A multi-wavelength study of the merger candidate Abell S0721 and the activities of its member galaxies

We present a multi-wavelength study of the merging history and its influence on galaxy activities of a newly detected merger candidate – Abell S0721. This cluster was only known as a poor cluster in the Shapley Supercluster, but when several survey data of different wavelengths are combined, evidence of strong merging is revealed. We have analyzed the optical and X-ray structures of the cluster, as well as galaxy dynamics and properties of the radio galaxies in the cluster. The dynamics analysis shows the velocity distribution of this system is significantly deviated from a 1-Gaussian model, indicating the existence of 2–3 dynamically different sub-systems; in addition, both optical and X-ray structures of the cluster show an elongated and multi-clump structure, two X-ray clumps imaged by ROSAT All Sky Survey are well correlated with two galaxy density peaks. This cluster is possibly a merger of several groups; our analysis shows that the projection angle for two clumps in the main structure is possibly near the projection plane, and the substructure is seen at ∼30–75° from the projection plane. The merging process could also be the origin to boost the activities of its member galaxies. Finally, as compared with other merger candidates in the Shapley Supercluster, the radio galaxies identified in Abell S0721 are all optically luminous, and the fraction of luminous radio galaxies is only lower than one merger candidate (which is proposed to be at the very beginning of a merger event), this suggests Abell S0721 is also at the beginning of a merger event.     

自调节模拟低通滤波器的研究

通过对有源低通滤波器，频率／电压转换器AD650及其变容二极管的特性分析，提出由信号频率来自调节有源低通滤波器截止频率的新设计方案，并对其可行性进行了分析和研究。     

相控阵天线有源单元方向图的计算方法

基于弗洛奎定理给出了一种计算无限相控阵有源单元方向图的方法。与传统的基于有源反射系数的方法不同,这种方法不但可以用于计算功率方向图,而且可以计算场方向图,因此可以计算诸如交叉极化、相位信息等更多的辐射特性。通过数值计算结果与仿真结果的比较验证了方法的正确性。     

重力梯度小卫星重力场捕获的Lyapunov法

探讨了重力梯度小卫星采用主动磁控技术进行重力场捕获的Ｌｙａ－ｐｕｎｏｖ能量耗散法;给出了分区控制的条件及逻辑;阐述了磁控力矩的产生方法。仿真结果表明,该方法简单、有效,控制精度达到磁控小卫星的较高水平。     

Extragalactic observations and future missions

We briefly review some questions of extragalactic astrophysics and cosmology that would most benefit from future missions outside the Earth's atmosphere in the IR and submillimeter. These include the formation and early evolution phases in galaxies and the probably related question of quasar formation; the observation of Active Galactic Nuclei embedded in thick dusty structures (torii) and its impact on the still debated unified model of AGN activity; the observability of radiation processes occurring at very highz through background measurements; the investigation of the large scale structure and velocity field in the distant universe; and studies of the interstellar medium in galaxies. Some more emphasis is given on the galaxy formation problem, because we believe that IR-mm sensitive observations will be crucial to its final solution.     

柔性多体卫星自抗扰控制系统的研究

设计了一种新型的姿态控制器一姿态自抗扰控制器。采用简化了的刚体动力学模型，即把柔性太阳帆板与柔性天线等的振动都看作外干扰，对象的不确定性、未建模动态与外干扰的总量都由自抗扰控制器估计出，再用该估计总量实现动态反馈补偿。该姿态控制器，只需控制输入转换矩阵的估计值，无需精确的卫星动力学模型。改变星体转动惯量或设置干扰力矩情况下的数学仿真表明，所设计的自抗扰控制器具有较小的稳态误差、较快的动态响应及对干扰有较强的抑制能力。     

行星际航天器主动热控系统模糊控制

对行星际航天器主动热控系统进行了研究。以“火星探路者”号为例，在其机械泵式单相液体循环冷却系统设计布局的基础上，使用更高换热效率、更低压力降的分形微管道网络换热器传递电子设备散发的热量，利用模糊控制策略对系统进行控制。通过合理的简化和假设，应用集总参数法建立系统动态特性模型，进行仿真研究。结果表明此主动热控系统能对航天器电子设备温度进行有效控制。     

主动控制式对接机构对接预捕获阶段的仿真

介绍了主动控制式对接机构对接的基本操作过程，并以具有六个作动阻尼器的主动接制式对接机构为例，对对接预捕获阶段作了详细的研究。 该阶段两对接飞行器的运动方程，给出了作动／阻尼器为满足捕获条件所需达到的长度的计算方法，设计了控制回路，在此基础上作了数值仿真。仿真结果表明，建立的数学模型是正确的，设计的控制系统控制效果良好。     

细长体双自旋卫星消旋主动章动控制动力学解耦的系统仿真

细长体双自旋卫星自旋部分的能量耗散会导致卫星章动运动的发散。利用消旋体的惯性积在动力学上的耦合作用,使消旋电机的轴向力矩通过耦合,产生横向力矩来阻尼章动,称之为消旋主动章动控制（ＤＡＮＣ）［１］。本文提出一种利用动力学解耦的仿真方案,用单轴平台进行细长体双自旋卫星消旋和章动控制的系统试验,验证了系统的可行性。     

航空装备现场使用质量和可靠性信息管理软件

对航空装备现场使用质量和可靠性信息的特点进行了阐述，并介绍其软件系统的组成和功能。着重讨论系统中用外场数据估计产品可靠性参数的分析、处理方法及此系统数据库的设计