706 硬X線望遠鏡用ミラーフォイルの振動特性
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概要
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In the present paper, vibration properties of mirror foils installed in a hard X-ray telescope (HXT) on-board a satellite were investigated. Vibration tests and FEM analysis of mirror foils installed in the part model of HXT were conducted. From the experimental results, it appeared that the mirror had resonant frequencies at 64, 73 and 11 OHz. The modal shapes of 64 and 73Hz showed that the maximum amplitude appeared at edges of the foil. On the other hand, vibration amplitude became maximum at the center in the modal shape of 11 OHz. Experimental results of frequency responses of these modes agreed well with analytical results except around 64Hz. It is considered that the resonant mode of 64Hz was strongly affected by nonlinear characteristics of friction constraint between the foils and HXT housing.
- 2011-09-05
著者
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国枝 秀世
名大 理
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国枝 秀世
Department Of Astrophysics Nagoya University
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KODAIRA Hironobu
Dept. of Physics, Kanazawa University
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Kosugi Hiroko
Kyoto Univ. Kyoto
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KUDO Hiroyuki
Waseda University
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宮澤 拓也
名大
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粟木 久光
愛媛大
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黄木 景二
愛媛大
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古澤 彰浩
名大
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前田 良知
JAXA
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石田 学
JAXA
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吉村 昂泰
高知工大
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高坂 達郎
高知工大
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山根 伸幸
名大
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加藤 大佳
名大
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国枝 秀世
名大
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