氢喷射温度对氢氧火箭发动机燃烧稳定性的影响

应用CFD方法对氢氧火箭发动机中高频燃烧不稳定性进行了数值模拟,研究分析了不同工况条件下氢喷射温度对燃烧振荡的影响规律,得出了压力振荡频率变化规律及稳定性极限图。结果表明：在一定的氢喷射温度范围内会发生不稳定燃烧,且随着混合比的增大,发生不稳定燃烧的氢喷射温度上限增大;不稳定燃烧振荡主频呈倍频关系,且在氢喷射温度（70K～110K）内,振荡主频最大。     

等参化FVDAM在复合材料湿热应力分析中的应用

在等参化有限元体积直接平均法（FVDAM）中引入等效湿胀系数,建立了复合材料湿热耦合的细观应力场分析模型。计算了湿热环境中不同纤维体积含量和湿含量复合材料的细观应力场。结果表明：湿热环境中复合材料界面径向应力最大值发生于纤维密集区的相邻纤维间的界面处,最小值出现在基体富区;初始吸湿对热残余应力有释放作用,最终吸湿的影响将超过热残余应力,界面应力状态也随之改变。计算所得细观应力场与有限元（FEM）法有较好的一致性。     

Hydrodynamic instabilities and transverse waves in propagation mechanism of gaseous detonations

The present study examines the role of transverse waves and hydrodynamic instabilities mainly, Richtmyer–Meshkov instability (RMI) and Kelvin–Helmholtz instability (KHI) in detonation structure using two-dimensional high-resolution numerical simulations of Euler equations. To compare the numerical results with those of experiments, Navier–Stokes simulations are also performed by utilizing the effect of diffusion in highly irregular detonations. Results for both moderate and low activation energy mixtures reveal that upon collision of two triple points a pair of forward and backward facing jets is formed. As the jets spread, they undergo Richtmyer–Meshkov instability. The drastic growth of the forward jet found to have profound role in re-acceleration of the detonation wave at the end of a detonation cell cycle. For irregular detonations, the transverse waves found to have substantial role in propagation mechanism of such detonations. In regular detonations, the lead shock ignites all the gases passing through it, hence, the transverse waves and hydrodynamic instabilities do not play crucial role in propagation mechanism of such regular detonations. In comparison with previous numerical simulations present simulation using single-step kinetics shows a distinct keystone-shaped region at the end of the detonation cell.     

Heliopause stability revisited: dispersion analysis and numerical simulations

The heliopause, a surface separating the tenuous hot heliosheath flow and the dense, strongly magnetized interstellar flow, is subject to instabilities of the Rayleigh–Taylor and Kelvin–Helmholtz types. The dynamic evolution of this discontinuity is of considerable importance for understanding the neutral atom and cosmic-ray filtration at the interface. Here, we investigate the stability of the upwind heliopause in the presence of charge exchange collisions using both an analytic (dispersion relation) approach and a numerical model that includes the interstellar magnetic field. The linear analysis yields a cubic dispersion relation that admits imaginary solutions for the full range of wavenumbers, implying that the stagnation point on the heliopause is unconditionally Rayleigh–Taylor unstable to small perturbations propagating parallel to the discontinuity surface. We confirm this result by following the nonlinear development of the instability with a time-dependent simulation using a four fluid MHD-neutral numerical code. For the typical solar wind and LISM conditions, we obtain cyclical evolution of the upwind heliopause with a period of the order of 100 years. We also identify two areas of space physics where the instability may have important implications.     

空间对接机构电磁阻尼器参数优化设计研究

电磁制动阻尼器曾被苏联用作周边式对接机构中的阻尼器,成功地完成多次对接任务,但是现有文献中只对它进行了定性分析,对设计还缺乏足够的依据。本文首先对这种电磁制动器的电磁场进行定量分析,并求解其电磁场,由此推导出电磁制动器的制动力矩。     

某涡喷发动机压气机气动失稳过程的非线性分析

对某涡喷发动机压气机的气动失稳过程进行了相关积分分析。对节流过程中压气机静压信号进行延时嵌入重构,发现失稳过程中重构相空间的吸引子结构发生了显著变化;应用相关积分值作为压气机内部流动状况变化的评价指标,发现节流过程中压气机第1级端部的流动最先发生不稳定,随后第2级先于第3,4级发生不稳定征兆;1,2级的失速类型为渐进型失速,3,4级为突变型失速;第3级叶根最先发生不稳定,且发展较快,最终导致全叶高失速;低通滤波可以提高相关积分方法检测失速征兆的时效性。分析表明,非线性的相关积分分析方法是进行压气机气动失稳过程研究的有效手段。      

曲率连续的非轴对称短舱气动型面参数化设计方法研究

为了进一步提高短舱内外流的气动性能,基于类别形状函数方法建立了曲率连续的非轴对称短舱气动型面参数化设计方法。主要思路是先设计关键截面型线,再设计纵向型线,最后通过纵向型线周向有序组合建立气动型面。为评价所建立的短舱气动型面设计方法的适用性,从曲率半径分布、主要工况下的流动特性和气动性能三个方面对所发展的方法和基于圆锥曲线的方法设计的超大涵道比(UHBPR)短舱进行了对比研究。结果表明：与基于圆锥曲线的方法设计的短舱相比,所建立的方法设计的短舱气动型面不存在轴向曲率半径波动。由于消除了曲率波动引起的短舱壁面附近局部过度加速形成的高速低压区,在马赫数为0.8的巡航条件下外罩壁面局部阻力降低了4.5%；在马赫数为0.82的飞行工况下,外罩壁面局部阻力降低了5.5%。进气道气动型面设计方法的改进,使得大攻角爬升条件下进气道总压恢复系数提高了0.41%,稳态周向总压畸变指数减小了8.82%。     

Analysis of the orbit lifetime of CubeSats in low Earth orbits including periodic variation in drag due to attitude motion

It is estimated that more than 22,300 human-made objects are in orbit around the Earth, with a total mass above 8,400,000 kg. Around 89% of these objects are non-operational and without control, which makes them to be considered orbital debris. These numbers consider only objects with dimensions larger than 10 cm. Besides those numbers, there are also about 2000 operational satellites in orbit nowadays. The space debris represents a hazard to operational satellites and to the space operations. A major concern is that this number is growing, due to new launches and particles generated by collisions. Another important point is that the development of CubeSats has increased exponentially in the last years, increasing the number of objects in space, mainly in the Low Earth Orbits (LEO). Due to the short operational time, CubeSats boost the debris population. One of the requirements for space debris mitigation in LEO is the limitation of the orbital lifetime of the satellites, which needs to be lower than 25 years. However, there are space debris with longer estimated decay time. In LEÓs, the influence of the atmospheric drag is the main orbital perturbation, and is used in maneuvers to increment the losses in the satellite orbital energy, to locate satellites in constellations and to accelerate the decay.The goal of the present research is to study the influence of aerodynamic rotational maneuver in the CubeSat?s orbital lifetime. The rotational axis is orthogonal to the orbital plane of the CubeSat, which generates variations in the ballistic coefficient along the trajectory. The maneuver is proposed to accelerate the decay and to mitigate orbital debris generated by non-operational CubeSats. The panel method is selected to determine the drag coefficient as a function of the flow incident angle and the spinning rate. The pressure distribution is integrated from the satellite faces at hypersonic rarefied flow to calculate the drag coefficient. The mathematical model considers the gravitational potential of the Earth and the deceleration due to drag. To analyze the effects of the rotation during the decay, multiple trajectories were propagated, comparing the results obtained assuming a constant drag coefficient with trajectories where the drag coefficient changes periodically. The initial perigees selected were lower than 400 km of altitude with eccentricities ranging from 0.00 to 0.02. Six values for the angular velocity were applied in the maneuver. The technique of rotating the spacecraft is an interesting solution to increase the orbit decay of a CubeSat without implementing additional de-orbit devices. Significant changes in the decay time are presented due to the increase of the mean drag coefficient calculated by the panel method, when the maneuver is applied, reducing the orbital lifetime, however the results are independent of the angular velocity of the satellite.     

可控肥皂膜气柱界面与激波相互作用的实验研究

基于肥皂膜技术提出了一种生成气柱界面的简单方法。形成的界面不需要支撑网格,因此初始条件可以很好地控制。在水平激波管中结合高速纹影开展了平面激波与二维或三维气柱界面作用的实验。纹影照片显示实验结果杂波更少,演变中的界面也比文献的结果更对称。此外,还特别研究了由极小曲面特征导致的三维效应,发现三维效应使界面的演变和发展变慢了。本研究将有助于更多了解三维性对Richtmyer-Meshkov不稳定性发展的影响。     

带滑移滞变系统的三阶段逐步收敛的识别方法

针对非线性带滑移滞变系统模型复杂，参数多，识别时收敛困难等问题，提出了一种三阶段逐步收敛的识别方法对Baber与Noori提出的带滑移滞变模型进行了参数识别。计算实例表明，该方法具有收敛速度快、且容易收敛的特点，对于参数较多、模型复杂的系统，是一种非常有效的参数识别方法。