非线性弹簧形态优化及可调节恒力装置设计

基于组合结构研究一种可调节恒力装置的设计方法，恒力装置由负刚度非线性弹簧和正刚度线性弹簧组合而成。采用B样条曲线描述非线性弹簧的形态，基于GA算法和非线性有限元法实现非线性弹簧的形态优化设计。根据恒力装置的工作原理，设计线性螺旋弹簧，并分析刚度/强度特性。组合结构的力学性能分析表明恒力装置可以实现输出恒力。为了实现自我保护、输出的恒力大小/方向可调，进行了恒力装置的部组件设计。本文的恒力装置设计方法为平面薄膜天线和太阳电池阵的工程研制提供了技术支撑。     

Coupled Stress-Electricity Model for Electromagnetic Emission Induced by Concrete Fracture

Electromagnetic emission induced during concrete fracturing is of great significance to health monitoring of concrete structures.A coupled stress-electricity model is established by analyzing the interaction between stress and electricity during concrete fracturing.And based on this model,the electromagnetic radiation parameters are calculated.The theoretical calculation is well coincident with experimental results.This work provides theoretical support for concrete testing system.     

超高速撞击下PTFE/Al含能材料薄板的载荷特性分析

不同于传统惰性材料的空间碎片防护结构,含能材料防护结构在超高速撞击下的冲击起爆特性是其防护能力得以提高的根本原因。PTFE/Al含能材料防护结构的冲击起爆特性改变了弹丸强冲击载荷下的破碎机制,弹丸内部的冲击压力对于分析含能材料在超高速撞击下的防护机理具有重要意义。对超高速撞击试验中回收的PTFE/Al防护结构后板进行损伤特性分析,获得了对应速度条件下弹丸的破碎特性。基于一维冲击波理论,分析PTFE/Al靶板在超高速撞击条件下的冲击响应过程,结合考虑化学反应效率的热化学反应模型,获得了弹丸在碰撞与爆炸联合作用下的载荷特性,通过与试验结果对比验证,获得该材料完全反应的临界撞击速度约为1800 m/s,弹丸的临界破碎速度为2875 m/s,小于铝防护结构中对应的临界破碎速度。给出了弹丸在PTFE/Al、铝两种防护结构中产生相同冲击压力时对应的临界速度,分别为弹道段的800 m/s和破碎段的3580 m/s。     

Application of small-size antennas for estimation of angles of arrival of HF signals scattered by ionospheric irregularities

A modification of the Doppler Interferometry Technique is suggested to enable estimating angles of arrival of comparatively broadband HF signals scattered by random irregularities of the ionospheric plasma with the use of small-size weakly directional antennas. The technique is based on the measurements of cross-spectra phases of the probe radiation recorded at least in three spatially separated points. The developed algorithm has been used to investigate the angular and frequency-time characteristics of HF signals propagating at frequencies above the maximum usable one (MUF) for the direct radio path Moscow-Kharkiv. The received signal spectra show presence of three families of spatial components attributed, respectively, to scattering by plasma irregularities near the middle point of the radio path, ground backscatter signals and scattering of the sounding signals by the intense plasma turbulence associated with auroral activations. It has been shown that the regions responsible for the formation of the third family components are located well inside the auroral oval. The drift velocity and direction of the auroral ionosphere plasma have been determined. The obtained estimates are consistent with the classical conception of the ionospheric plasma convection at high latitudes and do not contradict the results of investigations of the auroral ionosphere dynamics using the SuperDARN network.     

月面远程运输飞行轨迹优化设计

针对月球表面不同区域之间的载人或载货运输问题,设计了一种基于上升-巡航-下降模式的燃料最省飞行轨迹。首先通过求解不同飞行时间的Lambert问题确定了最佳飞行时间,并获得了对应的双脉冲解,然后利用有限推力替代两次速度脉冲,建立了非线性规划问题,求解得到了有限推力燃料最省飞行轨迹。优化设计过程中主要研究了两个主要难点:bang-bang控制与飞行高度约束。这两个问题通过推力加速度与飞行时间的数值延拓得以解决,同时揭示了月面飞行的基本原理。最后给出了3种不同应用场景的仿真算例,仿真结果表明,当飞行时间为小时量级时,上升-巡航-下降飞行模式下的优化解即为燃料最优解,如果飞行距离较远,则还需要适当增加飞行时间从而满足飞行高度约束。     

Ionospheric F2-Layer critical frequency retrieved from COSMIC radio occultation: A statistical comparison with measurements from a meridional ionosonde chain over Southeast Asia

In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed.     

Platform LSF软件在高性能计算集群中的实施与应用

随着信息处理技术的精度、可靠度等要求的进一步提高,采用高性能计算集群系统已经成为数字化制造中的关键技术之一.本文结合高性能计算应用现状的不足,阐述了Platform LSF软件设计思想和目标,介绍了该软件的实施与应用情况.     

对相控阵雷达自适应旁瓣对消的多点源压制干扰

分析了相控阵雷达自适应旁瓣对消的工作原理及方法.然后提出了用多台干扰设备协同工作的相参干扰.每台干扰设备在雷达处理间隔内发射能覆盖真实目标并且持续时间较短的干扰信号,多台设备协同工作在目标附近形成压制干扰.该方法影响雷达样本选择,从而降低自适应旁瓣对消的效果.仿真结果和外场试验表明了该方法的有效性.     

径向入射激波聚焦实验和数值模拟研究

为得到不同入射激波马赫数对凹腔内径向入射激波聚焦过程的影响,对马赫数为1.25和2.18的径向入射激波在实验段内反射聚焦的过程进行了实验和数值模拟研究。用高速CCD拍摄了凹腔中气流流场的纹影图片,并采用保持强稳定性的龙格—库塔格式、加权基本无振荡算法和块结构动态自适应网格加密对激波反射聚焦的过程进行了数值模拟,实验和数值模拟结果吻合较好。复杂的激波形状及其之间的相互作用(如激波反射,激波聚焦和不同激波的相互作用)在实验和数值模拟中都能很好地观测到。通过比较不同马赫数入射激波的反射聚焦过程,发现较高的马赫数下聚焦后能产生射流,而较低的马赫数下却没有。同时发现,入射激波马赫数能影响二次激波出现的位置和强度,进而影响聚焦过程流场的紊乱程度。     

Avoid online radiation risk: Theoretical simulation of chromosome breaks in cells exposed to heavy ions

In this study, we report an easy and quick method on simulating chromosome breaks in cells exposed to heavy charged particles. The theoretical value of chromosome break was calculated, and validated comparison with experimental value by using premature chromosome condensation technique. A good consistency was found between theoretical and experimental value. This suggested that higher relative biological effectiveness of heavy ions was closely correlated with its physical characteristics. Also, a safe approach on predicting chromosome breaks in cells exposed to heavy ions at off-line environment can be considered. Furthermore, three key factors influencing the theoretical simulation was investigated and discussed.