喷管流场和羽流场的N－S数值模拟

利用时间推进的方法，通过求解可压缩的、雷诺平均的Ｎ－Ｓ方程，并利用Ｂａｌｄｗｉｎ－Ｌｏｍａｘ两层代数滴流模型和Ｐｒａｎｄｔｌ混合长度模型，数值模拟了飞机和火箭发动机喷管的内流和羽流，获得了喷管内流场和羽流场的参数分布，计算结果与试验结果及国外研究成果一致。网格划分采和了自适应网格技术。     

热空腔-喷气流的组合辐射

讨论了热空腔(喷气发动机的加力筒)和喷气流的组合辐射问题, 推演了组合辐射的辐射传输微分方程, 导出了有边界辐射条件下的解。讨论了由多个温度不同的壁面组成且腔内充满高温燃气的热空腔辐射传输方程解的具体形式, 导出了它向后半球的光谱辐射强度的表达式;同时还推导了热空腔-喷气流组合辐射的光谱辐射强度的表达式。最后给出算例, 算例结果表明, 热空腔-喷气流组合辐射的空间分布具有与实测分布较一致的梨形包络, 其光谱分布也与实测的光谱分布的一致性较好。      

飞行器再入机动制导的一种新方法

基于飞行力学的原理，建立了飞行器攻击地面目标的运动方程，进而运用计算结构力学与最优控制的相似性原理，将求解Ｒｉｃｃａｔｉ方程的一种新方法引入飞行器再入机动制导问题中。由于采用的是结构静力学中的子结构消元法，从而避免了本征值问题的求解。该方法大幅度地提高了计算速度，同时具有很好的数值稳定性，计算结果表明该方法的有效性。     

非结构网格下Euler方程的高分辨率高精度解

提出了一种非结构网格下求解Ｅｕｌｅｒ方程的高分辨率高精度迎风格式。以Ｒｏｅ的矢通量差分分裂为基础,吸收了ＮＮＤ格式的优点,使其具有捕捉激波和滑移线的良好性能;在时间方向上采用Ｊａｍｅｓｏｎ的Ｒｕｎｇｅ－Ｋｕｔａ积分,并结合局部最大时间步长和残差光滑技术加速收敛。最后成功地完成了二维平板激波反射、跨音速Ｌａｖａｌ喷管内的流动和ＧＡＭＭ超音速前台阶绕流等算例,显示了该方法的有效性     

真空羽流场的 N-S 和 DSMC 耦合数值模拟

根据调姿发动机真空羽流场的特点,采用差分求解Ｎ－Ｓ方程数值模拟喷管内流场,用ＤＳＭＣ方法数值模拟喷管外羽流场,得到了符合流动规律的数值模拟结果。为姿控发动机喷管设计提供了参考,并为真空羽流污染研究打下了良好的基础。     

带副翼三维机翼绕流的Euler方程解

提出了一种求解带副翼偏转三维机翼绕的Ｅｕｌｅｒ方程计算方法。采用对接分区网格民分区求解算法的结合,有铲地求解绕引外形的复杂流动,提出了一种满足通量守恒的内边界耦吉选用ＶａｎＬｅｅｒ分裂格式离散玩粘通量项,并构造了一种Ｌｉｍｉｔｅｒ函数以保证ＴＶＤ性质。数值算例表明本方法是求解带操纵纵面偏转的机翼绕流的有效方法。     

Relationship Between Substorm Auroras and Processes in the Near-Earth Magnetotail

Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for monitoring of substorm intensity in terms of the magnetic flux and energy dissipation.     

Geoeffectivity of Coronal Mass Ejections

Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity, magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour high-latitude activity.     

Hamilton正则方程半解析法的收敛和对称分析

近年来,Hamilton正则方程半解析法在工程问题上的应用越来越广泛,但至今未见有关这种方法收敛性和对称性问题研究的文献。基于Hamilton正则方程的半解析法理论,通过变分原理详细推导了Hamiltonian元素的固支和简支边界公式及对称边界公式。多个实例的数值研究表明：随着网格加密,Hamilton正则方程半解析法的收敛速度快于一般传统位移有限元法,对称解法的效率明显优于整体解法。     

高温超导磁悬浮助推缩比试验系统动态测试分析

基于磁悬浮助推技术概念研究方案建立了一套悬浮加速缩比试验系统.从整体缩比模型振动试验出发,主要研究悬浮质量以及悬浮刚度对整体系统动态性能的影响,并在进行缩比单元动态试验结论的基础上,建立试验模型的加速试验动态采集系统,对整体模型进行运行性能试验.在试验基础上提出了提高磁悬浮推进系统运行稳定性的依据,并据此提出相应可行的解决方案设想.通过模型加速试验并采集试验数据定性分析磁浮系统的综合运动性能,以更好地评估系统稳定特性和品质,也为进一步研究磁悬浮助推发射的气动、分离系统稳定性和可靠性提供参考.