镜。使用常规入射角多层 X 射线反射镜的高分辨率消像差成像 X 射线显微镜在先进的 X 射线天文仪器、X 射线光刻、生物、生物医学、冶金和激光聚变研究等领域具有许多重要的应用。