Broad-band spectral properties of accreting X-ray binary pulsars

Broad-band spectra of accreting X-ray binary pulsars can be fitted by a phenomenological model composed of a power law with a high energy rollover above 10 keV, plus a blackbody component with a temperature of few hundred eV. While, at least qualitatively, the hard tail can be explained in terms of (inverse) Compton scattering, the origin of the soft component cannot find a unique explanation. Recently, a qualitative picture able to explain the overall broad-band spectrum of luminous X-ray pulsars was carried out by taking into account the effect of bulk Comptonization in the accretion column. After a review of these recent theoretical developments, I will present a case study of how different modeling of the continuum affect broad features, in particular the cyclotron resonance features in Vela X-1.     

Orbital phase spectroscopy of four high mass X-ray binary pulsars to study the stellar wind of the companion

Our work focuses on a comprehensive orbital phase-dependent spectroscopy of the four High Mass X-ray Binary Pulsars (HMXBPs) 4U 1538-52, GX 301-2, OAO 1657-415 and Vela X-1. We hereby report the measurements of the variation of the absorption column density and iron-line flux along with other spectral parameters over the binary orbit for the above-mentioned HMXBPs in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. Out of the four pulsars, only in 4U 1538-52, we find the model having a reasonable corroboration with the observations, whereas in the remaining three the stellar wind seems to be clumpy and a smooth symmetric stellar wind model appears to be quite inadequate in explaining the data. Moreover, in GX 301-2, neither the presence of a disk nor a gas stream from the companion was validated. Furthermore, the spectral results obtained in the case of OAO 1657-415 and Vela X-1 were more or less similar to that of GX 301-2.     

美军主要机载信号情报能力发展现状及趋势

信号情报与国家安全息息相关。近年来,美陆海空军都在加强机载信号情报能力建设。梳理了美军主要机载信号情报能力的发展现状,分析其面临的挑战,预测其未来的发展趋势。     

前苏联可靠性工程的几个特点

与美，英体系相比、前苏联可靠性工程独具特点，对可靠性保证概念；可靠性工程与产品故障机理分析相结合；可靠性分析与系统功能分析相结合；可靠性工程与相关学科相结合；注重工程实用与ＣＡＤ化等五个方面进行了阐述，并强调了研究和借鉴前苏联可靠性工程的重要性。     

美军网络中心战的发展及其对装备建设的启示

网络中心战是信息化战争的主要作战样式。信息技术的广泛应用,大大提高了装备作战的能力,同时也对装备建设提出了更新更高的要求。阐述了美军网络中心战的含义与结构组成,分析了美军网络中心战的建设情况、关键技术、作战应用及其发展动向,最后探讨了网络中心战对装备建设的影响。     

Crew autonomy for deep space exploration: Lessons from the Antarctic Search for Meteorites

Future piloted missions to explore asteroids, Mars, and other targets beyond the Moon will experience strict limitations on communication between vehicles in space and control centers on Earth. These limitations will require crews to operate with greater autonomy than any past space mission has demonstrated. The Antarctic Search for Meteorites (ANSMET) project, which regularly sends small teams of researchers to remote parts of the southern continent, resembles a space mission in many ways but does not rely upon a control center. It provides a useful crew autonomy model for planners of future deep space exploration missions. In contrast to current space missions, ANSMET gives the crew the authority to adjust competing work priorities, task assignments, and daily schedules; allows the crew to be the primary monitor of mission progress; demands greater crew accountability for operational errors; requires the crew to make the most of limited communication bandwidth; adopts systems designed for simple operation and failure recovery; and grants the crew a leading role in the selection and stowage of their equipment.     

Bi系超导体主要特征量的计算及分析

应用巡游载流子与负U中心局域化载流子混杂相互作用的高T_c氧化物超导体理论模型,对Bi系超导体2212相和2223相的主要特征量——超导转变温度、穿透深度、相干长度、热力学临界场和T_c处比热跳跃进行了数值计算,并将计算结果与实验值比较。根据计算结果,对高T_c氧化物超导体的一些特性进行了分析讨论。     

U型蜂窝夹芯前缘制造技术研究

为解决U型蜂窝夹芯前缘制造过程中常见的脱粘、铺层皱褶、蜂窝芯尺寸超差等技术质量问题,从调整蜂窝芯展开基准面、优化蜂窝芯热定型工艺、控制铺层滑移等角度入手、完善此类零件的制造工艺流程。经过多个典型件验证,零件表面平整,外形尺寸符合要求,内部无缺陷,研究结果给相似零件的制造提供了借鉴。     

X射线脉冲星4U 1538—52 的时间和能谱特性

本文处理分析了EXOSAT卫星对4U1538-524次中能观测资料,并结合其他观测结果对4U1538-52的时间和能谱特性作了分析和解释:中子星自转仍在减慢;能谱为幂律谱,Tenma卫星以后的观测未见Fe发射线;X射线dip现象可解释为一前景星对中子星的遮掩而形成;X射线爆发在不同的轨道位相出现,持续近1小时;在1keV附近似有一发射线。      

基于显式表达式的空间目标最大碰撞概率分析

最大碰撞概率的计算在空间目标碰撞风险评估中具有重要意义。基于碰撞概率的显式 表达式,利用一元函数和二元函数求极值的方法分别讨论了目标误差椭球形状固定和不定两 种情况下最大碰撞概率的计算方法,得到了两种情况下最大碰撞概率的表达式。对于误差椭 球形状固定的情况得到了碰撞概率最大时两目标位置协方差的取值,对于误差椭球不定情况 得到了碰撞概率最大时径向联合方差的取值和水平面内联合方差所满足的关系。分析了最大 碰撞概率的影响因素,讨论了水平面内误差方差的耦合特性。对今年二月发生的美俄卫星碰 撞事件进行了分析,得到误差椭球任意形状时最大碰撞概率为1.864E-3。