历经十年寿命试验的消旋天线机构轴承的可靠性分析

解决了一个计算可靠性问题的特例。分析了消旋天线机构轴承历经10年寿命试验的可靠性问题。并给出了轴承在不同可靠寿命要求下的可靠度(对应不同置信度)。     

气动力星座保持的闭环控制研究

本文研究了利用气动力进行星座保持的闭环控制问题。提出了一种改进的半全局指数收敛闭环控制律，对于指定的任意大的有界域，利用不变集定理论上证明了该控制律的稳定性和抗干扰性，又提出了双ε法以提高响应速度。     

杨振宁的科学研究艺术

杨振宁教授是位著名的物理学家，诺贝尔物理学奖金获得者。他在物理学研究中取得的成就同科学研究的艺术是分不开的。本文分析了如下三个问题：第一“对称性支配相互作用”与杨米尔斯规范场理论；第二，科学研究中的风格和ｔａｓｔｅ；第三，科学研究方向的选择。该文无论是对年青的研究还是对成熟的学者从事科学研究都有指导意义。     

SCP－1型贴片机PLC程序的设计

介绍了在研制ＳＣＰ－１型贴片机过程中，采用可编程控制器（ＰＬＣ）对各外设进行控制的程序编制过程。着重分析了串行口通讯协议的设置，并以吸片过程为例，具体地说明了ＰＬＣ程序的编制方法。     

Implementation of a three-phase high-power-factor rectifier with NPC topology

A three-phase four-wire power factor corrector based on neutral-point-clamped (NPC) topology is adopted to reduce the current harmonics and increase the input power factor. Using the NPC topology, the voltage stress of power switches can be reduced to the half of the dc-link voltage. With the dc-link voltage controller and the phase locked loop circuit, the balanced and sinusoidal line currents can be drawn from the ac supply system under the balance and unbalance mains voltages. The hysteresis current comparators are adopted in the current control loop to track the line current commands. Three voltage levels are generated on the ac terminal to the neutral point. Simulations and experiments are provided to verify the validity and the effectiveness of the proposed control scheme.     

阻尼材料在飞机炮振减振上的应用

阻尼材料在飞机结构上的应用是一个新课题。在飞机炮舱区应用新型阻尼材料,组成一个全新的阻尼结构系统来吸收由航炮射击时产生的冲击能量,以实现减振的设计目的,进而改善其炮击的振动环境。通过理论计算和地面试验实测,证明了应用新型阻尼材料可使炮舱区的动应力下降近30％。     

J—7LP飞机1：6遥控模型失速尾旋试验

对无动力J—7LP动力学缩比模型进行了遥控试飞,以研究其失速尾旋特性,全偏平尾和方向舵可使模型进八尾旋,舵面全回中即可从各种尾旋中改出。偏转副翼对尾旋特性有明显的影响。     

三维模型中关键特性标注和提取的实现

关键特性作为"少数重要"的产品信息,是保证产品质量和顾客满意度的重要因素,其指定和标识需要与三维模型相结合才具有更直观的意义,同时也方便对其进行更有效的管理.本文给出了关键特性的定义和分类,提出了三维模型中关键特性的标注方法,通过对UG进行二次开发,实现了关键特性的属性添加和信息提取,并通过某型导弹弹头舱段壳体零件进行了验证.     

心有芊芊竹——竹之节

竹，是草，但却不像草那般纤细柔弱；竹，不是树，却拥有与树一般的高度。于是，在这是与不是中，中国人赋予了竹太多的内涵，充盈着它虚空的竹节。     

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.