X-ray telescopes

This review summarises the present knowledge about X-ray reflection from real mirrors, with particular emphasis on X-ray scattering. The mirror configurations for a telescope are presented and their imaging capabilities are discussed. The fabrication techniques and the supporting metrology methods used for the manufacture of highly aspherical telescope mirrors are outlined, including direct grinding and polishing as well as replication methods. An account is given of the achievements obtained so far for the telescopes built for solar and non-solar X-ray astronomy applications.

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[75]  E. Costa,et al.  Reflectivity of gold coated surfaces in the soft x-ray range. , 1978, Applied optics.

[76]  J M Zavada,et al.  Residual surface roughness of diamond-turned optics. , 1975, Applied optics.

[77]  M. Zombeck AXAF, a permanent orbiting X-ray observatory - Telescope and instrumentation plans , 1982 .

[78]  Dirk Rudolph,et al.  Status Of The Zone Plate Microscope , 1982, Other Conferences.

[79]  B. Aschenbach,et al.  Design and construction of the ROSAT 5 arcsec mirror assembly , 1982 .

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[81]  J. H. Underwood,et al.  S056 x-ray telescope experiment on the Skylab Apollo Telescope Mount. , 1977, Applied optics.

[82]  Martin V. Zombeck,et al.  High Resolution X-Ray Scattering Measurements , 1982, Other Conferences.

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[84]  H. Brauninger,et al.  Measurements Of X-Ray Scattering From Wolter Type Telescopes and Various Flat Zerodur Mirrors , 1981, Other Conferences.

[85]  Wolfgang K. H. Schmidt,et al.  A proposed X-ray focusing device with wide field of view for use in X-ray astronomy , 1975 .

[86]  Scatter from X-ray Reflecting Surfaces. , 1968, Applied optics.