两种间接三维测试技术在航天领域的应用

针对航天领域实际生产中存在的被测对象,提出了两种间接式三维测量方法。即基于视觉技术的测量方法和基于经纬仪技术的测量方法,并分析了它们各自的关键技术。这两种方法针对其各自不同的测量对象能有效地实现大尺寸的空间三维测量。     

Hg_(1-x)Cd_xTe 中杂质对及双空位深能级的研究

以A.Kobayashi等的半经验紧束缚模型和Hjalmarson-Vogh-Wolford-Dow深能级理论为基础,计算了Hg1-xCdxTe中阳离子位替代式杂质（包括N,O,C）与最近邻替代式杂质形成sp3键杂质对后阳离子位杂质A1对称性深能级的变化以及最近邻理想双空位（Vc,Va）的深能级。计算结果表明：阳离子位杂质A1能级的变化取决于与其配对杂质的电负性,杂质对a1能级组分依赖关系dE/dx小于阳离子位单杂质A1能级的dE/dx,大于阴离子位单杂质T2能级的dE/dx,不同杂质对的dE/dx基本相同;理想双空位（Vc,Va）在能隙或近能隙区域产生一个a1态深能级,该能级的dE/dx很小,对于CdTe,位置在0.5eV,对于x<0.37的Hg1-xCdxTe,该能级成为导带共振态。     

3,6-双(1-氢-1,2,3,4-四唑-5-氨基)-1,2,4,5-四嗪-1,4-丁二胺盐的制备和热分解动力学及热安全性

利用3,6-双(1-氢-1,2,3,4-四唑-5-氨基)-1,2,4,5-四嗪(BTATz)和1,4-丁二胺,在DMSO中合成出了标题化合物。采用元素分析和红外光谱分析,测定了其结构。用DSC和TG/DTG热分析仪,对标题化合物进行了热分解行为及热分解动力学研究。结果表明,化合物的热分解过程只有一个放热阶段,该阶段的非等温热分解反应动力学方程的活化能和指前因子分别为92.95 kJ/mol和1016.58s-1。采用MicroDSCⅢ量热仪中的连续比定压热容测定模式,测定了化合物的比定压热容,比定压热容随温度呈现二次方关系,且298.15 K下的标准摩尔热容为443.22 J/(mol.K)。计算得到化合物的自加速分解温度(TSADT)、热爆炸临界温度(Tb)和绝热至爆时间分别为521.55、536.73 K和36.97 s。     

X-ray study of accretion flow in narrow-line Seyfert 1 galaxies

We present the results of a systematic study of narrow-line Seyfert 1 galaxies (NLS1s) observed with XMM-Newton. The 2–12 keV X-ray spectra of NLS1s are well represented by a single power law with a photon index Γ ∼ 2. When this hard power law continuum is extrapolated into the low energy band, we found that all objects in our sample show prominent soft excess emission. This excess emission is well parameterized by the thermal emission expected from an optically thick accretion disk, and we found the following three peculiar features: (1) The derived disk temperatures are significantly higher than the expectation from a standard Shakura-Sunyaev accretion disk, if we assume a central mass of a black hole to be 10^6–8M_⊙. (2) The temperatures are distributed within narrow range (ΔkT ∼ 0.08 keV) with an average temperature of 0.18 keV in spite of the range of four orders of magnitude in luminosity (10^41–45 erg s⁻¹). (3) We found a peculiar temperature–luminosity relation, where the luminosity seems to be almost saturated in spite of the significant change in temperature, during the observations of the most luminous NLS1 PKS 0558-504. These results strongly suggest that the standard accretion disk picture is no longer appropriate in the nuclei of NLS1s. We discuss a possible origin for the soft excess component, and suggest that a slim disk may be able to explain the observational results, if the photon trapping effect is properly taken into account.     

T-250转塔式加工中心数控系统的设计

简要论述了开放式数控系统的概念，并在华中Ⅰ型开放式数控系统的开放平台上，对T-250转塔式加工中心数控系统进行了设计。     

税收流失的治理对策

税收流失的治理一直是世界性的大难题，并为国际社会广泛关注。因此，世界各国无不采取各种措施减少税收流失，对税收流失行为进行惩罚。通过对税收的作用与流失原因的分析，看到治理税收流失是全方位、全社会的，而不是局部的，需要从法制、征管、税制、体制、监督和宣传等方面、多视角系统研究税收流失的治理对策。     

数控滚齿机及其编程

分析了数控滚齿机的种类及工作特点，并结合实际生产需要，重点介绍了数控滚齿机的编程方法及特点，为操作者与同行提供了一些有益的帮助。     

CFM56-5B 发动机VBV故障引起的EGT超温故障分析

从可变放气活门系统(VBV)的组成和工作原理入手,通过对系统部件和关联部件工作分析,结合维护过程的故障历史,指出了故障的排除方法和维护提示.     

Ion relaxation processes in the heliospheric interface: how perturbed are ion distribution functions?

Charge-exchange processes between interstellar H-/O-atoms and protons of the bulk of the interstellar plasma flow downstream of the outer bowshock in the heliospheric interface induce secondary ions leading to non-relaxated velocity distribution functions. The relaxation of these freshly induced ions towards an equilibrium distribution occurs due to Coulomb interactions and wave–particle interactions with the background turbulence. Since Coulomb interactions are of low relevance, we study here in detail the effect of wave–particle interactions. To find the turbulence levels in the interface we consider the MHD-wave transformation at the outer shock surface between the interface and the local interstellar plasma. The turbulence in the outer interface region is shown to be dominated by incompressible Alfvén waves both for cases of quasiparallel and quasiperpendicular shocks. Also we show that waves propagating towards the shock are more intensive than those propagating away from it. The level of Alfvén turbulence in the interface is estimated using the recent data on local interstellar turbulence deduced from observations of interstellar scintillations of distant radiosources. Two proton relaxation processes are considered: quasilinear resonant interactions with Alfvén waves and non-linear self-induced wave–particle scattering. The corresponding diffusion coefficients are estimated, and typical time periods for protons and oxygen ions relaxation are shown to be of the same order of magnitude as H-/O-atoms passage time over the extent of the interface. This indicates that perturbed ion distribution functions must be expected there.     

航空发动机承力系统试验建模技术研究

通过建立航空发动机整机振动分析模型,对试验与理论相结合的建模技术进行了研究,提出了试验建模的具体算法,并进行了精度分析。