Dy对EB-PVDβ-NiAl涂层高温瞬态氧化行为的影响(英文)

β-NiAl是一种有前景的应用于1150°C以上的抗氧化涂层材料。本文利用电子束物理气相沉积(EB-PVD)方法制备了0~0.5at%Dy含量的β-NiAl涂层,研究了涂层的瞬态氧化行为。1200°C时,在0.05at%Dy掺杂的涂层中只观察到了稳态α-Al2O3相,而在0.5at%Dy掺杂的涂层中,1h氧化过程中,发生了θ-Al2O3到α-Al2O3的相变。1100°C时,在最初的15min所有涂层均发生了θ-α相变。0.05at%Dy掺杂的涂层在45min的时候相变已经完成,这比0.5at%Dy掺杂涂层要早得多。过量Dy的掺杂能够延缓θ-α相变。未掺杂和过量掺杂涂层在20h氧化之后仍存在针状相θ-Al2O3,而0.05at%Dy掺杂的涂层中则为经典的颗粒状α-Al2O3形貌。     

Regeneration of organs and tissues in lower vertebrates during and after space flight.

In this paper most important data obtained in studies on the effect of space flight conditions on regeneration in the adult newt are summarized. We demonstrate a phenomenon of synchronization of limb and lens regeneration and increase in its rate during and after space flight. We also describe a peculiarities of cell proliferation in lens, limb and tail regenerates and of the process of minced muscle regeneration.     

论高校医院与全科医学

摘 要 保证高校教职工、大学生的身心健康，是高校医院义不容辞的责任。为此，应探索一条更适合高校实际情况的医疗模式。本文就高校医院应如何为师生员工提供全方位的医疗保健服务进行了初步探讨。     

近代烃类转化用换热转化器的开发与应用

汇集国内外开发的新型换热转化器(亦称转化炉)的设计形式和结构特征,可供老厂节气节能挖潜技术改造或新建装置优选和参考。     

顾及星像点分布的恒星相机在轨检校

由于卫星发射前后以及在轨运行过程中,环境因素的变化都可能引起恒星相机参数发生改变,从而导致星敏感器姿态测量精度下降.将多片空间后方交会方法应用于恒星相机的在轨检校.在利用该方法检校时,实验发现检校结果的精度受到参与检校的恒星影像上星像点分布的影响,由此进一步提出了凸包面积百分比准则,该方法自动选取分布较好的影像用于检校,有助于提高检校精度.实验结果证明:基于后方交会进行恒星相机在轨检校时,利用凸包法选取的影像片进行检校的精度明显优于未选片时检校的结果.      

Safety Analysis of Flow Parameters in a Rotor-stator Cavity

In order to ensure the safety of engine life limited parts (ELLP) according to airworthiness regulations, a numerical approach integrating one-way fluid structure interaction (FSI) and probabilistic risk assessment (PRA) is developed, by which the variation of flow parameters in a rotor-stator cavity on the safety of gas turbine disks is investigated. The results indicate that the flow parameters affect the probability of fracture of a gas turbine disk since they can change the distribution of stress and temperature of the disk. The failure probability of the disk rises with increasing rotation Reynolds number and Chebyshev number, but descends with increasing inlet Reynolds number. In addition, a sampling based sensitivity analysis with finite difference method is conducted to determine the sensitivities of the safety with respect to the flow parameters. The sensitivity estimates show that the rotation Reynolds number is the dominant variable in safety analysis of a rotor-stator cavity among the flow parameters.     

基于等高线图与小波变换的3D地形匹配算法研究

提出一种新的基于边缘的3D地形匹配算法。在算法中，一种结构紧凑的特征“等高线图”，用于表示参考高程图(DEM)及从实时数据恢复的高程图，这样3D地形匹配转化为基于等高线的匹配，即边缘(平面曲线)匹配问题。在边缘匹配过程中，首先用一种具有平移，旋转，尺度不变性的规范化小波描述子描述边缘。其次提出了一种基于小波系数域的快速边缘匹配算法，并分析了运算复杂性。由匹配成功的边缘对提取控制点的坐标。讨论了图像变换模型及基于最小均方根误差准则的图像变换参数估计方法。用真实地形实验表明该算法匹配精度高，计算速度快。最显著的特点是该算法抗噪声能力强。     

一种快速有效的雷达目标识别方法

基于核的学习算法提出一种快速有效的雷达目标识别方法。首先利用核的主分量分析方法对雷达目标的一维距离像进行特征提取,可以有效地提取出其中的非线性特征;然后基于一种新型的支撑矢量机——近似支撑矢量机作为分类器对所提取的特征进行识别。实验结果表明,所提出的识别方法其正确识别率与标准支撑矢量机相当,但在计算速度上却有很大的提高,并对噪声具有较好的抑制作用。     

Dark matter search with the CALET detector on-board ISS

The CALorimetric Electron Telescope, CALET, mission is proposed for the observation of high-energy electrons and gamma-rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe the electrons (without separation between e⁺ and e⁻) in 1 GeV–10 TeV and the gamma-rays in 20 MeV–several TeV with a high-energy resolution of 2% at 100 GeV, a good angular resolution of 0.06 degree at 100 GeV, and a high proton-rejection power of nearly 10⁶. The CALET has a geometrical factor of 1 m²sr, and the observation period is expected for more than three years. The very precise measurement of electrons enables us to detect a distinctive feature in the energy spectrum caused from WIMP dark matter in the Galactic halo. The excellent energy resolution of CALET, which is much better than GLAST or air Cherenkov telescopes over 10 GeV, enables us to detect gamma-ray lines in the sub-TeV region from WIMP dark matter annihilations. The CALET has, therefore, a unique capability to search for WIMP dark matter by the hybrid observations of electrons and gamma-rays.     

Near-Equatorial Electrons as Measured onboard the MirSpace Station

Some results of studying the electrons with energies of tens to hundreds of keV at the low and near- equatorial geomagnetic latitudes by using the instruments Sprut-V and Ryabina-2 onboard the Mirspace station in 1991 are presented. It is found that at L< 1.2 the enhanced electron fluxes are sporadically detected, being localized within three longitudinal intervals, 180° W–0°–15° E, 90°– 120° E, and 160° E–180°–135° W. The most intense electron fluxes are observed at the lower edge of the near-equatorial boundary of the inner radiation belt on longitudes of the South Atlantic Anomaly between 14 and 20 h MLT. The occurrence of electron bursts does not depend on the geomagnetic disturbance level. A hardening of the electron spectra is observed near the geomagnetic equator. At L< 1.1, the more energetic particles are located closer to the geomagnetic equator. The results are compared with the data on the low-frequency waves and fields at low and near-equatorial latitudes obtained by the Ariel-4and San Marco Dsatellites, as well as by the spacecraft and ground-based observations of the thunderstorm global distribution. The thunderstorms are considered as a possible source of electron production near the geomagnetic equator.