单推三分析化验误差来源研究

单推三分析化验误差来源是多方面的,确定单推三分析过程误差来源,能为操作人员提供减少或消除误差的依据。影响单推三分析结果的主要因素有几个:标准溶液浓度的变化,滴定过程各终点的读数,环境温度的变化。在分析化验过程中,第一终点读数对硝酸肼、氨的分析结果不产生影响,但对肼有影响;第二终点读数对肼、氨分析结果有影响,但对硝酸肼无影响;第三终点读数对上述三种物质的分析结果都有影响,尤其是硝酸肼,其分析化验结果很容易超出要求范围。     

Summary of the workshop on gamma-ray burst afterglows at the 34th COSPAR meeting

A summary is given of the presentations at the COSPAR workshop on γ-ray bursts with some personal commentary on the contributions, the SN/GRB connection, and on the role of magnetic fields in γ-ray bursts and their afterglows. Of special interest were the accumulated arguments for strong collimation and associated reduction in the total required energy for γ-ray bursts. Significant discussion was also devoted to the issues associated with iron and metal lines in X-ray spectra. It is important to note that some of the afterglows seem to require ambient densities 1 g cm⁻³, rather incompatible with a massive star environment. Of associated difficulty is the fact that few, if any, afterglows seem consistent with the r⁻² wind expected for a massive star model. There are reasons to think that if γ-ray bursts are associated with supernovae they are of Type Ic. This suggests that any wind present might be rich in carbon and oxygen, not hydrogen or helium. If γ-ray bursts are narrowly collimated, then the burst is only probing a small portion of any wind, perhaps just that time-dependent and isotropic structure directly along the rotation axis. The characteristics of “hypernovae” may be the result of orientation effects in a mildly inhomogeneous set of progenitors, rather than requiring an excessive total energy or luminosity. The recent event GRB 021004 provided a rich photometric and spectroscopic record and perhaps the most direct evidence yet for the association of a specific γ-ray burst with a massive star progenitor. If the magnetic field plays a significant role in launching a relativistic γ-ray burst jet from within a collapsing star, then the magnetic field may also play a role in the propagation, collimation, and stability of that jet within and beyond the star. The magneto-rotational instability (MRI) can operate under conditions of moderate rotation. This means that the MRI will be at work generating strong fields exponentially rapidly even as the disk of material begins to form and makes a transition from a non-Keplerian to quasi-Keplerian flow in the collapsar and related models.     

Microstructure and Mechanical Properties of Cross-rolled Ti_(50)Ni_(47)Fe_3 Shape Memory Alloy

The microstructures, the phase transformation characteristics, and the mechanical properties of the Ti50Ni47Fe3 alloy in as-forged and as-cross-rolled states were investigated. It is found that, after cross-rolling, the phase transformation temperature (Ms) of the alloy decreases drastically and the grains get refined. Moreover, its yield strength and fracture strength after cross-rolling hit 540 MPa and 687 MPa respectively, up by about 200 MPa over those in as-forged state.     

轴类零件三维尺寸自动标注算法

针对尺寸自动标注仅限于表达产品的几何信息而未关注其功能特性,从而导致所标注的尺寸无法恰当地描述产品设计意图的问题,提出一种基于产品功能特性的三维尺寸自动标注算法.首先,根据零件的功能构造了尺寸标注基准集;其次,建立了轴向尺寸标注优先级确定准则,构造轴向尺寸集,并采用图论法消除了尺寸冗余;然后,构建径向尺寸集,并采用尺寸冗余度法删除其中的冗余尺寸;最后,通过实例测试,验证了所提算法的可行性和有效性.     

空间机械臂视觉相机内参标定技术研究

针对空间机械臂视觉相机的任务需求与配置,内参标定技术是相机高精度获取合作目标位置、方向等运动信息的首要前提和重要保障。文章设计了一种基于二维平面靶的机械臂相机内参标定方法,用于解算焦距、主点坐标、畸变系数等。首先,利用相机拍摄多幅平面靶图像,求解平面靶与相机图像之间的映射矩阵;其次,构建相机内参约束方程;再次,利用特征值分解,解算焦距、主点坐标等参数值;最后,引入径向、切向畸变构建非线性模型,将解得的内参作为初值,利用Levenberg-Marquardt优化算法即可计算出相机内参最优解。试验结果表明,该方法完全适用于机械臂相机内参标定,标定结果均满足机械臂视觉相机获取合作目标三维位姿的测量精度要求。     

载人航天器密封舱内生物剂量三维仿真技术

对载人航天器密封舱内航天员遭受的生物剂量进行研究分析,可为乘员辐射防护设计和工程实施提供依据。文章将基于一维深度-剂量计算、结合扇区射线法的三维辐射仿真技术运用于载人航天器总体设计中,以某中期驻留载人航天器为例,构建生物剂量仿真分析模型。计算实例分析表明,三维剂量仿真结果可有效指导乘员辐射防护优化设计,对后续长期载人飞行中的航天员辐射安全设计具有较强的实用性。     

二元超声速进气道流管压缩量特性与应用初步研究

为研究流管压缩程度与超声速进气道临界总压恢复系数的规律,以双楔外压式进气道为例,对不同来流马赫数、多种方案进行实例研究。研究马赫数范围为2.0至4.0,各种压缩方案涉及宽泛的总转折角范围和多种楔角组合方式。研究结果表明,就通常设计中常用的压缩方案范围而言,临界总压恢复系数与流管收缩比呈明显的正相关变化规律,并在一定的范围内两者呈近似线性关系,基于流管收缩比可实现对临界总压恢复系数大小的近似判断。      

基于动量轮转速标定的轨道控制方法研究

某地球同步三轴卫星因故障导致推力器工作效率不稳定,使得采用原有方案进行向西轨道控制时姿态变化大,控制准确度降低.针对上述问题,通过分析卫星用于姿态控制的偏置动量轮的控制规律,利用星体角动量守恒条件,建立了偏置动量轮转速变化与轨道半长轴变化之间的相关性数学模型,提出了一种改进的基于偏置动量轮转速标定的轨道控制方法,同时结合姿态的稳定变化制定了轨道控制实施方案,并将其应用于实际卫星轨道控制中,取得了良好的控制效果.改进的控制方法提高了轨道控制的准确率,使得半长轴误差幅度由最大60％提高到0.2％左右,增加了姿态的稳定性,使得俯仰姿态变化幅度由最大0.7°减小到0.2°左右,降低了控制风险,减轻了地面控制人员的负担.     

U形渠道机翼形量水槽水跃数值模拟与试验研究

量水槽是灌区常见的特设量水设备,而槽后水力特性是判断其选型是否合理的重要指标之一。以某小型灌区末级灌溉渠系改造工程为原型,针对两种不同工况,采用基于TruVOF方法跟踪自由液面、Favor技术实现网格优化的湍流数学模型,对U形渠道机翼形量水槽水跃问题进行三维数值模拟,分析了水跃的时均流场、共轭水深、发生位置、跃长、断面流速分布以及水跃段能量损失等相关水力特性。采用与原型1：1比尺的水工模型试验资料对模拟结果进行验证,结果表明,二者吻合较好。通过对实测与数值仿真的共轭水深数据进行统计分析,得到了适用于U形渠道机翼形量水槽水跃共轭水深的近似计算公式。研究结果对机翼形量水槽在平原缓坡灌区末级渠系的应用研究提供了一定的参考和建议。     

一种航路4D航迹预测的方法

4D航迹预测是空管自动化系统中的一项核心技术,能够提高空域的利用率和安全性。为了在航路上快速准确的预测航空器的飞行轨迹,提出一种预测航路4D航迹的方法。首先利用Supermap制作航路网络,然后根据航空器的性能参数,推测各时间点的航空器位置,从而得到航路上航空器的飞行航迹,并通过实例进行了说明,为航迹预测提供一定参考。