空间材料深层充放电效应试验研究

利用电子枪发射的单能电子束、以及放射源发射的能谱结构接近空间电子环境的β射线电子,模拟试验了几种常用空间介质材料和某卫星部件的深层充电过程;结合对放电电流脉冲和电场脉冲的测量,观测了深层放电脉冲信号及其对试验电路的影响。试验结果表明,在类似实际空间强度的pA量级电子束辐照下,介质材料可以累积大量电荷,其表面电位可以达到近万V;随后发生的介质材料放电可产生高强度的放电电流脉冲和电场脉冲,放电脉冲对试验电路造成较强的干扰。     

XANES analysis of organic residues produced from the UV irradiation of astrophysical ice analogs

Organic residues formed in the laboratory from the ultraviolet (UV) photo-irradiation or ion bombardment of astrophysical ice analogs have been extensively studied for the last 15 years with a broad suite of techniques, including infrared (IR) and UV spectroscopies, as well as mass spectrometry. Analyses of these materials show that they consist of complex mixtures of organic compounds stable at room temperature, mostly soluble, that have not been fully characterized. However, the hydrolysis products of these residues have been partly identified using chromatography techniques, which indicate that they contain molecular precursors of prebiotic interest such as amino acids, nitrile-bearing compounds, and amphiphilic compounds. In this study, we present the first X-ray absorption near-edge structure (XANES) spectroscopy measurements of three organic residues made from the UV irradiation of ices having different starting compositions. XANES spectra confirm the presence of different chemical functions in these residues, and indicate that they are rich in nitrogen- and oxygen-bearing species. These data can be compared with XANES measurements of extraterrestrial materials. Finally, this study also shows how soft X rays can alter the chemical composition of samples.     

试论引进教材与国内教材的合理使用

教材作为高校系统授课的重要资料,它是依据教育的目标与内容所编著的,有利于教学活动的展开和学生的学习与掌握.当前在外语院校的教学中,引进教材和使用国内原版教材已成为一种趋势,但是实现二者阃的互补,注重引进教材中存在的问题,结合实际,为我所用,才能起到培养应用型人才的目的.     

Model of a fluxtube with a twisted magnetic field in the stratified solar atmosphere

We build a single vertical straight magnetic fluxtube spanning the solar photosphere and the transition region which does not expand with height. We assume that the fluxtube containing twisted magnetic fields is in magnetohydrostatic equilibrium within a realistic stratified atmosphere subject to solar gravity. Incorporating specific forms of current density and gas pressure in the Grad–Shafranov equation, we solve the magnetic flux function, and find it to be separable with a Coulomb wave function in radial direction while the vertical part of the solution decreases exponentially. We employ improved fluxtube boundary conditions and take a realistic ambient external pressure for the photosphere to transition region, to derive a family of solutions for reasonable values of the fluxtube radius and magnetic field strength at the base of the axis that are the free parameters in our model. We find that our model estimates are consistent with the magnetic field strength and the radii of Magnetic bright points (MBPs) as estimated from observations. We also derive thermodynamic quantities inside the fluxtube.     

李萨如图在磁记忆二维定量检测中的应用

依据磁记忆二维检测原理,将磁信号法向分量存在过零点,切向分量存在最大值联合起来检测,并引入李萨如图分析法,对用法向分量和切向分量合成的类李萨如图以及将法向分量和切向分量微分后合成的李萨如图进行比较分析,得出可以利用微分后合成的李萨如图封闭区域面积的大小来判断应力集中程度及用在不同的应力集中程度下李萨如图面积数量级作为阈值的结论.从而可为利用李萨如图分析法对磁记忆二维检测进行定量分析的进一步研究提供试验分析依据.     

复合材料电搭接分析

电搭接是指用金属编织线或金属片将机载设备的外壳与飞机基本结构连接起来,使两者处于一个共同的电位点。飞机上采用复合材料后,由于复合材料与金属之间电性能的差异,在GJB358-87中规定的搭接电阻值就不完全适用。本文在研究了大量国内外资料的基础上,根据国内目前的技术水平,对安装在复合材料结构上的机载设备,按不同的电搭接功能要求,提出了合适的搭接电阻值。     

T250与30CrMnSiA异种材料焊接工艺技术

从冶金方面分析了T250与30CrMnSiA材料焊接工艺性。通过手工钨极氩弧焊焊接工艺研究试验,选择焊丝材料,确定材料焊接状态,制定了合理有效的焊接工艺规范和措施。采用光学金相显微镜、维氏硬度测试和力学性能检测等手段,对T250与30CrMnSiA异种材料焊接接头金相组织、力学性能和显微硬度等方面进行详细分析。结果表明,T250和30GrMnSiA异种材料具有良好的焊接性,填充HT250焊丝,采用热输入量较小的焊接电流进行焊接,接头强度与30GrMnSiA材料强度相当。     

Investigations of an integrated angular velocity measurement and attitude control system for spacecraft using magnetically suspended double-gimbal CMGs

This paper presents an integrated angular velocity measurement and attitude control system of spacecraft using magnetically suspended double-gimbal control moment gyros (MSDGCMGs). The high speed rotor of MSDGCMG is alleviated by a five-degree-of-freedom permanent magnet biased AMB control system. With this special rotor supported manner, the MSDGCMG has the function of attitude rate sensing as well as attitude control. This characteristic provides a new approach to a compact light-weight spacecraft design, which can combine these two functions into a single device. This paper discusses the principles and implementations of AMB-based angular velocity measurement. Spacecraft dynamics with DGMSCMG actuators, including the dynamics of magnetically suspended high-speed rotor, the dynamics of inner gimbal and outer gimbal, as well as the determination method of spacecraft angular velocity are modeled, respectively. The effectiveness of the proposed integrated system is also validated numerically and experimentally.     

Improved orbital parameters of accreting millisecond pulsar SAX J1808.4-3658

We analyze the three outbursts of the X-ray millisecond pulsar SAX J1808.4-3658 that occurred in 1998, 2000, and 2002 observed with RXTE. With a technique based on epoch folding search we find an unique orbital solution valid over the five years of high temporal resolution data available. We revise the estimate of the orbital period, P_orb = 7249.1569(1) s and of its error, which we decrease by one order of magnitude. We also give the first constraint on the orbital period derivative, . We find that in 2002 the pulse profile shape is clearly asymmetric, showing a secondary peak at about 145° from the main pulse, which is different from the sinusoidal shape reported at the beginning of the 1998 outburst.     

Some Observational Evidence of Alfven Surface Waves Induced Magnetic Reconnection

The surface wave induced magnetic reconnection (SWIMR) model based on Alfven Resonance theory will be discussed briefly both for collisional and collisionless plasmas. It is shown that the spatial scales and time delays associated with Flux Transfer Events and Pulsed Ionospheric Flows, as observed by satellites and SuperDARN radars and the magnetic bubbles, observed at the high latitude boundary of the magnetopause, can be explained by the SWIMR model. This revised version was published online in August 2006 with corrections to the Cover Date.