计量交叉检查-先进x射线天体物理设施(AXAF)光学制造计划的一个基本方面

Optical Fabrication and Testing Workshop Pub Date : 1900-01-01 DOI:10.1364/oft.1992.thb4

T. E. Gordon, J. S. Patterson, P. Reid, D. Zweig

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摘要

AXAF天文台是美国宇航局计划的四个“大天文台”中的第三个。它被设计成在0.1到10 keV (124 - 1.24 Å)能量范围内成像宇宙x射线。镜面组件由四个同心共聚焦的沃尔特I型望远镜组成。每台望远镜包括两个锥形掠入射镜，一个抛物面和一个双曲面。

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Metrology Cross-checks - a fundamental aspect of the Advanced X-ray Astrophysics Facility (AXAF) Optics Fabrication Program

The AXAF observatory is the third of NASA's four planned "Great Observatories"1. It is designed to image cosmic x-rays in the energy regime of 0.1 to 10 keV (124 - 1.24 Å). The mirror assembly consists of four concentric, confocal, Wolter type I telescopes. Each telescope includes two conical grazing incidence mirrors, a paraboloid followed by a hyperboloid.

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Optical Fabrication and Testing Workshop

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