Kilohertz quasi-periodic oscillations in SAX J1808.4–3658

I present a short overview of the behavior and properties of the two simultaneous kilohertz quasi-periodic oscillations (kHz QPOs) seen in the accreting millisecond X-ray pulsar SAX J1808.4–3658. I will focus on the behavior of the upper frequency QPO as a function of time and count rate as seen during the 2002 outburst of this source. I will also discuss briefly the correlated behavior of this QPO with QPOs at lower frequencies (several tens of hertz).     

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.     

The double-pulsar binary J0737–3039

A recent multibeam pulsar survey of the outer Galactic plane at Parkes has discovered the first-known double-pulsar binary, a very compact double neutron star system in which both stars are observable as radio pulsars. In this review, we briefly describe the discovery and the studies which have been enabled by the unique properties of the system. These range from the most precise confirmation yet of the theory of general relativity, with the possibility of even more new tests and the measurement of second-order post-Newtonian effects, to studies of the magnetospheres and emission properties of the two pulsars. The discovery also results in a significant increase in the expected rate of occurrence of the mergers of double neutron star systems, and hence the rate of detection of such events by the new ground-based gravitational wave detectors.     

辐射发射参考源在EMC比对中的应用

辐射发射参考源是在对EMC测试系统进行比对测试和定期场地校验时必不可少的设备,介绍了辐射发射参考源的原理和特点、各种实现方式、国内外应用概况及其稳定性考核措施。     

加速器切线照相技术研究

根据工作实践研究了固体发动机切线照相无损检测中黑度分布、散射线防治、象质计使用、检测概率计算、脱粘临界值确定等技术问题.     

载人航天可靠性与空间环境试验

文章通过对国外载人航天事故统计,分析各种空间环境条件对航天器及航天员的影响,阐述了空间环境试验对提高载人航天可靠性的重要意义,提出为了提高载人航天的可靠性,应进行充分和严格的空间环境模拟试验。     

对转桨推进型鱼雷有动力影响研究

为使国内具备鱼雷有动力风洞试验能力 ,通过设备研制和对转桨推进型鱼雷性能研究试验表明 :一是动力对姿态导数影响达 40 % ,效率导数一般下降 1 0 %～ 1 5 % ,设计单位应重视上述特性对鱼雷航行与机动特性的影响 ;二是对转桨对雷体稳定性作用值得高度重视 ,传统认为对转桨是鱼雷辅助稳定装置的设计思想应有所调整 ,尤其对机动性要求高的鱼雷。     

0.1米低温风洞的设计

本文阐述了我国首次设计和建造的低温风洞的设计特点及共性能。这是一座以风扇驱动的闭口回流式风洞,用氮气作试验气体。试验段为0.1米的方形截面。计运转参数范围为:M=0.04～0.40,P_t=101.2 kPa～202.6kPa,T_t=79K～320K。试验时间为半小时。风洞壳体是用铝合金制造的,外部用超细玻璃棉绝热。风扇用交流电机拖动,转速用变频控制。     

国外风洞试验的新机制、新概念、新技术

风洞是空气动力学研究的重要地面试验设备,是保证一个国家航空航天处于领先地位的基础研究设施。面对新世纪航空航天领域的激烈竞争,世界发达国家加强了新概念风洞研制,改革风洞运行机制,一些新技术也在大型生产性风洞得到应用。