基于旋转多圆柱的冰风洞水滴参数分析方法

阐述了基于旋转多圆柱测量仪的冰风洞水滴参数分析方法.对二维圆柱的水滴撞击特性进行了计算分析;对二维旋转圆柱的霜状冰结冰过程进行了数值模拟;根据水滴参数对旋转圆柱结冰量的影响, 结合数学逼近的方法, 编制了由旋转多圆柱测量结果分析计算冰风洞水滴参数的软件, 最后用国外试验数据对软件分析结果进行了验证, 结果表明:计算方法正确, 可以实现冰风洞水滴参数快速测量.      

基于曲面主方向的正交系的非完整基理论及其在流体力学中的相关应用

本文将微分几何中光滑曲面上局部存在的基于主方向的正交系联系于张量分析中的非完整基理论,以此为曲面与其邻域上的张量场场论提供了一种新方法,称为基于曲面主方向的正交系的非完整基理论。这种场论方法,基于基面的沿主方向的参数坐标,然后沿基面的法方向进行空间延拓,以此获得基面邻域内的完整的正交系。对此引入非完整基理论,可得所有的非零Christoffel符号直接对应为基面或者当地曲面的主曲率或者测地曲率,因而张量场的各种微分算子相对于曲面的主方向与法方向展开,所得分量表达式仅含物理量与曲面曲率。由此不仅可以清晰地展现曲面几何特征与物理量/物理过程之间的关系,而且所获得的分量表达式形式上最为简单。另一方面,经典的诸如柱坐标系、球坐标系等正交系也隶属基于曲面主方向的正交系,从而本文方法可以统一相关正交系下的张量场场论。作为应用,本文推导了可变形曲面上涡量、涡量法向梯度与变形率张量的表达式,曲面上流体边界层方程的分量方程,曲面介质相关守恒律方程等。     

中低轨红外预警星座基于自由段跟踪的单星覆盖性能

推导了中低轨天基红外星座中单颗卫星基于自由段跟踪时的空域覆盖体积与星下黑体积,研究了其随轨道高度变化的规律,分析了存在切地角影响时的体积变化,并进行了计算。     

Magnetogasdynamic shock wave generated by a moving piston in a rotational axisymmetric isothermal flow of perfect gas with variable density

The propagation of a strong cylindrical shock wave in an ideal gas with azimuthal magnetic field, and with or without axisymmetric rotational effects, is investigated. The shock wave is driven out by a piston moving with time according to power law. The ambient medium is assumed to have radial, axial and azimuthal component of fluid velocities. The fluid velocities, the initial density and the initial magnetic field of the ambient medium are assumed to be varying and obey power laws. Solutions are obtained, when the flow between the shock and the piston is isothermal. The gas is assumed to have infinite electrical conductivity and the angular velocity of the ambient medium is assumed to be decreasing as the distance from the axis increases. It is expected that such an angular velocity may occur in the atmospheres of rotating planets and stars. The shock wave moves with variable velocity and the total energy of the wave is non-constant. The effects of variation of the initial density and the Alfven-Mach number on the flow-field are obtained. A comparison is also made between rotating and non-rotating cases.     

Filtration of Interstellar Atoms through the Heliospheric Interface

Interstellar atoms penetrate deep into the heliosphere after passing through the heliospheric interface—the region of the interaction of the solar wind with the interstellar medium. The heliospheric interface serves as a filter for the interstellar atoms of hydrogen and oxygen, and, to a lesser extent, nitrogen, due to their coupling with interstellar and heliospheric plasmas by charge exchange and electron impact ionization. The filtration has great importance for the determination of local interstellar abundances of these elements, which becomes now possible due to measurements of interstellar pickup by Ulysses and ACE, and anomalous cosmic rays by Voyagers, Ulysses, ACE, SAMPEX and Wind. The filtration of the different elements depends on the level of their coupling with the plasma in the interaction region. The recent studies of the filtration of the interstellar atoms in the heliospheric interface region is reviewed in this paper. The dependence of the filtration on the local interstellar proton and H atom number densities is discussed and the roles of the charge exchange and electron impact ionization on the filtration are evaluated. The influence of electron temperature in the inner heliosheath on the filtration process is discussed as well. Using the filtration coefficients obtained from the modeling and SWICS/Ulysses pickup ion measurements, the local interstellar abundances of the considered elements are determined.     

Revealing the hot intergalactic medium with ROSAT

The X-ray background intensity around galaxies and rich clusters of galaxies is investigated in three energy bands using the ROSAT All-Sky Survey maps. It is found that an amplitude of the XRB enhancements surrounding the Abell clusters and high density areas in the Lick galaxy counts depends on photon energy. Excess flux generated in the surrounding of the galaxy concentrations is consistent with the thermal emission by hot gas postulated by hydrodynamic simulations.     

微阴极电弧推力器工作性能影响因素研究

采用试验方法研究了微阴极电弧推力器中峰值放电电流及外加磁场对其推力、比冲、寿命的影响规律。试验结果表明:峰值放电电流增加,阴极烧蚀量增加,元冲量增大;相比于较低的峰值放电电流(10A),更高的峰值放电电流(40A)可延长推力器的工作寿命;外加磁场增强,推力器喷射等离子体轴向速度增大,比冲增加。     

“四横四纵”工作体系——论如何做好高职高专院校新生共青团工作

高校共青团组织作为高校学生工作的有机组成部分,在团结青年、教育青年、服务青年方面有着重要且不可替代的作用。切实做好高校共青团工作,需要增强工作理念创新,加强团组织体系和职能建设,全面布局,突出重点,提升影响力,充分发挥好团组织对学校各项工作的辅助作用。     

中碳钢管焊接热裂纹产生的原因及对策

中碳钢总体来说焊接性差，若焊材的选择不当或工艺处理不当都会导致焊接热裂纹的出现，热裂纹的产生主要与焊材或母材中碳、硫、磷含量过高有关，与焊接工艺方法也有一定关系。为避免热裂纹的出现，必须制订合理的焊接工艺，减少碳、硫、磷有害合金元素溶人焊缝，采用抗裂性好的碱性焊条或TIG焊接及适当的工艺措施等，对解决热裂纹有重要的意义。     

中介关系数据库查询语言

给出了中介关系数据模型,在此基础上构造了两类不同的中介关系数据库查询语言,中介关系演算和中介关系代数,中介关系演算以中介谓词演算ＭＦ为基础,通过引入直值程度词〈对立否定词和模糊否定词～扩充了关系演算的表达能力,同样地,中介关系代数以中介集合论ＭＳ为基础,扩充了关系代数的功能,此外,证明了中介关系演算和中介关系代数的语言表达能力上的等价性,中介关系演算和中介关系代数可作为研究模糊数据库理论的工具。