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.     

Reconstructed 3-d magnetic field structure and hard X-ray two ribbons for 2000 Bastille-day event

The Bastille-day event in 2000 produced energetic 3B/X5.6 flare with a halo CME, which had great geo-effects consequently. This event has been studied extensively and it is considered that it follows the two-ribbon flare model. The flare/CME event was triggered by an erupting filament and TRACE observations showed formation of giant arcade structures during the flare process. Hard X-ray (HXR) two ribbons revealed for the first time in this flare event (Masuda et al., 2001). The reconstruction of 3-D coronal magnetic fields revealed a magnetic flux rope structure, for the first time, from extrapolation of observed photospheric vector magnetogram data and the flux rope structure was co-spatial with portion of the filament and a UV bright lane (Yan et al., 2001a, 2001b). Here we review some recent work related to the flux rope structure and the HXR two ribbons by comparing their locations and the flux temporal profiles during the flare process so as to understand the energy release and particle accelerations. It is proposed that the rope instability may have triggered the flare event, and reconnection may occur during this process. The drifting pulsation structure in the decimetric frequency range is considered to manifest the rope ejection, or the initial phase of the coronal mass ejection. The HXR two ribbons were distributed along the flux rope and the rope foot points coincide with HXR sources. The energy dissipation from IPS observations occurred within about 100 R _⋅ is consistent with the estimate for the flux rope system. This revised version was published online in August 2006 with corrections to the Cover Date.     

用Visual FoxPro进行动态界面的设计

本文介绍用 Visual FoxPro的定时器。标签、按钮等控件和控件的属性、方法、事件等在界面上设计动态字幕、动态按钮等若干动态效果的方法。     

基于Web方式下的信息管理系统的开发

本文介绍了一个基于Web方式下信息信息管理系统的开发实例，重点阐述了Web方式下信息管理系统的设计思想以及及关键技术的实现     

FY-2气象卫星在轨管理工程测控关键技术(上)

介绍了风云二号(FY—2)地球静止轨道自旋气象卫星工程测控的关键技术。分析了位置保持、姿态确定、星蚀和日凌的原理，给出了位置保持、姿态控制策略和地影、月影、日凌预报算法。并提出了一种检验定姿结果正确性的方法，提供了相应的工程计算参数。这些策略都已成功地用于FY—2卫星的在轨管理工程测控。     

ZN3火箭姿态测量用太阳角计

本文给出了用于ＺＮ３火箭姿态测量太阳角计的原理和测量结果，讨论了背景抑制和标定方法，分析了误差来源。该仪器采用选取适当探测波段和比值测量方法较好地消除了地外太阳辐照和大气消光的影响，也有效地抑制了背景辐射的干扰，大大提高了测量精度。实测结果表明，火箭姿态角测量的均方根误差约为０．７°。这一方法适用于各种自旋稳定飞行器的姿态测量。     

卫星抗辐射加固技术

分析了FY－1C卫星运行轨道空间辐射环境，介绍了整星、单机、器件抗辐射要求。卫星研制过程中，对各单抗和系统在技术设计、元器件设计、软件编制等的抗辐射加固设计要求。特别对有CPU和存储器的单粒子翻转效应（SEU）和闩锁效应（SEL）试验。仪器和系统的软件均用故障注入的方法完成了抗SEU的仿真试验。     

关于双向弯曲变形构件危险截面的讨论

本文通过具体例题，阐述了双向弯曲变形构件中危险截面的判定方法，论证了合成弯矩大的截面不一定是危险截面的结论。     

FY—1C卫星的资料处理及应用研究

介绍了FY－1C的轨道特征、对地观测能力、星上数据贮存能力和数据传输能力等，以及卫星仪器特性、光谱波段特征和应用能力。最后给出了卫星资料的应用情况。     

卫星捕获太阳的新方法

对卫星入轨后捕获太阳的方法进行了研究 ,并对一种有效的控制规律进行了分析计算 ,最后对卫星的运动过程进行了仿真验证