TY - GEN
T1 - Novel ultra-lightweight and high-resolution MEMS X-ray optics
AU - Mitsuishi, Ikuyuki
AU - Ezoe, Yuichiro
AU - Takagi, Utako
AU - Mita, Makoto
AU - Riveros, Raul
AU - Yamaguchi, Hitomi
AU - Kato, Fumiki
AU - Sugiyama, Susumu
AU - Fujiwara, Kouzou
AU - Morishita, Kohei
AU - Nakajima, Kazuo
AU - Fujihira, Shinya
AU - Kanamori, Yoshiaki
AU - Yamasaki, Noriko Y.
AU - Mitsuda, Kazuhisa
AU - Maeda, Ryutaro
N1 - Copyright:
Copyright 2012 Elsevier B.V., All rights reserved.
PY - 2009
Y1 - 2009
N2 - We have been developing ultra light-weight X-ray optics using MEMS (Micro Electro Mechanical Systems) technologies.We utilized crystal planes after anisotropic wet etching of silicon (110) wafers as X-ray mirrors and succeeded in X-ray reflection and imaging. Since we can etch tiny pores in thin wafers, this type of optics can be the lightest X-ray telescope. However, because the crystal planes are alinged in certain directions, we must approximate ideal optical surfaces with flat planes, which limits angular resolution of the optics on the order of arcmin. In order to overcome this issue, we propose novel X-ray optics based on a combination of five recently developed MEMS technologies, namely silicon dry etching, X-ray LIGA, silicon hydrogen anneal, magnetic fluid assisted polishing and hot plastic deformation of silicon. In this paper, we describe this new method and report on our development of X-ray mirrors fabricated by these technologies and X-ray reflection experiments of two types of MEMS X-ray mirrors made of silicon and nickel. For the first time, X-ray reflections on these mirrors were detected in the angular response measurements. Compared to model calculations, surface roughness of the silicon and nickel mirrors were estimated to be 5 nm and 3 nm, respectively.
AB - We have been developing ultra light-weight X-ray optics using MEMS (Micro Electro Mechanical Systems) technologies.We utilized crystal planes after anisotropic wet etching of silicon (110) wafers as X-ray mirrors and succeeded in X-ray reflection and imaging. Since we can etch tiny pores in thin wafers, this type of optics can be the lightest X-ray telescope. However, because the crystal planes are alinged in certain directions, we must approximate ideal optical surfaces with flat planes, which limits angular resolution of the optics on the order of arcmin. In order to overcome this issue, we propose novel X-ray optics based on a combination of five recently developed MEMS technologies, namely silicon dry etching, X-ray LIGA, silicon hydrogen anneal, magnetic fluid assisted polishing and hot plastic deformation of silicon. In this paper, we describe this new method and report on our development of X-ray mirrors fabricated by these technologies and X-ray reflection experiments of two types of MEMS X-ray mirrors made of silicon and nickel. For the first time, X-ray reflections on these mirrors were detected in the angular response measurements. Compared to model calculations, surface roughness of the silicon and nickel mirrors were estimated to be 5 nm and 3 nm, respectively.
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U2 - 10.1117/12.823933
DO - 10.1117/12.823933
M3 - Conference contribution
AN - SCOPUS:69949115915
SN - 9780819476340
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - EUV and X-Ray Optics
T2 - EUV and X-Ray Optics: Synergy between Laboratory and Space
Y2 - 20 April 2009 through 22 April 2009
ER -