Weisskopf M C
Appl Opt. 1973 Jul 1;12(7):1436-9. doi: 10.1364/AO.12.001436.
The theoretical and practical constraints on designs of grazing-incidence x-ray telescopes are discussed. It is shown that there is a maximum useful diameter for an x-ray telescope. It is further shown that when practical constraints are considered, the maximum reflecting area is not necessarily achieved by utilizing the largest available area within this diameter. Equations are derived that allow rapid calculation of the effective area of an x-ray telescope before one proceeds to detailed studies utilizing Monte Carlo techniques.
讨论了掠入射X射线望远镜设计中的理论和实际限制。结果表明，X射线望远镜存在一个最大有用直径。进一步表明，当考虑实际限制时，最大反射面积不一定通过利用该直径内的最大可用面积来实现。推导了一些方程，这些方程允许在利用蒙特卡罗技术进行详细研究之前快速计算X射线望远镜的有效面积。
