在J2EE平台下进行多层分布式数据库系统开发的研究

J2EE是SUN公司提出的在分布式环境中的一种体系结构,EJB是基于J2EE(Java2平台企业版)开发基于Web企业应用程序的基础,EJB体系结构是生成业务应用程序的主要分布式组件模型。本文介绍了J2EE和EJB基本概念和特点,并列举了在J2EE平台下运用EJB技术开发多层分布式数据库系统的开发示例。     

在地球扁率摄动下的卫星编队飞行控制

卫星编队飞行的难点之一是在干扰力环境下控制队形。采用了一种基于线性二次调节器(LQR)的最优控制方法，对低轨道地球卫星所受的地球扁率摄动(J2力)加以模拟，并在模拟的地球低轨道J2力环境中。对几种卫星编队进行了模拟控制，从控制精度和能量消耗的角度对控制方法进行了分析，提出了卫星编队飞行中相对距离控制和绝对距离控制需要注意的问题。     

基于B/S在线考试系统的开发

首先介绍传统考试方法的现状及其发展方向,并根据目前学校考试的实际需要,提出一个新的基于B/S模式考试方式.接着介绍了相关的技术,并对其实现的可行性、可靠性、高效性等做了进一步分析,同时给出系统解决方案.最后,阐述了整个系统安全性以及需要完善和改进之处.     

The optical to X-ray spectrum of the broad-line ultrasoft AGN RE J2248-511

We present a series of monitoring observations of the ultrasoft broad-line Seyfert galaxy RE J2248-511 with XMM-Newton. Previous X-ray observations showed a transition from a very soft state to a harder state five years later. We find that the ultrasoft X-ray excess has re-emerged, yet there is no change in the hard power-law. Reflection models with a reflection fraction of 15, and Comptonisation models with two components of different temperatures and optical depths (kT₁ = 83 keV, T₁ = 30 eV, τ₁ = 0.8; KT₂ = 3.5 keV, T₂ = 60 eV, τ₂ = 2.8) can be fit to the spectrum, but cannot be constrained. The best representation of the spectrum is a model consisting of two blackbodies (kT₁ = 0.09 ± 0.01 keV, kT₂ = 0.21 ± 0.03 keV) plus a power-law (Γ = 1.8 ± 0.08). We also present simultaneous optical and infrared data showing that the optical spectral slope also changes dramatically on timescales of years. If the optical to X-ray flux comes primarily from a Comptonised accretion disk we obtain estimates for the black hole mass , accretion rate and inclination cos(i)  0.8 of the disk.     

Changes in radio emission from PSR J0737–3039B

The double pulsar system, J0737–3039, provides a unique probe of a pulsar magnetosphere due to its edge-on viewing geometry, a tight orbit and a significant rate of advance of the angle of periastron. In this paper, we report on the changes in radio emission from the long period pulsar in this system, J0737–3039B, over a period of 9 months. Observations of this system with Giant Metrewave Radio Telescope (GMRT) show that the duration of the first bright phase of the pulsar centered at 210° orbital longitude from the ascending node is shrinking. These observations will be useful to constrain the proposed models for this system.     

高温受弯构件表面裂纹疲劳扩展寿命预测

基于J-积分半经验公式建立了构件表面裂纹在其长度和深度方向上的疲劳扩展速率表达式,用来预计模拟SUS304钢构件在550℃高温环境中受弯曲载荷作用下表面裂纹的疲劳扩展寿命.并在相同条件下进行了疲劳裂纹扩展试验.结果表明,预测曲线与实验数据基本一致,证明了本文预测方法的有效性.     

J2摄动作用下近地轨道卫星编队构形长期演化机理分析

研究近地轨道卫星编队构形在引力摄动作用下的长期演化机理。把用转移矩阵法得出的相对运动分析解表达成一般轨道根数形式，为研究摄动影响而进一步表达成无奇点轨道根数形式；根据各轨道根数的J2摄动解分别研究编队构形在轨道坐标系三个方向上的振幅与相位的长期变化情况，揭示了构形引力摄动的长期演化机理；给出编队构形的摄动表达式，并以仿真实例验证其可信性；最后给出构形长期引力摄动的相关结论，并对编队构形设计提出建议，这将为研究编队构形的规划技术带来方便。     

Optical/X-ray correlations as a signature of jet-disc coupling in the accreting black hole XTE J1118+480

We interpret the rapid correlated UV/optical/X-ray variability of XTE J1118+480 as a signature of the coupling between the X-ray corona and a jet emitting synchrotron radiation in the optical band. We propose a scenario in which the jet and the X-ray corona are fed by the same energy reservoir where large amounts of accretion power are stored before being channelled into either the jet or the high energy radiation. This time-dependent model reproduces the main features of the rapid multi-wavelength variability of XTE J1118+480. A strong requirement of the model is that the total jet power should be at least a few times larger than the observed X-ray luminosity, implying a radiative efficiency for the jet _j  3 × 10⁻³. This would be consistent with the overall low radiative efficiency of the source. We present independent arguments showing that the jet probably dominates the energetic output of all accreting black holes in the low-hard state.     

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.     

3J53弹簧表面裂纹缺陷原因分析

3J53钢丝在车间缠绕成弹簧并经热处理后发现其表面存在线性缺陷。用扫描电镜对钢丝线性缺陷的形貌进行了分析,对线性缺陷区域进行了能谱分析,并利用金相显微镜观察了线性缺陷的中心部位及其周围区域的金相组织。结果表明:钢丝表面的线性缺陷呈锯齿状,沿钢丝轴向方向,为裂纹型折叠缺陷。折叠缺陷是钢丝在生产过程中形成,在绕簧和热处理过程中,裂纹型折叠缺陷发生扩展和延伸,最终形成线性缺陷。