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7篇 您的检索式:作者名="S.Hayashi"
    题名 作者 年代 出处 被引量
1氢化丁腈橡胶(HNBR)的低温性能显示文摘前言氢化丁腈橡胶(HNBR)是通过丁腈橡胶(NBR)的氢化而制成的一种耐热、耐油及耐燃油类的弹性体。如表1所示,HNBR是一种高饱和丁腈橡胶,由丙烯腈、乙烯、不饱和丁二烯及氢化乙烯基丁二烯等单体合成。S.Hayashi 候元斌 1998橡胶参考资料1998,28,11:5
2APPLICATION OF THE UNIFIED STATISTICAL MATERIAL DATABASE FOR DESIGN AND LIFE/RISK ASSESSMENT OF HIGH TEMPERATURE COMPONENTS显示文摘Statistical manipulation of material data was conducted for probabilistic life assessment or risk-based design and maintenance for high temperature components of power plants. To obtain the statistical distribution of material properties, dominant parameters affecting material properties are introduced into normalization of statistical variables. Those parameters are hardness, chemical composition, characteristic microstructural features and so on. Creep and fatigue properties are expressed by normalized parameters and the unified statistical distributions are obtained. These probability distribution functions show good coincidence statistically with the field database of steam turbine components. It was concluded that the unified statistical baseline approach is useful for the risk management of components in power plants.K.Fujiyama T.Fujiwara Y.Nakatani K.Saito A.Sakuma Y.Akikuni S.Hayashi S.Matsumoto 2004Acta Metallurgica Sinica(English Letters)2004,17,4:1
3A Stable and Highly Active Hybrid Mesoporous Solid Acid Catalyst显示文摘K.Nakajima I.Tomita M.Hara S.Hayashi K.Domen J.?N.Kondo 2005Adv Mater2005,,15:1
4氢化丁腈橡胶(HNBR)的低温性能显示文摘1、前言氢化丁腈橡胶(HNBR)是通过丁腈橡胶(NBR)的氢化而制成的一种耐热、耐油及耐燃油类的弹性体。如表1所示,HNBR是一种高饱和丁腈橡胶,由丙烯腈、乙烯、不饱和丁二烯及氢化乙烯基丁二烯等单体合成。丙烯腈单体赋予NBR以优异的耐油、耐燃油性及高的拉伸强度;S.Hayashi 郭宏盛 1992橡胶参考资料1992,,2:0
5Effect of Water Vapor on the Oxidation of Pt-modified Ni-22Al Alloys显示文摘Cyclic oxidation behavior of two-phaseγ+γ'-Ni-22Al-5 and -10 Pt alloys in air with and without 30 vol.%H_2O at 1000℃was investigated.The oxidation of 5 and 10 Pt alloys in air was initially rapid and followed by a slow steady-state stage.The oxidation during this steady-state stage was followed the parabolic rate law,and the parabolic rate constants for the two different Pt content alloys were similar.However the mass change of 5 Pt alloy during the initial rapid oxidation stage was much higher than that of 10 Pt,and it resulted in higher oxidation mass gain on 5 Pt alloy after 500 cycles.Similar oxidation behavior,initial rapid followed by slow steady-state,was observed when the alloys were oxidized in air+30%H_2O,however the initial oxidation mass change in the wet atmosphere was much higher for both alloys than in air.Interestingly,the oxidation rate constants for both alloys during the steady-state stage significantly decreased in the atmosphere with water vapor.Particularly,oxidation mass gain on the 5 Pt alloy was not observed after about 100 cycles of oxidation.S.HAYASHI M.AUCHI T.NARITA B.GLEESON 2009中国腐蚀与防护学报2009,29,4:0
6猪胚胎冷冻移植成功显示文摘将哺乳类动物的胚胎冷冻保存在液氮中的试验已经在一些动物成功,如小鼠(Whit-tingham等,1972),牛(Wilmut和Rowson,1973)、绵羊(Willadsen等,1976)、山羊(Bilton和Moor,1976)和马(Yamamoto等,1982)。牛的冷冻胚胎已经商业化生产。然而,猪胚胎的冷冻和解冻还未获得成功。据报道,猪的胚胎对于低温,即使是+10℃(Wil-mut,1972;Niemann,1985)都极敏感。本研究是检验由桑葚胚到孵出期囊胚各胚龄猪胚胎冷冻-解冻后能否存活。采用有性周期的8~24个月龄。S.Hayashi 朱捷 1989国外畜牧科技1989,16,6:0
7Near-infrared polarimetry of the GG Tauri A binary system显示文摘A high angular resolution near-infrared image that shows the intensity of polarization for the GG Tau A binary system was obtained with the Subaru Telescope.The image shows a circumbinary disk scattering the light from the central binary. The azimuthal profile of the intensity of polarization for the circumbinary disk is roughly reproduced by a simple disk model with the Henyey-Greenstein phase function and the Rayleigh function, indicating there are small dust grains at the surface of the disk.Combined with a previous observation of the circumbinary disk, our image indicates that the gap structure in the circumbinary disk orbits counterclockwise, but material in the disk orbits clockwise. We propose that there is a shadow caused by material located between the central binary and the circumbinary disk. The separations and position angles of the stellar components of the binary in the past 20 yr are consistent with the binary orbit with a = 33.4 AU and e = 0.34.Yoichi Itoh Yumiko Oasa Tomoyuki Kudo Nobuhiko Kusakabe Jun Hashimoto Lyu Abe Wolfgang Brandner Timothy D.Brandt Joseph C.Carson Sebastian Egner Markus Feldt Carol A.Grady Olivier Guyon Yutaka Hayano Masahiko Hayashi Saeko S.Hayashi Thomas Henning Klaus W.Hodapp Miki Ishii Masanori Iye Markus Janson Ryo Kandori Gillian R.Knapp Masayuki Kuzuhara Jungmi Kwon Taro Matsuo Michael W.McElwain Shoken Miyama Jun-Ichi Morino Amaya Moro-Martin Tetsuo Nishimura Tae-Soo Pyo Eugene Serabyn Takuya Suenaga Hiroshi Suto Ryuji Suzuki Yasuhiro H.Takahashi Naruhisa Takato Hiroshi Terada Christian Thalmann Daigo Tomono Edwin L.Turner Makoto Watanabe John Wisniewski Toru Yamada Satoshi Mayama Thayne Currie Hideki Takami Tomonori Usuda Motohide Tamura 2014Research in Astronomy and Astrophysics2014,14,11:0
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