三轴稳定遥感卫星姿控系统故障情况下的系统重构

论述三轴对地稳定遥感卫星姿控系统中部分轮子或部分陀螺故障情况下的姿控系统重构。文中论述了只在俯仰通道有一偏置动量轮正常工作，而滚动和偏航通道轮子故障条件下的系统重构。另外还论述了偏航陀螺故障，姿控系统其它部件正常情况下，控制系统采用Whecon原理与PIM控制相结合的设计。以上两种系统重构拟用于实际系统中，经过数学仿真验证，姿控系统在故障情况下能够完成基本任务。     

基于仿真的单元化制造系统的单元分组

在传统单元分组方法的基础上,提出了用仿真方法解决瓶颈机床的分组问题.采用着色Petri网,对生产系统建模.以BEA算法作为分组基础,经过仿真试验得到最终的单元分组结果.试验表明,用仿真的方法能够弥补传统分组算法复杂的缺点.     

数控系统内置式PLC的FPGA实现方法

提出了一种用FPGA实现数控系统内置式PLC的方法.通过在FPGA内部实现PLC逻辑,并提供能够编译PLC指令的编译器,实现了数控系统对通用PLC编程语言的支持.所述方法在基于ARM FPGA的数控系统上得到了实现.     

CDMA网络中CQT定点测试排除掉话故障分析

CDMA网络的建设过程中由于规划、硬件问题、软件参数设置等造成个别地区通话质量差、掉话率高等问题,网络优化人员可以通过后台参数分析、后台信令分析、现场测试等辅助手段排除网络故障。在故障发生地点通过现场定点测试定位故障是处理此类用户故障投诉的较好方法。论文尝试通过测试软件CQT定点测试法分析CDMA网络中典型掉话故障。     

培养学生英语口语交际能力的策略探讨

文章就大学生英语口语交际能力存在的问题进行了分析,探讨如何提高英语口语交际能力的策略。     

空战机动动作库设计方式研究

具体阐述了两类常见空战动作库的设计 :典型战术动作库和基本操作动作库 ,详细分析了这两类空战机动动作库的不足 ,最后提出了改进动作库设计的具体意见和建议。     

延长热电池寿命的途径探讨

从防空导弹地面电源－－热电池的热设计和工艺角度出发，分析影响电池工作寿命的因素，提出延长电池工作寿命的三条途径：合理控制热电池的内部热量；提高加热片的均匀性；合理选择外保温材料。实践证明，这些途径是可行的。     

数字人感系统的研究

随着飞机模拟器技术的发展,电机伺服系统在人感系统中也得到了广泛的应用。本文着重讨论 了以DSP芯片为核心的数字人感系统组成和工作原理,并分析了系统的特点及功能。     

数字式射击瞄准计算机设计与实现

某型射击军械系统的射瞄计算机原采用模拟机电式技术实现,存在体积大、功耗大、可靠性及可维护性差等缺点,因此,使用数字式计算机技术对其进行升级改造势在必行.本文首先对原系统的火控原理及火控构型的进行了分析;其次,介绍了射击瞄准计算机的对外接口关系.重点介绍了数字式射击瞄准计算机的采样解算时间的确定、计算方法的选取及接口设计等内容.本文所设计的数字式射击瞄准计算机已通过了系统验证并得到了使用,克服了原有系统所存在的固有缺点.文中的设计思想与所用的工程方法对类似武器系统的升级改造有所借鉴.     

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.