Astrophysical Observations with High Resolution X-ray Telescopes

Physics – Optics

Scientific paper

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Image Processing, X-Ray

Scientific paper

In slightly less than twenty years, from its birth in 1962, X-ray astronomy has developed into a major branch of astronomy, equalling in importance the more established disciplines for the study of astrophysical problems. This has resulted from two major technological advances: 1) the capability of placing into space, above the Earth's attenuating atmosphere, large and sophisticated scientific payloads, and 2) the development of high resolution X-ray imaging optics and associated detectors. This paper illustrates the rapid development of X-ray imaging optics and discusses their application to astrophysical observations, both solar and non-solar. In conjunction with various spectroscopic techniques, X-ray telescopes are being used for astrophysical plasma diagnostics, obtainig elemental abundances, temperatures, and densities. Several examples are given. Further advances in X-ray imaging optics will require the development of new metrology techniques in order to determine and control mirror figure and scattering. Future programs are discussed.

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