Optics for EUV, X-Ray, and Gamma-Ray Astronomy IX 2019
DOI: 10.1117/12.2530696
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Status of the silicon pore optics technology

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Cited by 17 publications
(11 citation statements)
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“…The Advanced Telescope for High ENergy Astrophysics (Athena) telescope is selected as the next large class X-ray observatory of the European Space Agency (ESA) 1 . The mission will feature a single X-ray telescope with a focal length of 12 m and a mirror design based on the silicon pore optics (SPO) technology [2][3][4] . Achieving the science cases for Athena requires excellent X-ray reflective mirror coatings.…”
Section: Introductionmentioning
confidence: 99%
“…The Advanced Telescope for High ENergy Astrophysics (Athena) telescope is selected as the next large class X-ray observatory of the European Space Agency (ESA) 1 . The mission will feature a single X-ray telescope with a focal length of 12 m and a mirror design based on the silicon pore optics (SPO) technology [2][3][4] . Achieving the science cases for Athena requires excellent X-ray reflective mirror coatings.…”
Section: Introductionmentioning
confidence: 99%
“…Включение в интерфейс азота защищает от проникновения примесей, и радиационная стойкость диодов возрастает на несколько порядков. Однако, пассивирующее окно вызывает поверхностную рекомбинацию при получении большой дозы ионизирующего излучения, что приводит к снижению квантового выхода [12,13]. Результаты исследований стабиль-Метрологические исследования характеристик многослойных поверхностных покрытий с использованием синхротронного излучения ности фотодиодов с использованием синхротронного излучения электронных накопительных кольцах «Сибирь-1» и MLS показали, что при суммарной энерге-тической экспозиции 500 МДж/м 2 в течение нескольких часов изменение абсолютной спектральной чувствительности при нормировании сигнала фотодиода на ток электронного пучка не превышало десятых долей процента.…”
Section: Research Articleunclassified
“…This translates into about 300 m 2 of superpolished mirror surface and requires a new mirror technology to break the general correlation stated above, to make a light-weight yet stiff mirror, in order to achieve the desired optical performance. This technology is being developed by ESA [5], cosine and its partners, both in industry and academia and is called Silicon Pore Optics (SPO) [6].…”
Section: Introductionmentioning
confidence: 99%