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Grazing-Incidence Focusing Optics for X-Ray Telescopes (Review)

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Abstract

This review is devoted to the principles, state of the art, and problems of grazing-incidence optics for focusing soft X-ray radiation, which is used in telescopes at orbital stations. The possibilities of constructing light X-ray telescopes with a large effective data-collection area and good angular resolution, which are based on Kirkpatrick–Baez, Wolter, and “lobster eye” optics, are considered. Special attention is paid to the description of methods for optimizing the parameters for the production of X-ray optics and X-ray mirrors.

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Funding

This study was supported by the Ministry of Science and Education of the Russian Federation within the framework of studies on the State Job of the Crystallography and Photonics Federal Research Center, Russian Academy of Sciences.

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    V. V. Lider

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K–B—Kirkpatrick–Baez optical system; FoV—field of view; W–Sh—Wolter–Schwarzschild optical system; HPD—point scattering function; HEW—half-energy width; SPO—silicon porous optics; MCP—microchannel plate; MEMS—microelectromechanical system; ALE—“lobster eye” optics in the Angel geometry; ShLE—“lobster eye” optics in the Schmidt geometry.

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Lider, V.V. Grazing-Incidence Focusing Optics for X-Ray Telescopes (Review). Instrum Exp Tech 65, 191–217 (2022). https://doi.org/10.1134/S002044122202004X

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