排序方式: 共有54条查询结果,搜索用时 15 毫秒
51.
CO_2对CO加氢制甲醇有着很大影响。当CO_2含量少(约3%以下)时,可促进CO加氢,超出此限度后,即阻碍作用,这效应并不与CO_2的绝对分压有关,只要CO/CO_2恒定,这个作用就得以显露,即使总压低至常压附近也是这样。但常压下,于通常反应温度间出现随温度升高,甲醇产率下降的现象,这可能与生成甲醇的选择性减少有关,故采用在较低温度下(200℃)予以评价。反应压力大范围变动时的这个特性对弄清 Cu/ZnO 催化剂是否存在两种不同的活性中心会有所帮助。 相似文献
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提出了一种新的进化计算策略,综合了信息论测度与最优决策过程,提出并证明了该计算体系的有关性质和定理.该进化计算策略有助于非线性系统的自适应辩识和预测,具有较为广泛的应用前景. 相似文献
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Antoci V Handler G Campante TL Thygesen AO Moya A Kallinger T Stello D Grigahcène A Kjeldsen H Bedding TR Lüftinger T Christensen-Dalsgaard J Catanzaro G Frasca A De Cat P Uytterhoeven K Bruntt H Houdek G Kurtz DW Lenz P Kaiser A Van Cleve J Allen C Clarke BD 《Nature》2011,477(7366):570-573
Delta Scuti (δSct) stars are opacity-driven pulsators with masses of 1.5-2.5 M⊙, their pulsations resulting from the varying ionization of helium. In less massive stars such as the Sun, convection transports mass and energy through the outer 30 per cent of the star and excites a rich spectrum of resonant acoustic modes. Based on the solar example, with no firm theoretical basis, models predict that the convective envelope in δSct stars extends only about 1 per cent of the radius, but with sufficient energy to excite solar-like oscillations. This was not observed before the Kepler mission, so the presence of a convective envelope in the models has been questioned. Here we report the detection of solar-like oscillations in the δSct star HD187547, implying that surface convection operates efficiently in stars about twice as massive as the Sun, as the ad hoc models predicted. 相似文献
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