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Publikováno v:
SPIE Proceedings.
In order to demonstrate optical technology readiness for the Advanced X-ray Astrophysical Facility (AXAF), a Wolter Type I telescope was built. This telescope, called the Technology Mirror Assembly (TMA), was designed to have a system resolution of 0
Publikováno v:
SPIE Proceedings.
The achievement of the derived goals for mirror surface quality on the Advanced X-ray Astrophyscis Facility (AXAF), Technology Mirror Assembly (TMA) required a combination of state-of-the-art metrology and polishing techniques. In this paper, we summ