Lobster Eye X-ray Optics
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F24%3A00378146" target="_blank" >RIV/68407700:21230/24:00378146 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1007/978-981-19-6960-7_3" target="_blank" >https://doi.org/10.1007/978-981-19-6960-7_3</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/978-981-19-6960-7_3" target="_blank" >10.1007/978-981-19-6960-7_3</a>
Alternative languages
Result language
angličtina
Original language name
Lobster Eye X-ray Optics
Original language description
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 wide fields of view, low mass, and reduced costs. The basic workings of lobster eye optics using Micro-Pore Optics (MPOs) and their various uses are discussed. The issues and limiting factors of these optics are evaluated, and current missions using lobster eye optics to fulfill their science objectives are reviewed. The Multi-Foil Optics (MFO) approach represents a promising alternative. These arrangements can also be widely applied in laboratory devices. The chapter also examines the details of alternative applications for non-Wolter systems in other areas of science, where some of these systems have already demonstrated their advantages such as the K-B systems which have already found wide applications in laboratories and synchrotrons.
Czech name
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Czech description
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Classification
Type
C - Chapter in a specialist book
CEP classification
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OECD FORD branch
20201 - Electrical and electronic engineering
Result continuities
Project
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Continuities
R - Projekt Ramcoveho programu EK
Others
Publication year
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Book/collection name
Handbook of X-ray and Gamma-ray Astrophysics
ISBN
978-981-19-6960-7
Number of pages of the result
39
Pages from-to
137-175
Number of pages of the book
5000
Publisher name
Springer
Place of publication
Wien
UT code for WoS chapter
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