A Test Facility For Astronomical X-Ray Optics

R. A. Lewis, J. Bordas, Finn Erland Christensen

    Research output: Contribution to journalConference articleResearchpeer-review

    Abstract

    Grazing incidence x-ray optics for x-ray astronomical applications are used outside the earths atmosphere. These devices require a large collection aperture and the imaging of an x-ray source which is essentially placed at infinity. The ideal testing system for these optical elements has to approximate that encountered under working conditions, however the testing of these optical elements is notoriously difficult with conventional x-ray generators. Synchrotron Radiation (SR) sources are sufficiently brilliant to produce a nearly perfect parallel beam over a large area whilst still retaining a flux considerably higher than that available from conventional x-ray generators. A facility designed for the testing of x-ray optics, particularly in connection with x-ray telescopes is described below. It is proposed that this facility will be accommodated at the Synchrotron Radiation Source at the Daresbury Laboratory in the U.K.
    Original languageEnglish
    JournalProceedings of SPIE - The International Society for Optical Engineering
    Volume1160
    Pages (from-to)500-506
    Number of pages7
    ISSN0277-786X
    DOIs
    Publication statusPublished - 1989
    Event33rd Annual Technical Symposium: X-Ray/EUV Optics for Astronomy and Microscopy - San Diego, United States
    Duration: 7 Aug 198911 Aug 1989
    Conference number: 33

    Conference

    Conference33rd Annual Technical Symposium
    Number33
    Country/TerritoryUnited States
    CitySan Diego
    Period07/08/198911/08/1989

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