Experimental investigations on hull-fin interferences of the LOTTE airship

In the present paper experimental aerodynamic investigations on an airship configuration at angle of attack with special emphasis on the hull-fin region are reported. In particular, visualizations of flow phenomena on both hull and fins are studied. Quantitative measurements of the integral force and moment characteristics as well as local pressure coefficients serve to establish a data pool for code validation.     

三维接触问题的接触状态有限元解法及应用

在文献［１］的基础上论述了有摩擦、有间隙的三维弹性接触问题接触状态有限元解法，并通过理论考题进行了验证。最后，在应用部分对汽轮机汽缸法兰连接汽密性进行了计算。     

基于电子束电离的高超声速磁流体发电机

为了获得高超声速低温来流条件下基于电子束电离的磁流体发电机性能,采用三维低磁雷诺数磁流体动力学五方程模型和简化的电子束电离模型,对等截面分段法拉第型磁流体发电机内的流动进行数值模拟,研究了电离能量花费、磁场强度对发电通道性能的影响,得出了不同电离花费下电离所形成的电子数密度和电导率.研究结果表明,电子束电离低温来流能够产生足够的电导率,当负载系数保持为0.5时,电效率基本保持在0.5 ～0.6之间,电效率大小受磁场强度影响不大,电离能量花费Pion(MW/m3)为0.06,0.6,6,30,300时的电导率σ(S/m)分别为0.28,0.9,3,7,27.当电离能量花费为30MW/m3,能量提取率达到26％,电效率为66％,发电机性能接近最佳,对应的磁场强度为10T.     

流向磁场作用下二维磁流体槽道湍流直接模拟

对低磁雷诺数近似下流向磁场作用的二维磁流体槽道湍流进行了直接数值模拟(DNS,Direct Numerical Simulation),给出了 Re=10 000时不同磁相互作用数下二维磁流体槽道湍流的近壁速度分布、湍流脉动速度均方根、雷诺应力等统计量的变化,并与中性流体二维槽道湍流进行了比较.结果表明:流向磁场作用会导致对数区上移;雷诺应力最大值随磁相互作用数呈线性变化;随着磁相互作用数的增大,下壁面平均涡量的时间演化由拟周期性向周期性转变,且脉动周期逐渐增大并当流动层流化后下壁面平均涡量成为常值.      

磁流体管流准一维模型的数值验证与性能分析

为了快速分析磁流体管流,采用涡轮喷气发动机模型对磁流体管流进行类比分析,引入变截面管流理论和修改过的多变效率表达式,推导了磁流体发电器和加速器的准一维模型,采用二维数值方法验证了准一维模型的可行性,利用该准一维模型对磁流体管流进行了性能分析,结果表明,多变效率的引入使准一维模型更加完整,当负载系数不变时,磁流体装置中的平均马赫数越低,其等熵效率越高。     

一类TVD型组合差分方法及其在磁流体数值计算中的应用

根据太阳风数值模拟的特点，考虑到算法的质量（收敛速度、稳定性、精度等），结合磁流体数值计算的特性，对三维球坐标磁流体动力学（MHD）方程组中的流体部分采用一种修正Lax-Friedrichs差分法而对磁场部分采用MacComack格式，发展了一类快捷的具有TVD特性的组合数值新方法，作为格式的检验，在一维情况下，将其与PPM格式进行了比较，对一维快慢磁流体激波问题得到了与PPM格式精度相同的结果，然后将其诮到定态太阳风的数值模拟上，在不同等离子体β情形下，可得到理想的太阳风定态结构，为今后将此数值模式应用到具有复杂磁场位型或三维直实太阳风暴的数值模拟研究奠定了基础。     

Optimal diving maneuver strategy considering guidance accuracy for hypersonic vehicle

An optimal maneuver strategy considering terminal guidance accuracy for hypersonic vehicle in dive phase is investigated in this paper. First, it derives the complete three-dimensional nonlinear coupled motion equation without any approximations based on diving relative motion relationship directly, and converts it into linear decoupled state space equation with the same relative degree by feedback linearization. Second, the diving guidance law is designed based on the decoupled equation to meet the terminal impact point and falling angle constraints. In order to further improve the interception capability, it constructs maneuver control model through adding maneuver control item to the guidance law. Then, an integrated performance index consisting of maximum line-of-sight angle rate and minimum energy consumption is designed, and optimal control is employed to obtain optimal maneuver strategy when the encounter time is determined and undetermined, respectively. Furthermore, the performance index and suboptimal strategy are reconstructed to deal with the control capability constraint and the serous influence on terminal guidance accuracy caused by maneuvering flight. Finally, the approach is tested using the Common Aero Vehicle-H model. Simulation results demonstrate that the proposed strategy can achieve high precision guidance and effective maneuver at the same time, and the indices are also optimized.     

Splitting Based Scheme for Three-dimensional MHD with Dual Time Stepping

A new hybrid numerical scheme of combining an E-CUSP (Energy-Convective Upwind and Split Pressure) method for the fluid part and the Constrained Transport (CT) for the magnetic induction part is proposed. In order to avoid the occurrence of negative pressure in the reconstructed profiles and its updated value, a positivity preserving method is provided. Furthermore, the MHD equations are solved at each physical time step by advancing in pseudo time. The use of dual time stepping is beneficial in the computation since the use of dual time stepping allows the physical time step not to be limited by the corresponding values in the smallest cell and to be selected based on the numerical accuracy criterion. This newly established hybrid scheme combined with positivity preserving method and dual time technique has demonstrated the accurateness and robustness through numerical experiments of benchmark problems such as the 2D Orszag-Tang vortex problem and the 3D shock-cloud interaction problem.      

An analytical model of prominence dynamics

Solar prominences are magnetic structures incarcerating cool and dense gas in an otherwise hot solar corona. Prominences can be categorized as quiescent and active. Their origin and the presence of cool gas ($～{10}^4$?K) within the hot ($～{10}^6\text{K}$) solar corona remains poorly understood. The structure and dynamics of solar prominences was investigated in a large number of observational and theoretical (both analytical and numerical) studies. In this paper, an analytic model of quiescent solar prominence is developed and used to demonstrate that the prominence velocity increases exponentially, which means that some gas falls downward towards the solar surface, and that Alfvén waves are naturally present in the solar prominences. These theoretical predictions are consistent with the current observational data of solar quiescent prominences.