应用微机校定三相变压器的联结组及标号

三相变压的联结组标号对其正常运行极为重要，必须校定，而目前变还缺少全面快捷的校定方法和设备。本文介绍采用微机系统来实现联结组桔的校定，首先把四类联结组差别区分开，然后分析指出同一类联结组中，除有六种正序标号外，存在六种逆序标号，提出用新的筛选法能简捷地判别校定同一类的十二种标号，当微机系统进行实际测试时，必须考虑电源电压三相不对称程序的影响，故经数学推导得出用实测计算值代替理想计算值作判别比较的基     

Pre-Main Sequence Stars Seen by ISO

Observations of pre-main sequence objects (T Tauri, Herbig Ae/Be and FU Orionis stars) obtained with the instrumentation on board the Infrared Space Observatory (ISO) are reviewed. All the observations have been mainly carried out by using the two spectrographs SWS and LWS, adopting their low resolution modes and such data have been used both for lines detection and to reconstruct the spectral energy distributions. Line emission and photometric behaviour of pre-main sequence objects have been analyzed in the framework of the current models, discussing the agreement (or disagreement) with them and trying to derive the questions which should be answered by the forthcoming FIR instrumentation. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

用电荷耦合器件测量激波辐射

用电荷耦合器件作摄谱探头，进行激波辐射的测量，解决了测量中遇到的同步问题。测量结果与一米光栅摄谱仪的记录干板比较，效果良好。     

On the optical variability of a be star,HDE 245770, — the optical counterpart of the transient X-ray pulsar A0535+26

Photoelectric WBVR observations of Be star HDE 245770=V 725 Tau, the optical counterpart of the transient X-ray pulsar A0535+26, having a pulse period of about 104 s, were conducted for more than 10 years. An irregular long-term optical variability of the star with amplitudes of the order of a few tenths of magnitude was found to be a usual phenomenon. In some cases rapid changes of the star's optical luminosity with a characteristic period of a few tens of minutes or a few hours, and an amplitude of several hundredths of magnitude in all the spectral bands used, which have practically coincided or correlated with the X-ray pulsar outbursts detected by X-ray satellites, were observed.Photoelectric recording of the optical flux from HDE 245770 were made in 1981–1982 with a time resolution of 1 second and 10 s, respectively, in theR spectral band (₀ 7000 Å) and in the narrowH -emission-line band (_1/2 75 Å) using a 48-cm reflector of High-Mountain Tien-Shan observatory of the Sternberg Astronomical Institute near Alma-Ata. An analysis of autocorrelation functions of the flux changes from object under study and a comparison with the star BD+26° 876 indicated the variability of luminosity of V 725 Tau in theR spectral band on a time scale of a few tens of second; this variability resembles shot noise with a characteristic time of stochastic bursts of about 15–20 s and their amplitudes of about a few tenths of a percent. InH -emission-line radiation autocorrelation functions and power spectra show quasiperiodic variability of luminosity of HDE 245770 with a characteristic period of about 100–150 s and an amplitude in the neighbour-hood of 0.5%. The latter result is not quite reliable because of not quite fine weather conditions during the observations; independent observations and check-up are required.     

数字处理技术在电子侦察中的应用

通过对信号进行侦察的数学模型和一种基于混沌序列的反侦察系统的介绍,讨论了在对抗与反对抗中取得信息优势的关键技术。指出了数字处理技术在电子侦察领域的重要作用及应用状况,并提出了一种新的反侦察技术的设想。     

几乎最佳自相关序列偶搜索算法的研究

几乎最佳自相关序列偶是一种新的最佳信号,但其一般的搜索方法——穷举法,搜索量太大。根据几乎最佳自相关序列偶的必要条件,提出一种新的搜索方法,给出算法流程图,并进行了实验验证。实验结果表明,算法可大大减小搜索量,比穷举法效果好且耗时短。     

一种利用辅助序列的PN序列捕捉系统

提出一种利用辅助序列进行PN序列捕捉的闭环系统,利用辅助序列估计本地PN序列与接收信号的相位差和方向,从而减小捕获时间。     

产生伪随机序列的一种方法

由于混沌是一种动态的、类随机的非线性系统,且具有对初始条件敏感、连续的功率谱、各态遍历等特性,因此可产生伪随机序列。本文就是将混沌连续的功率谱进行反褶、平移、相加、缩放等变换构造出了一种新的伪随机序列,通过理论分析和仿真试验,初步验证了该序列的各项特性是满足了Golomb的3个公设。此序列产生方法简单,基本可以广泛应用于保密通信等领域。     

单OSV服务多卫星的转移轨道优化研究

利用混合法解决了有限推力作用下单OSV服务多卫星的转移轨道优化问题.首先从OSV携带燃料的角度出发,初步筛选出在其服务范围内的服务对象,基于双脉冲交会假设,确定了服务序列以及时间节点;其次针对每一段转移轨道,利用Pontryagin极小值原理推导出最优控制律,设定开-关-开的发动机工作方式,将初始协态变量和开关机时间进行参数化处理,采用遗传算法对非线性规划问题进行求解;最后对整条轨道进行拼接优化.仿真结果表明,混合法对协态变量初值猜测敏感性小,降低了搜索最优转移轨道的难度,且控制轨线光滑.     

ABPSK原理及实现

从理论到实践，比较详细地说明了ABPSK调制的原理及与普通DBPSK调制的关系，给出了具体的实现过程框图，通过计算机模拟给出了若干调制的例子，并给出了相应的图表。