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Risa Nagura Yuki Watanabe Naoto Sato Shujiro Komiya Shinya Suzuki Kentaro Katano Hayato Minami Kosuke Noborio 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):589-597
A plant growth system for crop production under microgravity is part of a life supporting system designed for long-duration space missions. A plant growth in soil in space requires the understanding of water movement in soil void spaces under microgravity. Under 1G-force condition, on earth, water movement in porous media is driven by gradients of matric and gravitational potentials. Under microgravity condition, water movement in porous media is supposed to be driven only by a matric potential gradient, but it is still not well understood. We hypothesized that under microgravity water in void spaces of porous media hardly moved comparing in void spaces without obstacles because the concave surfaces of the porous media hindered water movement. The objective of this study was to investigate water movement on the convex surfaces of porous media under microgravity. We conducted parabolic flight experiments that provided 20–25?s of microgravity at the top of a parabolic flight. We observed water movement in void spaces in soil-like porous media made by glass beads and glass spheres (round-bottomed glass flasks) in the different conditions of water injection under microgravity. Without water injection, water did not move much in neither glass beads nor glass spheres. When water was injected during microgravity, water accumulated in contacts between the particles, and the water made thick fluid films on the particles surface. When the water injection was stopped under microgravity, water was held in the contacts between the particles. This study showed that water did not move upward in the void spaces with or without the water injection. In addition, our results suggested that the difficulty of water movement on the convex (i.e. particle surfaces) might result in slower water move in porous media under microgravity than at 1G-force. 相似文献
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为了深入理解分层旋流流场特征和燃烧稳定性,采用OpenFOAM对分层旋流燃烧器的冷态和燃烧流场进行了大涡模拟。研究了旋流数对分层旋流流场结构和非稳态特性的影响。采用Q准则显示了流场中的瞬时涡结构;利用功率谱分析了流场中的进动特征。结果表明:在冷态工况下,旋流对回流区的位置和大小影响较小。随着旋流数增大,出口气流受到旋流诱导的离心作用,流动发散,流场扩张角变大,流场下游出现二次回流区。平均流场的三维流线与螺旋涡在空间中均表现成正交关系,表明螺旋涡是由剪切层Kelvin-Helmholtz不稳定性产生。在燃烧工况下,随着旋流数增大,回流区的面积增大,平均温度分布不断沿径向扩张,火焰锋面脉动增强,涡旋发生破碎的位置明显向上游移动。 相似文献
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为拓宽大弯角扩压叶栅可用攻角范围,优化叶片吸力面流动分离结构,本文以一大弯角叶栅为研究对象,对叶片采用压力面到吸力面打通的双“C”型槽道结构处理,在保持槽道长度及其他参数不变的条件下,设置85%、80%、75%、70%轴向弦长四个出口位置研究槽道出口位置对叶栅性能的影响。研究发现,特定攻角下,槽道出口位于吸力面角区分离线起始点之后、尾缘分离线之前,对吸力面流动分离的控制效果较佳;在全攻角范围,槽道出口则取在0o攻角对应较佳出口位置为好。为减小槽道内总压损失,本文提出了一种“SC”型槽道改进结构,在80%轴向弦长槽道出口位置处与双“C”型槽道以及原型叶栅进行对比。结果表明,“SC”型槽道结构相比于双“C”型槽道结构,叶栅尾迹损失及槽道内总压损失减少,槽道出口射流速度提高,叶片尾缘处静压升高;相比于原型叶栅则能有效降低其在全攻角范围内的总压损失,基本消除叶片吸力面附面层分离,削弱角区分离,提高叶栅的扩压能力。 相似文献
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《中国航空学报》2021,34(4):306-319
A nonlinear dynamic modeling method for primary mirror of Flower-like Deployable Space Telescope (F-DST) undergoing large deployment motion is proposed in this paper. To ensure pointing accuracy and attitude stability of the paraboloidal primary mirror, the mirror is discretized into equal thickness shell elements by considering shell curvature. And the material nonlinear constitutive relation of flexible mirror is acquired using Absolute Nodal Coordinate Formulation (ANCF). Furthermore, the primary mirror of F-DST can be regarded as a clustered multi-body system, and its dynamic equations of elastic deformation and deployment motion are established by virtual work principle. Finally, the deployment motion of primary mirror by different driving conditions are simulated, the results show that the vibrations of mirrors that driven by elastic hinge device are more than that driven by servo motor. In addition, single sub-mirror deployment process will perturb the pointing accuracy of primary mirror, and the multiple sub-mirrors simultaneously deploying will seriously affect all the sub-mirrors surface accuracy because of the coupling effect. Thus, there are theoretical value and practical significance for the controlling surface accuracy and attitude accuracy of space telescope. 相似文献
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The carrier synchronization algorithm of the autonomous radio for deep space is studied. When the signal modulation is unknown, this paper improves the existing universal carrier synchronization loop for multiple modulations, expands the frequency tracking range of the loop, proposes a Tong detection-based M-ary Phase Shift Keying (M-PSK) signal locking detection algorithm to rapidly and effectively determine whether the current phase discrimination mode matches the modulation mode, so as to independently choose whether to switch the phase discrimination mode. Through theoretical analysis and comparison, it is described that the total detection probability of the algorithm proposed in this paper is significantly higher than the probability of single lock detection. Simulation results show that the algorithm has high detection probability and low computational complexity at a low signal to noise ratio. 相似文献