The effects of ray aberrations due to various surface errors on the point image are discussed, and a new method and rationale for optimizing the performance of nested arrays of grazing incidence telescopes is introduced.
Technical support for AXAF
1983-11-01
Report
No indication
English
Tema Archive | 1989
|British Library Online Contents | 1992
|Axaf Hypervelocity Impact Test Results
British Library Online Contents | 1997
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