综合控制系统研究及其仿真

研究了综合火力/飞行/推进控制系统原理及其各个子系统的控制律设计方法,研究通过飞行、推进、火控等系统的综合实现自动飞行、自动攻击的原理,并利用VC 和Open GL联合开发了综合控制仿真、设计平台,结合有效的任务管理及控制律剪裁,实现了灵活的系统运行配置,将设计平台和仿真平台集为一体,并将多个系统的综合、测试、仿真在一个平台上实现。最后通过数字仿真表明,综合控制系统明显地提高了飞机综合化、自动化水平,也验证仿真平台达到了设计要求。     

超塑变形对TC4 室温力学性能的影响

在T=880℃和ε=9.8 ×10-4 s-1下,进行了TC4圆筒件超塑成形试验,研究了超塑变形量对TC4室温强度、疲劳性能和金相组织的影响.结果表明:随着变形量的增加,晶粒尺寸增大.当超塑胀形延伸率e为55％时,晶粒尺寸由供应态的约8μm增加为约20 μm.随着e增加,TC4室温下的屈服强度、抗拉强度和条件疲劳强度降低.当e为55％时,材料的屈服强度、抗拉强度下降约7％;循环周期为106下的疲劳强度下降约10％.     

带扰流片的升力风扇操纵特性数据采集系统设计

以带扰流片的升力风扇为动力系统的无人机,在动力学建模和控制方式上与传统升力风扇无人机有很大不同,升力风扇的操纵特性是这类升力风扇无人机动力学建模的关键,而目前国内尚未检索到对此进行研究或实验的报告或文献。因此,为了研究带扰流片的升力风扇动力系统的动态操纵特性,利用LabVIEW设计并制作一套动态数据试验采集系统,设计试验输入,完成带扰流片的升力风扇操纵特性动态数据采集,所获得数据及后续建模过程表明本试验采集系统是正确、有效的。     

Fault self-repair strategy based on evolvable hardware and reparation balance technology

In the face of harsh natural environment applications such as earth-orbiting and deep space satellites, underwater sea vehicles, strong electromagnetic interference and temperature stress,the circuits faults appear easily. Circuit faults will inevitably lead to serious losses of availability or impeded mission success without self-repair over the mission duration. Traditional fault-repair methods based on redundant fault-tolerant technique are straightforward to implement, yet their area, power and weight cost can be excessive. Moreover they utilize all plug-in or component level circuits to realize redundant backup, such that their applicability is limited. Hence, a novel selfrepair technology based on evolvable hardware（EHW） and reparation balance technology（RBT） is proposed. Its cost is low, and fault self-repair of various circuits and devices can be realized through dynamic configuration. Making full use of the fault signals, correcting circuit can be found through EHW technique to realize the balance and compensation of the fault output-signals. In this paper, the self-repair model was analyzed which based on EHW and RBT technique, the specific self-repair strategy was studied, the corresponding self-repair circuit fault system was designed, and the typical faults were simulated and analyzed which combined with the actual electronic devices. Simulation results demonstrated that the proposed fault self-repair strategy was feasible. Compared to traditional techniques, fault self-repair based on EHW consumes fewer hardware resources, and the scope of fault self-repair was expanded significantly.     

通用的航电系统总线接口仿真平台的设计和应用

针对当前航电系统仿真器的缺点,提出了一种通用的航电系统总线接口仿真平台的设计思想,通过建立仿真数据库,从待仿真的航电系统设备中的接口信息抽象出属性和行为,然后用数据库的方式来描述,实现了仿真软件和仿真对象的分离,从而使该仿真平台具备了通用性和灵活性。该仿真平台已经在某型机航电系统地面联试中得到了应用。     

一种悬挂物兼容飞机航电与武器总线的设计方法

在某悬挂物作为通用系统挂装不同型号飞机时,由于不同型号飞机对该悬挂物采用航电和武器两种不同的总线通信方式,导致该悬挂物不能兼容挂载多型飞机。本文针对现有的总线应用情况,提出了一种悬挂物可兼容飞机不同总线通信方式的设计方案,并给出了方案的具体实现方法。     

试论管理标准体系和体系表

阐述了管理标准体系的构成,以及管理标准体系表层次之间的相互关系和作用。     

超声波激振铰刀铰孔的研究

本文研究了将超声波能量施予刀具，使其产生一定振幅的超频振动铰孔的工艺方法。进行了铰孔精度、表面粗糙度及其铰孔规律的试验，也探讨了振铰孔的机理。     

论高校医院与全科医学

保证高校教职工、大学生的身心健康,是高校医院义不容辞的责任.为此,应探索一条更适合高校实际情况的医疗模式.本文就高校医院应如何为师生员工提供全方位的医疗保健服务进行了初步探讨.     

The Role of Magnetic Reconnection in CME Acceleration

Observations carried out from the coronagraphs on board space missions (LASCO/SOHO, Solar Maximum and Skylab) and ground-based facilities (HAO/Mauna Loa Observatory) show that coronal mass ejections (CMEs) can be classified into two classes based on their kinematics evolution. These two classes of CMEs are so-called fast and slow CMEs. The fast CME starts with a high initial speed that remains more or less constant; it is also called the constant-speed CME. On the other hand, the slow CME starts with a low initial speed, but shows a gradual acceleration; it is also called the accelerated and slow CME. Low and Zhang [Astrophys. J. 564, L53–L56, 2002] suggested that these two classes of CMEs could be a result of a difference in the initial topology of the magnetic fields associated with the underlying quiescent prominences. A normal prominence magnetic field topology will lead to a fast CME, while an inverse quiescent prominence results in a slow CME, because of the nature of the magnetic reconnection processes. In a recent study given by Wu et al. [Solar Phys. 225, 157–175, 2004], it was shown that an inverse quiescent prominence magnetic topology also could produce a fast CME. In this study, we perform a numerical MHD simulation for CMEs occurring in both normal and inverse quiescent prominence magnetic topology. This study demonstrates three major physical processes responsible for destabilization of these two types of prominence magnetic field topologies that can launch CMEs. These three initiation processes are identical to those used by Wu et al. [Solar Phys. 225, 157–175, 2004]. The simulations show that both fast and slow CMEs can be initiated from these two different types of magnetic topologies. However, the normal quiescent prominence magnetic topology does show the possibility for launching a reconnection island (or secondary O-line) that might be thought of as a “CME’’.