Lobster Eye X-ray Optics
Rene Hudec, Charly Feldman

TL;DR
This paper reviews the principles, recent developments, and applications of lobster eye X-ray optics, highlighting their potential for wide-field X-ray imaging in astronomy and laboratory settings.
Contribution
It provides a comprehensive overview of lobster eye X-ray optics, including design principles, recent innovations, and their applications in space and laboratory environments.
Findings
Lobster eye optics enable wide field of view X-ray imaging.
Micro Pore Optics (MPOs) are key components in lobster eye systems.
Multi Foil Optics (MFO) offers a promising alternative for future applications.
Abstract
This chapter describes the history, principles, and recent developments of large field of view X-ray optics based on lobster eye designs. Most of grazing incidence (reflective) X-ray imaging systems used in astronomy and other applications, are based on the Wolter 1 (or modified) arrangement. But there are also other designs and configurations proposed for future applications for both laboratory and space environments. Kirkpatrick-Baez (K-B) based lenses as well as various types of lobster eye optics serve as an example. Analogously to Wolter lenses, all these systems use the principle that the X-rays are reflected twice to create focal images. Various future projects in X-ray astronomy and astrophysics will require large optics with wide fields of view. Both large Kirkpatrick-Baez modules and lobster eye X-ray telescopes may serve as solutions as these can offer innovations such as…
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Taxonomy
TopicsAdvanced X-ray Imaging Techniques · Astrophysical Phenomena and Observations · Adaptive optics and wavefront sensing
