飞行器航迹倾角的自适应动态面控制

针对飞行器纵向模型具有参数不确定性和外界干扰的特点,提出一种飞行器航迹倾角的自适应动态面控制方法.动态面控制方法通过引入一阶低通滤波器避免了传统反演设计存在的"微分爆炸"现象,采用自适应律对模型未知参数进行在线估计,并利用非线性阻尼项克服外界干扰.通过Lyapunov方法证明得出闭环系统半全局一致稳定,跟踪误差可通过调节控制器参数达到任意小.仿真结果表明:该方法能在简化控制设计过程的同时保证航迹倾角跟踪上预定轨迹,控制系统具有较强的自适应能力且对外界干扰具有一定的鲁棒性.     

大攻角侧向喷流流场特性及喷流干扰效应

采用HLLC近似黎曼解格式求解N-S方程,对大攻角条件下超音速尖拱细长旋成体导弹的单侧向喷流干扰流场进行了数值模拟.并对喷流流场压力分布、喷口附近流动及流场旋涡结构进行了研究,分析了大攻角对细长旋成体侧向喷流干扰压力分布及干扰因子的影响.研究结果表明,HLLC格式计算复杂流场具有较好的数值稳定性;侧向喷流与来流的干扰总...     

运载器末助推段非线性姿态控制器设计

根据单摆模型近似晃动质量推导晃动运动与姿态运动的动力学方程,基于状态相关黎卡提方程方法,综合动态逆控制方法设计了运载器末助推段非线性姿态控制器,由状态反馈实现姿态跟踪和晃动抑制。因实际中模拟晃动运动的单摆状态无法测量,引入输出多采样率技术,通过在一个采样周期内多次检测被控对象的输出估计状态,实现设计的状态反馈控制律。数...     

跨超声速风洞大开角段设计技术研究

跨超声速风洞大开角段设计技术研究对于提高大开角段的安全性能与改进稳定段入口气流质量有着重大意义.由于影响大开角段性能的参数较多,完全通过试验方法进行设计的成本过高.本文通过数值模拟方法,结合适当的边界条件,对不同参数的大开角段进行了模拟,从数值模拟的结果可以看到,孔板开孔率和扩开角对大开角段性能有显著影响,通过比较得出了较为合理的参数匹配.这表明本文所用的方法用于大开角段气动设计是可行的,这为数值模拟方法应用于风洞部段气动设计创造了一定的条件.     

周向总压畸变条件下多级轴流压气机失速首发级预测分析

基于多级轴流压气机的逐级特性,发展了1种预测周向总压畸变条件下多级轴流压气机失速首发级的方法。该方法结合平行压气机模型和级叠加计算方法,以进气畸变条件下多级轴流压气机某级的有效相对气流角达到稳定状态时该级的最大相对气流角为条件,进行多级轴流压气机失速首发级的预测分析。通过对J85—13发动机8级轴流压气机总压畸变试验数据进行模拟计算,预测出该轴流压气机畸变条件下的失速首发级。     

Ionization effect of solar protons in the Earth atmosphere – Case study of the 20 January 2005 SEP event

The cosmic ray ground level enhancement on January 20, 2005 is among the largest recorded events in the history of cosmic ray measurements. The solar protons of MeV energies cause an excess of ionization in the atmosphere, specifically over polar caps following major solar disturbances. The ionization effect in the Earth atmosphere is obtained for various latitudes on the basis of solar proton energy spectra, reconstructed from GOES 11 measurements and subsequent full Monte Carlo simulation of cosmic ray induced atmospheric cascade. The estimation of ionization rates is based on a numerical model for cosmic ray induced ionization. The evolution of atmospheric cascade is performed with the CORSIKA 6.52 code using FLUKA 2006b and QGSJET II hadron interaction models. The atmospheric ion rate ionization is explicitly obtained for 40°N, 60°N and 80°N latitudes. The time evolution of obtained ion rates is presented. It is demonstrated that ionization effect is negative for 40°N and small for 60°N, because of accompanying Forbush decrease. The ionization effect is significant only in sub-polar and polar atmosphere during the major ground level enhancement of 20 January 2005.     

Drag force on solar sails due to absorption of solar radiation

We consider a special relativistic effect, known as the Poynting–Robertson effect, on various types of trajectories of solar sails. Since this effect occurs at order v^?/c, where v^? is the transversal speed relative to the sun, it can dominate over other special relativistic effects, which occur at order v²/c². While solar radiation can be used to propel the solar sail, the absorbed portion of it also gives rise to a drag force in the transversal direction. For escape trajectories, this diminishes the cruising velocity, which can have a cumulative effect on the heliocentric distance. For a solar sail directly facing the sun in a bound orbit, the Poynting–Robertson effect decreases its orbital speed, thereby causing it to slowly spiral towards the sun. We also consider this effect for non-Keplerian orbits in which the solar sail is tilted in the azimuthal direction. While in principle the drag force could be counter-balanced by an extremely small tilt of the solar sail in the polar direction, periodic adjustments are more feasible.     

The possibilities of polar meteorology,environmental remote sensing,communications and space weather applications from Artificial Lagrange Orbit

The ability to observe meteorological events in the polar regions of the Earth from satellite celebrated an anniversary, with the launch of TIROS-I in a pseudo-polar orbit on 1 April 1960. Yet, after 50 years, polar orbiting satellites are still the best view of the polar regions of the Earth. The luxuries of geostationary satellite orbit including rapid scan operations, feature tracking, and atmospheric motion vectors (or cloud drift winds), are enjoyed only by the middle and tropical latitudes or perhaps only cover the deep polar regions in the case of satellite derived winds from polar orbit. The prospect of a solar sailing satellite system in an Artificial Lagrange Orbit (ALO, also known as “pole sitters”) offers the opportunity for polar environmental remote sensing, communications, forecasting and space weather monitoring. While there are other orbital possibilities to achieve this goal, an ALO satellite system offers one of the best analogs to the geostationary satellite system for routine polar latitude observations.     

太阳模拟器光照不均匀性的研究

辐照不均匀性是太阳模拟器的一项主要技术指标.首先通过对国内外辐照不均匀性测量装置进行了充分的调研,决定采用“决门法”设计完成了辐照不均匀性的测量装置.接着通过试验证明了晴空无遮挡的太阳光可以作为该装置的标准光源并进行了该装置的标定.然后,利用该装置对自然光源进行了测试,结果与利用标准表测试一致.最后,利用该装置对脉冲式太阳模拟器的辐照不均匀性进行了现场测试.     

经济型月球探测器精确定点软着陆制导算法

针对未来经济型月球探测器精确定点软着陆问题,考虑发动机特性及终端状态约束,对主减速段制导算法进行了研究。首先考虑到未来月球通信网络的建立和资源的利用,提出了一种探测器在环月极轨道运行时的月面着陆点全覆盖环月调相策略。然后在北东地坐标系下建立软着陆主减速段的质心动力学模型,依据动力学模型将探测器的运动分为纵向平面运动和横向运动并分别设计在线闭环制导律。纵向平面运动采用改进显式制导算法,并基于有限推力思想和主减速段误差传播特性设计了满足终端航向位置约束的点火角修正策略;对于横向运动控制,首先基于ZEM/ZEV最优反馈制导律给出横向制导指令,然后采用PWPF将连续形式的制导指令调制为脉冲形式。仿真结果表明了该制导律能够满足所有终端状态约束,具有燃耗次优性、自主性、实时性和一定的鲁棒性,同时易于工程实现。