近红外光谱测定NEPE胶组分含量

研究了近红外光谱测定NEPE胶中硝化甘油、丁三醇三硝酸酯、聚乙二醇含量的方法,采用相关系数、显变分析、间隔偏最小二乘法、遗传算法等方法选择波长,对相关实验条件和影响因素进行了研究.实验结果表明,数据平移处理可以有效改善样品吸光度与浓度之间的相关性;遗传算法选择波长优于相关系数法和间隔偏最小二乘法,显变分析不适合于本项研究;近红外光谱法快速测定NEPE胶组分含量的结果与标准分析方法的测定结果一致,两者相差小于1%;水分含量的变化、正常加热操作对NEPE胶组分含量测定的影响不明显.     

Broad spectral line and continuum variabilities in QSO spectra induced by microlensing of diffusive massive substructure

We investigate the variability of the continuum and broad lines in QSO spectra (particularly in the Hβ line and continuum at λ 5100 Å) caused by microlensing of a diffuse massive structure (like an open star cluster). We modeled the continuum and line emitting region and simulate a lensing event by a star cluster located in an intervening galaxy. Such a type of microlensing event can have a significant influence on magnification and centroid shift of the broad lines and continuum source. We explore relationships between the continuum and broad line flux variability during the microlensing event.     

A simplified approach to uncertainty quantification for orbits in impulsive deflection scenarios

For the majority of near-Earth Asteroid (NEA) impact scenarios, optimal deflection strategies use a massive impactor or a nuclear explosive, either of which produce an impulsive change to the orbit of the object. However, uncertainties regarding the object composition and the efficiency of the deflection event lead to a non-negligible uncertainty in the deflection delta-velocity. Propagating this uncertainty through the resulting orbit will create a positional uncertainty envelope at the original impact epoch. We calculate a simplified analytic evolution for impulsively deflected NEAs and perform a full propagation of uncertainties that is nonlinear in the deflection delta-velocity vector. This provides an understanding of both the optimal deflection velocities needed for a given scenario, as well as the resulting positional uncertainty and corresponding residual impact probability. Confidence of a successful deflection attempt as a function of launch opportunities is also discussed for a specific case.     

月球电离层掩星探测研究

日本SELENE/KAGUYA探测任务提供了研究月球电离层的机会。采用无线电掩星探测技术和趋势外推算法,消除地球电离层和行星际等离子体的干扰影响,残余的信号相位信息的变化反映了月球电离层的信息,估算出月球周围附近近似对称分布的稀薄电离层中电子总含量(TEC)约为每立方米10-14个。     

三角带较大功率增速传动的可行性研究

三角带传动具有结构简单，制造维修方便，过载保护等优点，一般用来实现减速传动，只有当传送的功率较小时，才用来实现增速传动，在工程实际应用中，常常遇到功率较大时需要传送较大功率时，能否利用三角带实现增速传动的问题，然后介绍了三角带增速传动的功率损失以及普通三角带和特种三角带的区别。在此基础上提出利用特种三角带实现较大功率增速传动的可行性，最后阐述了三角带增速传动的计算准则及步骤，对较大。     

星敏感器调焦方法研究

调焦是星敏感器产品设计生产的一个关键环节.精确的调焦可以提高星敏感器的灵敏度和测量精度,保证星敏感器的性能指标.从焦点位置、光轴与芯片法线不重合、芯片安装精确度、质心稳定性等方面分析了影响调焦的各种因素,总结出调焦方法.     

某型机化铣零件成形工艺

化铣是一种能使表面形状复杂、加工精度要求高的零件达到加工要求的表面处理方法。铝合金的化学铣切已经成为航空工业零件成形的可靠加工方法,尤其是在加工飞机蒙皮时要比用传统的机械加工方法优越得多。本文对某型机零件表面出现锤痕现象进行了技术分析,发现其锤痕原因是由于成形零件用榔头校形而造成。同时,提出了采用钣金"一步成形法"即在淬火时效期内进行零件成形后再化铣的工艺方法。     

置氢对TC21合金粉末物理性能和压制性能的影响

采用扫描电镜观察、粉末镶嵌试样、XRD和模压成形等方法,研究了置氢(H,wt%)对TC21合金粉末颗粒形貌、表面状态、显微组织、相组成、显微硬度和压制性能等的影响.结果表明:置氢TC21粉末颗粒形貌为不规则状,粉末主要由亮相α相及暗相β相组成,颗粒显微组织呈片状、α/β集束状和网篮状.随置氢量的增加,置氢TC21粉末显微硬度呈降低趋势;α相逐渐减少,β相逐渐增多,并且有少量的α"相生成;粉末的压缩性能呈先变差后变好的不明显变化趋势,成形性能先变差又逐渐变好,置氢量0.10 wt%,0.39 wt%TC21粉末压制性能较好,置氢量0.22 wt%的TC21粉末的压制性能最差.