高精度接触式测头测量力影响分析与建模

针对高精度非球面检测过程中,测量力对接触式传感器测头测量不确定度的影响问题,本文在建立接触式测头简化结构模型的基础上,分析建立了测杆倾斜、滑动以及弯曲变形对测量精度的影响模型.并通过仿真分析得出了高精度非球面测量过程中接触式测头受非球面相对口径等的影响规律,即,其中测杆的弯曲变形是测量力影响的主要分量.为进一步提高接触式测量的精度奠定了基础.     

脉冲微推力器平均推力测量研究

平均推力测量是脉冲微推力器推进性能研究的关键问题之一。研究了在标准的周期性信号作用下,二阶系统的响应与输入之间的关系。在欠阻尼条件下,得到了系统稳态平均回复力等于平均推力的重要结论,仿真结果证实了结论。研究结果亦可应用于脉冲微推力器的总冲研究。     

Driving major solar flares and eruptions: A review

This review focuses on the processes that energize and trigger M- and X-class solar flares and associated flux-rope destabilizations. Numerical modeling of specific solar regions is hampered by uncertain coronal-field reconstructions and by poorly understood magnetic reconnection; these limitations result in uncertain estimates of field topology, energy, and helicity. The primary advances in understanding field destabilizations therefore come from the combination of generic numerical experiments with interpretation of sets of observations. These suggest a critical role for the emergence of twisted flux ropes into pre-existing strong field for many, if not all, of the active regions that produce M- or X-class flares. The flux and internal twist of the emerging ropes appear to play as important a role in determining whether an eruption will develop predominantly as flare, confined eruption, or CME, as do the properties of the embedding field. Based on reviewed literature, I outline a scenario for major flares and eruptions that combines flux-rope emergence, mass draining, near-surface reconnection, and the interaction with the surrounding field. Whether deterministic forecasting is in principle possible remains to be seen: to date no reliable such forecasts can be made. Large-sample studies based on long-duration, comprehensive observations of active regions from their emergence through their flaring phase are needed to help us better understand these complex phenomena.     

Possible physical properties of the flow in the vicinity of the heliopause

An interface between the fully ionized hydrogen plasma of the solar wind (SW) and the partially ionized hydrogen gas flow of the local interstellar medium (LISM) is formed as a region where there is a strong interaction between these two flows. The interface is bounded by the solar wind termination shock (TS) and the LISM bow shock (BS) and is separated on two regions by the heliopause (HP) separating the solar wind and charged component of the LISM (plasma component below). The BS is formed due to the deceleration of the supersonic LISM flow relative to the solar system. Regions of the interface between the TS and HP and between the HP and BS were in literature named as the inner and outer heliosheaths, respectively. An investigation of the structure and physical properties of the heliosheath is at present especially interested due to the fact that Voyager-1 and Voyager-2 have crossed the TS in December 2004 (Burlaga, L.F., Ness, N.F., Acuna, M.Y., et al. Crossing the termination shock into the the heliosheath. Magnetic fields. Science 309, 2027–2029, 2005; Fisk, L.A. Journey into the unknown beyond. Science 309, 2016–2017, 2005; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Voyager 1 in the foreshock, termination shock and heliosheath. Science 309, 2020–2024, 2005; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. Voyager 1 explores the termination shock region and the heliosheath beyond. Science 309, 2017–2020, 2005) and in September 2007 (Jokipii, J.R. A shock for Voyager 2. Nature 454, 38–39, 2008; Gurnett, D.A., Kurth, W.S. Intense plasma waves at and near the solar wind termination shock. Nature 454, 78–80, 2008. doi: 10.1038/nature07023; Wang, L., Lin, R.P., Larson, D.E., Luhmann, J.G. Domination of heliosheath pressure by shock-accelerated pickup ions from observations of neutral atoms. Nature 454, 81–83, 2008. doi: 10.1038/nature07068.14; Burlaga, L.F., Ness, N.F., Acuna, M.H., et al. Magnetic fields at the solar wind termination shock. Nature 454, 75–77, 2008. doi: 10.1038/nature07029; Richardson, J.D., Kasper, J.C., Wang, C., et al. Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock. Nature 454, 63–66, 2008. doi: 10.1038/nature07024; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. An asymmetric solar wind termination shock. Nature 454, 71–74, 2008. doi: 10.1038/nature07022; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Mediation of the solar wind termination shock by non-thermal ions. Nature 454, 67–70, 2008. doi: 10.1038/nature 07030), respectively, and entered to the inner heliosheath.     

基于FPGA的可变尺寸块运动估计高效结构

针对可变尺寸块运动估计(VBSME,Variable Block-Size Motion Estimation)的硬件结构在现场可编程门阵列(FPGA, Field Programmable Gate Array)上实现时消耗资源多且速度慢的问题,提出了一种面积和速度优化的VBSME硬件结构.其中,绝对差累加和(SAD,Sum of Absolute Differences)的计算采用基于随机存储器(RAM,Random Access Memory)的累加计算方式,比基于寄存器合并的方式节省了面积并增加了速度;通过采用脉动比较链而非总线结构,增强了多个SAD值的比较能力,并能高效地实现对部分差排除算法(PDE,Partial Difference Elimination)的支持.基于Virtex-II型FPGA器件,本结构消耗了2261个slice,时钟频率达到164MHz,在搜索窗口为16×16时可实时处理标清格式的视频.与同类设计相比,设计的面积可减少77%,速度增加218%,FPGA的硬件效率显著提升.     

基于成像拖尾效应的图像测速算法

根据相机成像拖影长度与相机运动及曝光时间的关系,提出一种基于成像拖尾效应的图像测速方法,给出了用航拍相机进行图像测速的实施方案。建立了影像与成像平面和地面景物间的相对运动模型,设计了基于互相关分析的拖影长度测量方案,给出了测量算法,并分析了像素尺寸和成像比例等对测速精度的影响。算例表明：该法对速度无剧烈变化的准匀速运动的测速效果较好,为飞行器实时飞行速度测量提供了一种解决方案。     

某型号固体发动机推力测试偏差与侧向力干扰问题分析与试验

分析了影响某固体发动机静止试验推力测试偏差的因素.分析结果表明,由于试车架结构问题,发动机工作过程产生的偏斜力与偏心力以及各个方向的振动是推力测试偏差过大的主要因素.据此优化设计试车架结构,控制并减少安装偏差,消除侧向力对工作传感器的干扰,提高推力测试的可靠性,以满足固体火箭发动机推力测试技术要求.     

磁响应Fe3O4/HCS复合微球的制备及特性

由壳聚糖与环氧丙烷制备了羟丙基壳聚糖(HCS)。将其配制成水溶液,利用离子凝胶法,与多聚磷酸钠(TPP)反应,制备了粒径在0.6μm羟丙基壳聚糖微球。再用滴定水解法制备了四氧化三铁微粒,激光粒度分析显示滴定水解法制备的Fe3O4粒径分布较窄,粒径小。在此基础上采用交联聚合法制备了Fe3O4/HCS复合微球,微球为实心,四氧化三铁微粒被包裹于微球内部,形状规则,粒径约为0.8μm,经过磁响应分析表明Fe3O4/HCS复合微球具有磁响应性。     

有源相控阵中场测量中的空间误差研究

由于中场监测设备量少,且测量效率高,所以是有源相控阵雷达阵面测量的重要方法之一,在工程中得到了广泛应用。其系统误差包括监测方法误差和测量设备误差,其中测量方法误差非常关键,而测量设备误差与所采用的具体设备有关。在中场测量中,探头的位置偏移导致的空间误差是其特有的测量方法误差。本文对空间误差进行了理论分析,并以x波段有源相控阵的中场测量为例,给出了空间误差的计算结果和实验结果。计算结果表明,空间幅度误差很小;空间相位误差与被测阵面口径、测量距离和探头位置偏移有关。实验结果进一步验证了这种计算结果。分析结果为中场测量的实施提供了参考,具有一定的工程意义。