复合固体推进剂燃速温度敏感系数的模拟计算

本文根据“价电子反应”稳态燃烧模型和模拟计算方法,模拟计算了AP粒径、粒径分布宽度,AL含量、AL粒径以及压力对“AP/AL/HTPB/催化剂”系列推进剂的燃速温度敏感系数σp的影响规律,结果同文献[4]所综合或分析预测的结果一致.可以认为:初温对凝聚相反应的影响是主要的;AP粒径越大,σp越高;AP粒径分布宽度对σp有显著影响;铝含量增加,σp略有降低,压力升高,σp降低.     

气体密度超声检测法的研究

介绍了一种利用超声技术在线快速测量气体密度的方法。其原理是测出气体介质的压力和声速后,再根据由热力学和弹性介质力学建立起来的压力、声速和密度之间的关系算出密度。所有监控、测量和数据处理均由微机完成。还给出了在几种不同介质中的试验结果,并对结果进行了半定量的误差分析。与理论分析相比,有较好的一致性。超声检测法是一种在线检测气体密度的新方法。     

等效动压洞壁干扰修正方法的研究与应用

带螺旋桨飞机模型风洞实验进行洞壁干扰修正时,必须考虑螺旋桨滑流的影响。运用等效动压对运八飞机带螺旋桨模型风洞实验才气进行洞壁干扰修正,分析洞壁对带螺旋桨飞机模型试验数据的影响,并与壁压信息修正方法进行了比较。两种修正方法的修正结果基本一致,壁压信息法能实际反映洞壁干扰影响,但壁压信息法需要进行准确的壁压测量,增加实验工作量;等效动压法是以经典的洞壁干扰修正公式为基础,考虑了螺旋桨滑流的影响,而且带     

基于图像特征分类和RBF网络的两轴车辆动态称重技术

汽车在行驶过程中的总重信号通常由各轴重信号确定,各轴重信号的测试精度取决于对车辆运动参数和振动信号等的精确分析。本文采用径向基函数(Radial basis function,RBF)网络处理轴重信号,针对该网络的泛化能力与拟合精度的矛盾,将车辆按照重量分为大、中、小3种类型,并进行整车建模和网络训练;实际测试过程中,利用汽车俯视图像提取类型特征,然后根据汽车的类型将测试参数输入不同的神经网络进行处理,以静态测量结果为相对真值。仿真结果表明,分类建模比单一混合建模具有更高的测试精度。     

基于合作目标和视觉的无人飞行器全天候自动着陆导引关键技术

 GPS受他国控制和易受干扰对基于该导航系统的无人飞行器导航和着陆具有潜在危险,为了使其安全自动着陆,提出通过在着陆跑道(广场或公路)上预设具有受控发射红外光的地面合作目标,实现无人飞行器的视觉全天候自动精确着陆新技术。首先研究得到切实可行的工作过程;然后研制了合作目标,通过理论分析和实验得出,无论能见度高低,8~12 μm中远红外视觉系统探测到的合作目标图像质量远优于可见光视觉系统,研究得到合作目标和背景的温差在170~200 ℃时,成像效果最好。在识别研究中发现,基于传统的不变矩算法对合作目标的识别可靠性稍差,为了进一步准确地识别合作目标,又提出了基于方向链码的合作目标识别算法,该方法的耗时为不变距的96%,但是识别的可靠性比前者有显著提高。     

冲压发动机超声速进气道研究进展

超声速进气道是冲压发动机的关键部件之一。简要介绍了冲压发动机常用的典型进气道。重点叙述了进气道的最新研究成果,主要包括等溢流角弯曲前缘侧壁压缩进气道设计概念、支板引射压缩进气道、双模态超燃冲压发动机变几何进气道、全外压缩式超声速“参数进气道”、固定型面方转椭圆形超声速进气道（REST）等的设计概念与方案。最后概括了先进进气道的发展趋势。     

Inter-satellite calibration of FengYun 3 medium energy electron fluxes with POES electron measurements

We perform an L-shell dependent inter-satellite calibration of FengYun 3 medium energy electron measurements with POES measurements based on rough orbital conjunctions within 5?min?×?0.1?L?×?0.5 MLT. By comparing electron flux data between the U.S. Polar Orbiting Environmental Satellites (POES) and Chinese sun-synchronous satellites including FY-3B and FY-3C for a whole year of 2014, we attempt to remove less reliable data and evaluate systematic uncertainties associated with the FY-3B and FY-3C datasets, expecting to quantify the inter-satellite calibration factors for the 150–350?keV energy channel at L?=?2–7. Compared to the POES data, the FY-3B and FY-3C data generally exhibit a similar trend of electron flux variations but more or less underestimate them within a factor of 5 for the medium electron energy 150–350?keV channel. Good consistency in the flux conjunctions after the inter-calibration procedures gives us certain confidence to generalize our method to calibrate electron flux measurements from various satellite instruments.     

基于大气偏振光的载体姿态参数提取方法

大气偏振模式是地球自有属性,可为大气层内的生物和载体提供导航信息.提出一种利用大气偏振模式矢量性特征获取载体姿态参数的直接方法,首先利用图像法从单反相机获取的180°全天域灰度图中重建出大气偏振模式,然后对该模式进程进行分析和处理,确定出天空每个测量点的E-矢量信息,接着利用这些E-矢量建立载体的姿态变换矩阵,最后引入奇异值分解的经典方法最小化误差函数,获取到载体的姿态参数.该方法的有效性通过模拟飞行器控制台得以验证,最大解算偏差不超过0.5°.     

Occurrence features of simultaneous H+- and He+-band EMIC emissions in the outer radiation belt

As an important loss mechanism of radiation belt electrons, electromagnetic ion cyclotron (EMIC) waves show up as three distinct frequency bands below the hydrogen (H⁺), helium (He⁺), and oxygen (O⁺) ion gyrofrequencies. Compared to O⁺-band EMIC waves, H⁺- and He⁺-band emissions generally occur more frequently and result in more efficient scattering removal of <～5?MeV relativistic electrons. Therefore, knowledge about the occurrence of these two bands is important for understanding the evolution of the relativistic electron population. To evaluate the occurrence pattern and wave properties of H⁺- and He⁺-band EMIC waves when they occur concurrently, we investigate 64 events of multi-band EMIC emissions identified from high quality Van Allen Probes wave data. Our quantitative results demonstrate a strong occurrence dependence of the multi-band EMIC emissions on magnetic local time (MLT) and L-shell to mainly concentrate on the dayside region of L?=?～4–6. We also find that the average magnetic field amplitude of H⁺-band waves is larger than that of He⁺-band waves only when L?<?4.5 and AE¹?<?300?nT, and He⁺-band emissions are more intense under all other conditions. In contrast to 5 events that have average H⁺-band amplitude over 2 nT, 19 events exhibit >2 nT He⁺-band amplitude, indicating that the He⁺-band waves can be more easily amplified than the H⁺-band waves under the same circumstances. For simultaneous occurrences of the two EMIC wave bands, their frequencies vary with L-shell and geomagnetic activity: the peak wave frequency of H⁺-band emissions varies between 0.25 and 0.8 f_cp with the average between 0.25 and 0.6 f_cp, while that of He⁺-band emissions varies between 0.03 and 0.23 f_cp with the average between 0.05 and 0.15 f_cp. These newly observed occurrence features of simultaneous H⁺- and He⁺-band EMIC emissions provide improved information to quantify the overall contribution of multi-band EMIC waves to the loss processes of radiation belt electrons.     

Detection of the quantity of kinesin and microgravity-sensitive kinesin genes in rat bone marrow stromal cells grown in a simulated microgravity environment

Kinesin and kinesin-like proteins (KLPs) constitute a superfamily of microtubule motor proteins found in all eukaryotic organisms. Members of the kinesin superfamily are known to play important roles in many fundamental cellular and developmental processes. To date, few published studies have reported on the effects of microgravity on kinesin expression. In this paper, we describe the expression pattern and microgravity-sensitive genes of kinesin in rat bone marrow stromal cells cultured in a ground-based rotating bioreactor. The quantity of kinesin under the clinorotation condition was examined by immunoblot analysis with anti-kinesin. Furthermore, the distribution of kinesin at various times during clinorotation was determined by dual immunostaining, using anti-kinesin monoclonal antibody or anti-β-tubulin monoclonal antibody. In terms of kinesin quantity, we found that the ratios of the amounts of clinorotated/stationary KLPs decreased from clinorotation day 5 to day 10, although it increased on days 2 and 3. Immunofluorescence analysis revealed that kinesin in the nucleus was the first to be affected by simulated microgravity, following the kinesin at the periphery that was affected at various times during clinorotation. Real-time RT-PCR analysis of kinesin mRNA expression was performed and led to the identification of 3 microgravity-sensitive kinesin genes: KIF9, KIFC1, and KIF21A. Our results suggest that kinesin has a distinct expression pattern, and the identification of microgravity-sensitive kinesin genes offers insight into fundamental cell biology.