基于迹向控制量的编队星群相位控制

为了得到控制量与控制时机对相位改变的直观公式,基于Hill方程以及迹向控制的约束条件,定性分析共面绕飞编队中控制量、控制时机与编队卫星相位之间的关系,分析结果表明:当需要改变的相位角小于90°时,可实现最省燃料的控制;当需要改变的相位角大于90°时,可进行趋于最小控制量的控制;当在相对运动椭圆上下点实施控制时,相位无变化.     

三维Euler方程的自适应非结构网络计算

介绍一种三维自适应非结构网格的Euler方程求解技术。采用有限体积中心差分的格点格式对Euler方程进行空间离散,多步龙格-库塔时间推进,并采用当地时间步长、焓阻尼修正等加速收敛。采用Delaunay三角剖分技术生成三维流场的四面体网格。网格自适应技术中的网格局部加密也采用Delaunay三角剖分技术。最后用ONERAM6机翼的跨音速绕流计算说明本文方法的有效性。     

Modelling and observing Jovian electron propagation times in the inner heliosphere

The propagation of Jovian electrons in interplanetary space was modelled by solving the relevant transport equation numerically through the use of stochastic differential equations. This approach allows us to calculate, for the first time, the propagation time of Jovian electrons from the Jovian magnetosphere to Earth. Using observed quiet-time increases of electron intensities at Earth, we also derive values for this quantity. Comparing the modelled and observed propagation times we can gauge the magnitude of the transport parameters sufficiently to place a limit on the 6 MeV Jovian electron flux reaching Earth. We also investigate how the modelled propagation time, and corresponding Jovian electron flux, varies with the well-known ∼13 month periodicity in the magnetic connectivity of Earth and Jupiter. The results show that the Jovian electron intensity varies by a factor of ∼10 during this cycle of magnetic connectivity.     

The use of Gaussian equations of motions of a satellite for local gravity anomaly recovery

The orbital elements of a low Earth orbiting satellite and their velocities can be used for local determination of gravity anomaly. The important issue is to find direct relations among the anomalies and these parameters. Here, a primary theoretical study is presented for this purpose. The Gaussian equations of motion of a satellite are used to develop integral formulas for recovering the gravity anomalies. The behaviour of kernels of the integrals are investigated for a two-month simulated orbit similar to that of the Gravity field and steady-state ocean circulation explorer (GOCE) mission over Fennoscandia. Numerical investigations show that the integral formulas have neither isotropic nor well-behaved kernels. In such a case, gravity anomaly recovery is not successful due to large spatial truncation error of the integral formulas. Reformulation of the problem by combining the orbital elements and their velocities leads to an integral with a well-behaved kernel which is suitable for our purpose. Also based on these combinations some general relations among the orbital elements and their velocities are obtained which can be used for validation of orbital parameters and their velocities.     

广义离散随机线性系统的最优调节器

讨论广义离散随机线性系统在二次型性能指标下的最优控制问题。导出的最优控制律由系统输出和部分状态的线性反馈构成,这不仅降低了滤波的黎卡提方程的阶次,显著地减少了计算量,而且在工程中也是可实现的。     

再入飞行器高超声速绕流的一步和二步有限元计算

本文针对再入飞行器的空气动力问题，采用一步和二步有限元格式求解可缩守恒型Ｅｕｌｅｒ方程，并结合不同的人工粘性模型来捕捉激波，给出了高超声速二维钝头绕流的结果。     

带副翼三维机翼绕流的N-S方程解

提出了一种求解带副翼偏转三维机翼绕流的N-S方程计算方法。采用对接分区网格与分区求解算法的结合,有效地求解绕此外形的复杂流动。提出了一种满足通量守恒的内边界耦合条件。数值方法中选用vanLeer分裂格式离散无粘通量项,并构造了一种Limiter函数以保证TVD性质,采用中心差分格式来离散粘性通量项。数值算例表明该方法是求解带操纵面偏转的机翼绕流的有效方法。     

三维不可压边界层抛物化稳定性方程的椭圆特性研究

针对三维平行不可压边界层流动的抛物化稳定性方程,研究其剩余的椭圆特性,提出了消除该特性的具体方法,并对抛物化稳定性方程解与全椭圆问题解的一致性进行了证明。     

PVM平台下通量守恒的嵌入自适应网格解激波和底部流

运用嵌入式自适应网格技术来提高结构网格求解复杂流场的分辨率。该方法根据流场的形成,将密集网格嵌入到物理量剧烈变化的区域,使求解精度得以提高的同时,避免较大的计算开销,从而达到求解效率和求解精度之间的平衡。 Ｐ Ｖ Ｍ 平台使得被嵌入的网格可以在网络中不同的机器上完成,大幅度降低了墙上时间。原始网格与被嵌入网格之间数值通量守恒的实现增强了该方法在捕捉间断时的有效性和可靠性。     

人工释能法求解线性代数方程组

本文建立求解线性代数方程组的人工释能法迭代格式,并给出该迭代格式收敛的充分必要条件和最佳释能时机,同时给出实现人工释能法的数值计算方法及其数值稳定性条件。