定义在屏幕上显示汉字形文件形的函数

在工程图样中技术要求、标题拦与明细表等用汉字来说明。用户使用非汉化的ＡｕｔｏＣＡＤ（英）２．１８版～１０．０版编辑图形，有时需要加汉字文本到图上。本文将介绍应用定义在屏幕上显示一个汉字形文件中各个形的函数，在输出的汉字表上可以准确检索出汉字的形名，便于汉字调用。     

Highlights of the Brazilian Solar Spectroscope

The digital, decimetric (950–2500 MHz) Brazilian Solar Spectroscope (BSS, Sawant, H.S., Subramanian, K.R., Faria, C., et al. Brazilian Solar Spectroscope (BSS). Solar Phys. 200, 167–176, 2001) with high time (10–1000 ms) and frequency (1–10 MHz) resolution is in regular operation since April, 1998, at the National Space Research Institute (INPE) at São José dos Campos, Brazil. The BSS has now been upgraded with a new digital data acquisition and data processing system. The new version of the BSS has improved the observational possibilities with the capability to record up to 200 frequency channels available in the selectable frequency range 950–2500 MHz. The GPS receiver permits the acquisition of data with time accuracy in the order of 0.1 ms. The software system of the BSS is composed by two distinct modules: the first, data acquisition system provides a flexible Graphical User Interface (GUI) that allows one to choose the observational parameters. The second module is the real time visualization system that permits real time visualization of the observed dynamic spectrum and additionally allows procedures for visualization and preliminary analysis of the recorded solar spectra. Using the new visualization system, we have realized two new types of dm-radio fine structures: narrow band type III bursts with positive as well as negative group frequency drift and dots emissions arranged in zebra-like and fiber-like chains. Furthermore, we have found flare generated fast wave trains according to their tadpole signature in wavelet power spectra for a decimetric type IV radio event (June 6, 2000 flare).     

The Swift Supergiant Fast X-ray Transients Project: A review,new results and future perspectives

We present a review of the Supergiant Fast X-ray Transients (SFXT) Project, a systematic investigation of the properties of SFXTs with a strategy that combines Swift monitoring programs with outburst follow-up observations. This strategy has quickly tripled the available sets of broad-band data of SFXT outbursts, and gathered a wealth of out-of-outburst data, which have led us to a broad-band spectral characterization, an assessment of the fraction of the time these sources spend in each phase, and their duty cycle of inactivity. We present some new observational results obtained through our outburst follow-ups, as fitting examples of the exceptional capabilities of Swift in catching bright flares and monitor them panchromatically.     

双体卫星对日定向姿态机动控制

研究了双体卫星(DFP)对日定向姿态机动控制问题。首先分析双体卫星工作机理,建立载荷舱与平台舱姿态模型,推导磁浮机构线圈和磁钢相对距离的数学表达式。提出基于PD控制的载荷舱对日姿态机动、平台舱姿态跟踪以及两舱避碰等控制策略。在此基础上,为提高平台舱姿态跟踪速度,设计反步控制器对平台舱飞轮的动态特性进行补偿。进一步,为提高两舱协同控制性能,对传统PD控制进行改进,提出基于变增益PD控制的载荷舱姿态机动控制律,将两舱相对姿态信息包含在载荷舱对日姿态机动控制律中,有效降低了两舱碰撞风险,提高了两舱姿态机动速度。仿真结果表明,本文控制算法能有效实现双体卫星对日定向,且能避免两舱碰撞。     

太阳软X射线背景水平与X级的增强发射

本文根据1986年1月-1992年12月期间,130个1-8?的X级别的X射线事件与相应背景发射水平所作的分析,发现90%以上的X级X射线事件,都发生在X射线背景发射≥C1(10-6W／m2)水平上,这一统计规律,可从耀斑加速的非热电子对色球等离于体的加热得到合理的解释.      

太阳微波爆发与高能质子的共生过程

本文根据近年来对太阳射电爆发与高能质子／γ射线谱线辐射等观测资料的统计分析,得出不同型别的太阳射电爆发中以微波爆发与γ射线辐射／质子事件发生过程中的高能质子共生率最高,趋近100％,这一结果,否定了以前认为米波Ⅱ型或米波Ⅳ型爆发拥有产生高能质子必要条件的看法;指出：上述微波爆发可以细分为脉冲型和微波Ⅳ型（Ⅳμ型）,它们的物理条件不同,共生关系的表现特征也不尽相同;并且对上述共生现象的物理过程作了初步的解释和探讨．     

空间站对日定向装置试验台的控制器设计与精度考核

针对太阳电池帆板大挠性、大惯量等特性,导致对对日定向装置施加的大幅值、高频响的变负载力矩难以模拟和模拟精度不足的问题,设计了以电动负载模拟器为核心装置的地面半物理仿真试验台。首先建立了电动负载模拟器（加载单元）模型,采用递推最小二乘法对加载单元各参数进行辨识,并分析各参数对加载单元响应特性的影响。提出一种超前校正与模糊自适应PID相结合的复合控制算法,该方法有效地拓宽了加载单元带宽、改善了力矩跟随性能和抑制了力矩误差。用不同信号对试验台响应速度、加载带宽和加载精度进行分析和考核。实验结果表明：该复合控制算法使加载力矩较好地复现了太阳电池帆板模型的期望输出力矩,为对日定向装置对太阳电池帆板的驱动性能考核实验模拟出较为精确的期望模型的负载（测试）力矩。     

Primordial Helium and ΔY/ΔZ from H II Regions and from Fine Structure in the Main Sequence Based on Hipparcos Parallaxes

The primordial helium abundance YP is important for cosmology and the ratio Y/Z of the changes relative to primordial abundances constrains models of stellar evolution. While the most accurate estimates of YP come from emission lines in extragalactic H II regions, they involve an extrapolation to zero metallicity which itself is closely tied up with the slope Y/Z. Recently certain systematic effects have come to light in this exercise which make it useful to have an independent estimate of Y/Z from fine structure in the main sequence of nearby stars. We derive such an estimate from Hipparcos data for stars with Z Z and find values between 2 and 3, which are consistent with stellar models, but still have a large uncertainty.     

发展空—地数据链面临的问题

70年代ARINC和SITA公司建立了为航空公司运营服务的空—地VHF数据链,采用面向字符协议.其机载设备分别为ACARS和AIRCOM,两家公司分别在全球建立了地面通信网路.新CNS/ATM系统所定义的空—地数据链不论通信的物理手段用卫星、VHF或S模式,均在面向位的协议下,可以在航空电信网(ATN)中互连传送.任何一个国家发展空—地数据链时都面临着选择,应考虑是迁就旧体制发展面向字符的网路,还是一步到位地直接发展面向位的网络.     

证券投资组合的优化分析

在日趋发达的商品经济社会,证券投资在各类经济活动中有着重要的地位.如何从几种证券中选择最优投资组合,这就是证券投资组合分析的内容.主要介绍从建立数学模型,选用非线性分析的数值计算方法,到在微机上实现的过程和最终的分析结果.