航天发射用磁悬浮助推发射系统概念研究

针对日益增加的航天发射成本问题和安全、可靠、低成本航天发射方式的需求,阐述了磁悬浮助推发射概念及其优越性.初步分析了磁悬浮助推发射系统组成及各分系统功能.通过比较电磁悬浮(EMS)和超导电动(EDS)两种磁悬浮系统性能,结果表明EDS是更适合于磁悬浮助推发射的磁悬浮系统方案.通过助推发射能量需求初步分析,直线电机加速能量供给系统是难题之一,需要重点解决.采用飞行弹道分析方法,说明地面助推水平起飞单级入轨运载器方案的可行性及特点.与其它航天助推发射方式比较,磁悬浮助推发射在提高入轨载荷和降低发射成本方面具有优势.     

A new parameter to define interplanetary coronal mass ejections

The interplanetary manifestations of coronal mass ejections, ICMEs, have many signatures in the solar wind but none of these signatures in the velocity, density, temperature, magnetic field, plasma composition or energetic particles uniquely and unambiguously identifies the occurrence of an ICME. Different investigators identify different events when confronted with the same data. Herein, we present a single physical parameter that combines information from multiple plasma components and that holds the promise of defining a beginning and an end of the region of influence ICME and an indication of the location of the encounter with the ICME relative to its central meridian. This parameter is the total plasma pressure perpendicular to the magnetic field, consisting of the sum of the magnetic pressure and plasma kinetic or thermal pressure. It provides a vehicle for classifying the nature of the ICME encounter and, in many cases, provides an unambiguous start and stop time of the event. However, it does not provide a start and stop time for any embedded flux rope. This identification depends on examination of the magnetic field.     

Force-free magnetic field in a cylindrical flux rope without a constant alpha

It is generally assumed that magnetic fields inside interplanetary magnetic clouds and flux ropes in the solar photosphere are force-free. In order to model such fields, the solution of rot B = B is commonly used where  = const. But comparisons of this solutions with observations show significant difference. To treat this problem,we examine the solutions with .     

The Magnetostatic Cleanliness Program for the Cassini Spacecraft

The Cassini spacecraft, launched in October 1997 and expected to reach Saturn in 2004, carries two magnetometer experiments on a 10-m boom, one at the mid-section of the boom and the other situated at the end of the boom. In order to gather valid scientific magnetic field data and avoid electromagnetic interference, the spacecraft had to comply with stringent magnetostatic cleanliness requirements. This paper describes the results of the Cassini magnetics cleanliness program that achieved the goal of minimizing the magnetic field interference with Cassini’s DC magnetic field science instruments.This revised version was published online in July 2005 with a corrected cover date.     

一般令牌网络的性能分析

提出了一般令牌网络的性能分析模型,在模型中,访问方式为“循环策略”,消息包到达各站点服从Ｐｏｉｓｓｏｎ分布,消息包到达率不完全相同,消息包长度既有常数也有负指数分布,根据随时过程的理论导出令牌循环时间Ｔ的均值和方差的一般解析表达式,同时应用排队论的方法进行一步分析了平均消息延时,平均消息长度和逻辑环路利用率。     

高灵敏度与高稳定性的飞机客舱内物品监测系统

介绍了一种新型的高稳定度、高灵敏度的飞机客舱内物品监测系统的工作原理和基本电路。该系统具有检测灵敏度高,抗干扰能力强,工作稳定可靠的特点。     

俯仰轴飞行品质时域准则计算和模拟

对于某些现代飞机采用等效系统准则评价飞行品质有困难时，新的规范提出了直接采用高阶系统时域响应准则，包括按驾驶员指令的俯仰速率响应来确定的Chalk准则以及按驾驶员指令的姿态和轨迹响应之间的相互关系来确定的Gibson准则；为避免错觉，还提出了驾驶员座位处法向过载的响应要求。在简要介绍了这些准则的背景和机理后，以某型飞机为例，按时域准则进行了计算和评价。     

基于滤波扩张观测器的有限时间收敛制导律

为提高拦截机动目标的精度,基于滤波扩张状态观测器提出了一种考虑自动驾驶动态特性的有限时间收敛制导律.通过滤波扩张状态观测器对制导律中目标机动信息进行补偿,使导弹在拦截目标时具有更高的拦截精度.仿真结果表明,在目标机动情况下,设计的制导律能保证视线角速度在有限时间内收敛到零,拦截弹过载较小,具有较好的动态特性和鲁棒性.同时与普通的扩张观测器的估计结果相比,滤波扩张状态观测器对机动目标的跟踪效果较佳.     

模糊实时控制在雷达伺服系统中的仿真与应用

从分析模糊控制器各参数与系统响应特性之间的关系出发，讨论了各参数在控制过程中的作用，并在此基础上提出了三段式模糊控制器（ 开关控制、基本模糊控制、自调参模糊控制） 。经计算机仿真和实时控制实验表明，三段式模糊控制器能显著减少甚至消除系统超调，对系统参数及结构变化不敏感，具有很强的鲁棒性，并能提高伺服系统的位置精度。     

VXI测控程序开发的几点经验

概要阐述了在某系统VXI测控程序开发过程中 ,遇到的几个主要问题 :WindowsNT的实时性、应用VISA库开发模件的驱动程序、寄存器状态的保存、加快串口通讯、程序自动化等 ,及其解决办法