X-ray telescope

TL;DR: In this article, an X-ray telescope displaying Xray radiation with wavelength λ comprising a band comprised of bent monocrystalline plates (1, 2) with atomic planes (5) parallel to the surface of these plates, was presented.

Abstract: The present invention relates to an X-ray telescope displaying X-ray radiation with wavelength {lambda} comprising a band comprised of bent monocrystalline plates (1, 2) with atomic planes (5) parallel to the surface of these monocrystalline plates (1, 2), wherein the distance of the monocrystalline plates (1, 2) from each other changes in each monocrystalline plate (1, 2) according to the following relationship d = wherein n is a natural number indicating number of wavelengths {lambda} falling on the difference of ray trajectories upon reflection from two adjacent atomic planes (5) and p represents the double of the distance of the focal line (F) from a crest line (V) of a parabolic band, i.e. that for a given monocrystalline plate (1, 2) extending between (ximin) and (ximax) stands for the relationship = , wherein (di0) represents the distance between the atomic planes (5) at a point with the coordinate (ximin) and (d) represents the distance between the atomic planes (5) at a point with the coordinate (x). This characteristic can be achieved by distribution of temperatures in various places according to the experimentally measured dependence of a grid parameter {gamma} on the temperature value T(x) = T(ximin) +