Abstract
Silicon Pore Optics (SPO) uses commercially available monocrystalline double-sided super-polished silicon wafers as a basis to produce mirrors that form lightweight high-resolution X-ray optics. The technology has been invented by cosine measurement systems and the European Space Agency (ESA) and developed together with scientific and industrial partners to mass production levels. It leverages techniques and processes developed over decades by the semiconductor industry to handle, process, and clean silicon wafers and plates. SPO is an enabling technology for large spaceborne X-ray telescopes such as Athena and ARCUS, operating in the 0.2–12 keV band, with angular resolution aiming for 5 arcsec. SPO has also shown to be a versatile technology that can be further developed for gamma-ray optics, medical applications, and material research.
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Barrière, N.M. et al. (2022). Silicon Pore Optics. In: Bambi, C., Santangelo, A. (eds) Handbook of X-ray and Gamma-ray Astrophysics. Springer, Singapore. https://doi.org/10.1007/978-981-16-4544-0_5-1
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