The Local Bubble and Interstellar Material Near the Sun

The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun appears to be located in one of these flows of low density material. This nearby interstellar matter, dubbed the Local Fluff, has a bulk velocity of ∼19 km s⁻¹ in the local standard of rest. The flow is coming from the direction of the gas and dust ring formed where the Loop I supernova remnant merges into the LB. Optical polarization data suggest that the local interstellar magnetic field lines are draped over the heliosphere. A longstanding discrepancy between the high thermal pressure of plasma filling the LB and low thermal pressures in the embedded Local Fluff cloudlets is partially mitigated when the ram pressure component parallel to the cloudlet flow direction is included.     

基于VXI总线的发动机综合调节器自动测试系统的研制

介绍了某型发动机综合调节器自动测试系统的研制情况,并重点讲述了在系统开发过程中所使用的几项关键技术。     

Stellar flares

Radio and X-ray observations of stellar flares provide the most direct probes of energy relaase particle acceleration, and energy transport on stars other than the Sun. In this review, the observational basis for our understanding of the flare phenomenon on other stars is briefly described and outstanding interpretive and theoretical issues are discussed. I shall confine my attention to objects which are solar-like, to the extent that they possess deep convective envelopes and display activity which is presumed to be magnetic in origin. These include pre-main sequence objects, classical flare stars, and close binaries. Future directions are briefly discussed.     

利用改正数信息的北斗三号实时精密单点定位及性能分析

北斗三号全球卫星导航系统已正式建成并开通服务。为了利用实时改正数信息系统地揭示北斗三号精密单点定位性能，并为用户提供理论依据和应用参考，首先解算了卫星实时精密轨道、钟差及其改正数，分析了其精度。然后基于实时改正数信息，利用监测站广播星历和观测数据，分别进行了双频静态、双频仿动态、单频静态和单频仿动态仿实时精密单点定位，以评估其性能。结果表明：北斗三号MEO卫星实时轨道和钟差精度均值分别约为12cm和0.2ns，满足实时精密单点定位需求。静态实时精密单点定位精度优于动态，双频优于单频，均可达到分米级。对于定位收敛时间，双频静态最短，约为40min；双频动态和单频静态均约为85min；单频动态最长，约为120min。     

面向对象的航空工程试验数据资源管理

针对目前工程试验数据管理中存在的问题，提出了基于面向对象数据模型的航空工程试验数据资源管理系统的设计思想和实现方法，说明了测试数据模型的对象模式，详细描述数据库表的设计，并给出应用实例。     

欧洲返回舱CTV气动特性综述

研究分析了欧洲航天局天地往返运输系统之载人飞船返回舱CTV的气动特性，并与第一代联盟号飞船返回舱的气动特性作了对比研究。该返回舱为钝双锥外形，与联盟号飞船返回舱相比，它具有升阻比高、机动性强、稳定性好等特点。本文还对两类返回舱的气动热特性、防热材料重量、飞行弹道及通讯中断问题进行了对比分析研究。     

无人驾驶高空侦察机爬升控制方案分析

介绍了无人驾驶高空侦察机（ＵＡＶ）的爬升轨迹控制方案原理，对纵向控制回路进行了详细分析，按简单拉力法进行了飞行性能计算，同时还分析了爬升方案曲线与优化性能轨迹的关系，并对爬升轨迹计算和试飞遥测数据进行了比较。经分析计算与试飞结果表明，对于爬升较缓慢的飞机，本控制方案可实现沿优化性能轨迹上升，并自动转入有利速度巡航。     

一种新颖的瞬时浮点放大器

介绍了瞬时浮点放大器的原理及构成，并给出一种结构新的具有２５６阶的瞬时浮点放大器，可有效地提高数据采集系统的测量范围。     

废气排放塔尾流区随机游动扩散模拟研究

本文对一种建筑结构与形式特异的废气排放源－过江隧道风井塔，进行了如下研究：（１）在环境风洞中通过风井塔后流场的测量，分析给出塔后尾流特征，并进行示踪气体扩散模拟试验和烟云照相；（２）在上述工作基础上，建立一个先进的随机游动扩散模式，模拟尾流区污染物扩散的基本规律，模式计算结果与实验结果吻合较好。建筑物的存在使得地面最大浓度增大３￣４倍，且出现位置离源更近。研究表明，随机游动方法研究对有明显湍流不均     

The Plasma Environment of Comet 67P/Churyumov-Gerasimenko Throughout the Rosetta Main Mission

The plasma environment of comet 67P/Churyumov-Gerasimenko, the Rosetta mission target comet, is explored over a range of heliocentric distances throughout the mission: 3.25 AU (Rosetta instruments on), 2.7 AU (Lander down), 2.0 AU, and 1.3 AU (perihelion). Because of the large range of gas production rates, we have used both a fluid-based magnetohydrodynamic (MHD) model as well as a semi-kinetic hybrid particle model to study the plasma distribution. We describe the variation in plasma environs over the mission as well as the differences between the two modeling approaches under different conditions. In addition, we present results from a field aligned, two-stream transport electron model of the suprathermal electron flux when the comet is near perihelion.