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排序方式: 共有682条查询结果,搜索用时 15 毫秒
81.
82.
根据空间平台拦截器与目标的相对运动方程,基于线性系统最优控制理论提出了一种综合三维极小脱靶量与极小能量的最优控制律。给出了最优推力大小与方向控制,以及最优过渡时间和关机时刻确定的模型。仿真结果表明:该最优控制律控制精度高,易于工程实现。 相似文献
83.
84.
应用理论分析与数值模拟方法,将对流传热的场协同原理从不可压缩流动推广至高超声速化学非平衡流动中。结果表明,高超声速化学非平衡层流与湍流的热流密度取决于流动的当地单位体积的动量与单位质量总焓梯度的协同。用当地单位体积的动量与单位质量总焓梯度的协同研究高超声速化学非平衡流动的壁面传热问题,对层流流动下的对流传热,不但计及了高超声速化学非平衡流的密度变化对热流密度的影响,而且包括了静焓梯度、压力梯度、边界层内的分子黏性剪切效应对热流密度的作用;对湍流问题,除了上述层流流动各项对热流密度的影响外,还计及了雷诺剪切应力对热流密度的作用。考虑到高超声速化学非平衡流静焓的定义,高超声速化学非平衡层流及湍流的场协同同时计及所有组分的平动能、转动能、振动能及电子能等梯度的贡献。 相似文献
85.
考虑可压缩与热传导的壁面函数边界条件及其应用 总被引:4,自引:0,他引:4
考虑到可压缩和热传导效应的壁面函数边界条件,被耦合到了采用k-ω两方程湍流模型、用有限体积法求解N-S方程的程序中。壁面函数基于耦合的速度和温度型,并且在边界层内的粘性子区和对数区内一致有效。引入壁面函数边界条件后,通过算例验证在y <100的范围内,得到的物面压力、摩阻、热流与实验结果比较,结果可靠。而无壁面函数边界条件时,要得到相同精度的结果,要求y ≈1。壁面函数的引入,为工程上准确预测飞行器在湍流流动中表面受力与气动热提供了保障。 相似文献
86.
In order to apply the air fin successfully and ensure the maneuverability of hypersonic vehicle, a key problem to be studied urgently is the heat flux brought by the fin mounting gap. The appearance of mounting gap and fin shaft can induce many complex flow structures which need more attentions to be investigated. Under Ma 6, Nano-tracer-based Planar Laser Scattering (NPLS) and Temperature Sensitive Paints (TSP) were applied to visualize and measure transient flow structures and heat flux distribution of a swept fin-induced flow field with different height mounting gaps. Complementarily, Reynolds-averaged N-S equations were solved with k-ω SST turbulent model. The heat flux distribution results of numerical simulation and TSP observed the change of high heat flux region with different mounting gap, both in position and magnitude. The streamlines based on Computational Fluid Dynamics (CFD) and flow visualization results obtained by NPLS revealed the cause of high heat flux region. The high heat flux region in this flow field is mainly related to the reattachment of vortex and flow stagnation. The increase of gap height can lead to stronger gap overflow and shaft-induced horseshoe vortex, which are source of the high heat flux around the fin. The case with the highest mounting gap (4 mm) en-counters the most severe aerodynamic heating, both on the surface of fin and plate. Thus, under the premise of ensuring the flexibility of the fin, the gap should be set as small as possible. 相似文献
87.
Zero mass flux jets, synthesized by acoustic actuators, have been used for the purpose of jet mixing enhancement and jet vectoring. Zero mass flux jets composed of entirely entrained fluid allow momentum transfer into the embedding flow. In the present experiments, miniature-scale high aspect ratio actuator jets are placed along the long sides and near the exit plane of a primary two-dimensional jet. In different modes, the primary jet can be vectored either towards or away from the actuator jets and the jet mixing is enhanced. The disturbance of the excitation frequency is developed while the unstable frequency of the primary jet is completely suppressed. 相似文献
88.
89.
为了使新疆和田地区夏季在经济性合理前提下使室内通风环境满足人体热舒适要求。利用蒸发冷却技术将室外空气处理后送入室内,通过数值模拟分析得出在夏季室内负荷最大时刻采用机械辅助式自然通风,使得室温能够雏持在26-8℃,风速为0.6m/s,基本满足人体热舒适要求。在室外温度适宜的过渡季节采用Trombe墙和太阳能烟囱复合的自然通风系统,建筑太阳能烟囱的经济高度为10m。 相似文献
90.
Panagiotis K. Marhavilas 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
The analysis of energetic particles and magnetic field measurements from the Ulysses spacecraft has shown that in a series of events, the energy density contained in the suprathermal tail particle distribution is comparable to or larger than that of the magnetic field, creating conditions of high-beta plasma. In this work we analyze periods of high-beta suprathermal plasma occurrences (βep > 1) in interplanetary space, using the ratio (βep) of the energetic particle (20 keV to ∼5 MeV) and magnetic field energy densities from measurements covering the entire Ulysses mission lifetime (1990–2009) in order to reveal new or to reconfirm some recently defined interesting characteristics. The main key-results of the work are summarized as follows: (i) we verify that high-beta events are detected within well identified regions corresponding mainly to the vicinity of shock surfaces and magnetic structures, and associated with energetic particle intensity enhancements due to (a) reacceleration at shock-fronts and (b) unusually large magnetic field depressions. (ii) We define three considerable features for the high-beta events, concentrated on the next points: (a) there is an appreciable solar-activity influence on the high-beta events, during the maximum and middle solar-cycle phase, (b) the annual peak magnitude and the number of occurrences of high events are well correlated with the sunspot number, (c) the high-beta suprathermal plasma events present a spatial distribution in heliographic latitudes (HL) up to ∼±80°, and a specific important concentration on the low (−25° ? HL < −6°, 6° < HL ? 25°) and median (−45° ? HL < −25°, 25° < HL ? 45°) latitudes. We also reconfirm by a statistical analysis the results of Marhavilas and Sarris (2011), that the high-beta suprathermal plasma (βep > 1) events are characterized by a very large parameter βep (up to 1732.5), a great total duration (406 days) and a large percentage of the Ulysses-mission lifetime (which is equal to 6.34% of the total duration with usable measurements, and 11.3% of the duration in presence of suprathermal particles events). 相似文献