塞式喷管底部二次流的数值模拟研究

从 N-S方程出发 ,采用二阶精度的 NND格式对塞式喷管的流场进行了数值模拟 ,重点研究了一线性塞式喷管底部二次流在低中高空的特性。研究表明 ,塞式喷管底部回流区的消失不仅与二次流流量大小有关 ,而且与底部压强有关 ;加入二次流会使塞式喷管的推力上升 ,但在大多数情况下其比冲会下降 ,只有特定压强比条件下 ,加入少量的二次流比冲才会上升     

小功率电弧喷射发动机的数值计算

为详细了解电弧喷射发动机内部工作过程和相关工作参数对其性能的影响，参照实验用发动机的工作参数建立了模型，数值模拟了电弧喷射发动机工作通道内流场和电磁场。利用NND格式求解耦合电磁源项N－S方程，Gauss-Seidel迭代加超松驰方法求解椭圆型电磁场方程，计算得到的发动机工作通道内流场、电磁场结构，与实验数据进行了对比。结果表明，对同一结构尺寸的发动机，随推进剂流量变化，发动机性能存在最佳值；在一定流量范围内，实验数据和计算结果相符。     

用非结构直角网格和欧拉方程计算飞机绕流

 采用八叉树结构 ,生成复杂外形绕流计算的非结构直角网格。物面附近用投影方法 ,使网格贴体。并将Jameson的有限体积法推广用于这种网格的欧拉方程计算。对歼击机模型的绕流计算表明 ,网格生成的机时花费很少 ,总体质量好 ,因而欧拉方程解算的收敛质量也好。     

飞机在有源干扰保护下的探测概率研究

研究了飞机与雷达探测系统遭遇时，雷达对飞机的探测概率随距离的变化问题，采用X^2类目标波动模型，针对飞机在有源干扰保护的情况对探测概率随距离的变化进行了研究，对不同RCS对探测概率的影响问题进行了分析，研究结果可为飞机的雷达探测敏感性评估，飞机生存力的定量化分析与权衡，以及雷达探测系统的效能评估提供量化依据。     

旋转机翼悬停气动特性研究

鸭式旋转机翼(CRW)是一种先进的高速直升机方案,旋翼同时也是机翼,是其最关键气动部件之一。采用结构分区拼接网格技术进行空间离散,分区建立参考系,通过求解多重参考系下的N-S方程来计算旋翼流场,首先以传统的Caradonna-Tung实验旋翼的亚、跨声速悬停流场分析为例验证该方法的可靠性,进而采用该方法对旋转机翼悬停流场进行了数值计算,旋翼拉力计算值和地面实验值吻合较好,结果分析表明旋转机翼的悬停流场有着不同于传统旋翼的流场特性。     

用非结构直角网格和欧拉方程计算运载火箭绕流

采用八叉树结构，物面附近用投影法，生成运载火箭绕流计算的非结构直角网格。并将Jameson的有限体积法推广用于这种网格的欧拉方程计算。算例表明，网格生成的时机化费很少，质量好；欧拉方程解算的收敛质量也好。     

Tolerance of wheat and lettuce plants grown on human mineralized waste to high temperature stress

The main objective of a life support system for space missions is to supply a crew with food, water and oxygen, and to eliminate their wastes. The ultimate goal is to achieve the highest degree of closure of the system using controlled processes offering a high level of reliability and flexibility. Enhancement of closure of a biological life support system (BLSS) that includes plants relies on increased regeneration of plant waste, and utilization of solid and liquid human wastes. Clearly, the robustness of a BLSS subjected to stress will be substantially determined by the robustness of the plant components of the phototrophic unit. The aim of the present work was to estimate the heat resistance of two plants (wheat and lettuce) grown on human wastes. Human exometabolites mineralized by hydrogen peroxide in an electromagnetic field were used to make a nutrient solution for the plants. We looked for a possible increase in the heat tolerance of the wheat plants using changes in photosynthetically active radiation (PAR) intensity during heat stress. At age 15 days, plants were subjected to a rise in air temperature (from 23 ± 1 °C to 44 ± 1 °С) under different PAR intensities for 4 h. The status of the photosynthetic apparatus of the plants was assessed by external СО₂ gas exchange and fluorescence measurements. The increased irradiance of the plants during the high temperature period demonstrated its protective action for both the photosynthetic apparatus of the leaves and subsequent plant growth and development. The productivity of the plants subjected to temperature changes at 250 W m⁻² of PAR did not differ from that of controls, whereas the productivity of the plants subjected to the same heat stress but in darkness was halved.     

Motion of deformable planets and stability of their stationary rotations

A mechanical system consisting from N deformable spheres interacting according to the law of gravity is considered as a model of planetary system. Deformations of the viscoelastic spheres are described according to the model of the theory of elasticity of small deformations, the Kelvin-Voigt model of viscous forces, and occur under the action of gravitational fields and fields of centrifugal forces. Approximate equations describing motions of the centers of mass of the spheres and their rotations relative to the centers of mass are constructed by the method of separation of motions on the basis of solving quasistatic problems of the theory of viscoelasticity with allowance made for smallness of sphere deformations. Using the first integral of conservation of the angular momentum of the system relative to its center of mass, the expression for the changed potential energy is obtained with the use of the Routh method. An investigation of stationary rotations is carried out, and it is shown that all of them are unstable, if the number of planets is more than two.     

Motion of three viscoelastic planets in the field of their mutual attraction forces

Translational-rotational motion of three planets modeled by viscoelastic balls in the gravitational field of mutual attraction is studied in this paper. The system of equations of motion for the mechanical system under consideration is deduced from the d’Alembert-Lagrange variational principle. Using the method of separation of motions, an approximate system of ordinary differential equations, describing the translational-rotational motion of the planets, is obtained with taking into account perturbations caused by elasticity and dissipation. The found steady-state motion of the system is an analog to triangular libration points in the classical three-body problem.     

任意二维物体捕捉自由涡的驻定态稳定性分析

证明了任意二维物体能捕捉到的驻定态自由涡最多只有中性稳定性；物表面用抽无助于稳定性。如果有一点源能与自由涡相联，有可能使驻定态自由涡达到真正稳定。