MgO衬底NbN/AlN/NbN多层膜的制备

本文主要讨论磁控溅射设备制备的NbN/AlN/NbN三层结构的技术工艺,为制备All-NbN的 NbN/AlN/NbN SIS 隧道结作准备.我们在室温下利用直流磁控溅射工艺制备了单晶NbN薄膜,并对其超导电性做了初步的研究;又利用射频磁控溅射工艺制备了取向较好的AlN薄膜.我们利用磁控溅射方法制作NbN/AlN/NbN多层薄膜,然后对制备SIS隧道结进行了一些探索.     

Star Formation in Molecular Cloud Associated with IRAS 07028-1100

The first mapping observations in 12^CO J=2-1 and 12^CO J=1-0 lines were made towards molecular cloud associated with IRAS 07028-1100. The results show a mono-polar outflow (primarily blueshifted component) near IRAS 07028-1100, which suggests that star formation is occurring in this region. On the basis of the MSX (Midcourse Space Experiment) band-A image, molecular cloud core contours, NVSS data and IRAS data, we identify IRAS 07028-1100 as an embedded young intermediate-mass star. According to the 2MASS data, we suggest a sequential star formation in the infrared cluster associated with IRAS 07028-1100.     

300GHz超导SIS接收机系统的设计与构建

超导SIS(Superconductor-Insulator-Superconductor)混频技术是新兴的低噪声检测技术.其卓越的低噪声性能已使其成为毫米波和亚毫米波频段灵敏度最高的谱线接收设备,接收机的自动控制和稳定性有更高的要求,研制能够长期稳定工作的接收机有很重要的意义.本文主要讨论了我们自行研究设计工作在4K温度,准光学系统的毫米波超导SIS接收机的组成部件,根据我们制备的超导SIS隧道结器件的特性指标,计算设计了300GHz波段的超导接收机天线和结的集成芯片.     

Statistical analysis of Fe abundances gradients in the Galaxy

Using the high precision data of the proper motions and parallaxes from Hipparcos catalogue, we obtained the orbital parameters of 1302 stars in the Galaxy based on the mass distribution model provided by Allen and Santillón. Fe abundances of 1295 stars among our samples were analyzed. With the correlation analyses between [Fe/H] and orbital parameters, we obtained that the Fe gradient is - 0.057 ± 0.007 dex/kpc along the direction of the maximum galactocentric distance (hereafter DG_max) in the range of 8.5 kpc < DG_max < 17 kpc. We also got the result that the vertical gradient is steeper than the radial gradient. Furthermore, we divided the samples into two subgroups: giants and dwarfs; F, G and K stars; and then analyzed them respectively. Our results show that the gradient becomes flatter and flatter from giants to dwarfs, from F type to G and K type stars. We also divided the samples into disk and halo stars using maximum vertical distance Z_max = 1 kpc as the criterion and got the result that the abundances of the disk stars are much higher than that of the halo stars. Our work suggests the existence of the galactic gradient and supports those chemlcal evolution medels which show that the halo was formed before the disk at the early stage of the Galaxy.     

MgO(111)上NbN和AlN薄膜的生长研究

在制备NbN/AlN/NbN隧道结的工艺过程中,为了获得具有优质单晶结构的NbN薄膜,我们在MgO(111)基片上探索了直流溅射法制备NbN薄膜的生长工艺条件,XRD研究分析表明,我们获得了单晶结构良好的NbN薄膜;为了支持作为上电极的NbN薄膜的生长,也需要良好的AlN薄膜用作势垒层,我们采用射频磁控溅射设备和纯净的Al靶对AlN薄膜进行了制备研究.实验结果表明,所获得的AlN薄膜具有六方c-轴取向,并讨论了衬底和薄膜界面处可能的结构情况.     

Mutual recombination in slow Si^＋ ＋ H^- collisions

This paper studies the process of mutual neutralization of Si^＋ and H^- ions in slow collisions within the multichannel Landau-Zener model. All important ionic-covalent couplings in this collision system are included in the collision dynamics. The cross sections for population of specific final states of product Si atom are calculated in the CM energy range 0.05 e∨/u-5 ke∨/u. Both singlet and triplet states are considered. At collision energies below -10 e∨/u, the most populated singlet state is Si（3p4p, ^1S0）, while for energies above -150e∨/u it is the Si（3p, 4p, ^1P1） state. In the case of triplet states, the mixed 3p4p（^3S1 ＋^3P0） states are the most populated in the entire collision energy range investigated. The total cross section exhibits a broad maximum around 200 300e∨/u and for ECM ≤ 10e∨/u it monotonically increases with decreasing the collision energy, reaching a value of 8 × 10^-13 cm^2 at ECM = 0.05 e∨/u. The ion-pair formation process in Si（3p^2 ^3PJ）＋H（1s） collisions has also been considered and its cross section in the considered energy range is very small （smaller than 10^-20 cm^2 in the energy region below 1 ke∨/u）.     

舰船装备可靠性工程中的几个重要模型特点分析

可靠性是舰船装备的重要质量特性，是影响装备作战效能及其寿命周期费用的主要因素。对舰船装备可靠性工程中的故障模式影响和危害度分析模型、故障树分析模型、舰队保障库存大纲模型、老虎模型、以可用性为中心的库存模型、以战备完好性为基础的备件配置法模型进行了分析。这些模型在目前舰船装备的可靠性工程中具有重要的地位，对装备的战备完好性和任务成功性则是一个基本的分析评估手段。     

Magnetic Fields in Active Late—Type Stars

The very high resolution and high signal-to-noise ratio spectra of ten x-ray selected stars are obtained by the NAOC Coude spectropraph.Magnetic field measurements of these stars have been performed using the profileaddition technique.The magnetic field strength and filling factor are obtained,and we find that there exist strong magnetic fields on very active stars.