单流体二维太阳风结构的磁流体力学模拟

在添加动量项的条件下，对单流体二维磁流体力学方程组进行模拟，得到了子午面上的太阳风结构，结果表明，添加动量项的形式及其被加入的位置对远区太阳风速度和质子密度有重要的影响。本文在适当的区域加入合适的动量项得出了远区太阳风速和质子密度与Ulysses观测基本符合的结果。文中给出了较合适的动量添加区域为3.5-10Rs(Rs为太阳半径）。     

“嫦娥二号”卫星L2点角动量管理

对“嫦娥二号”(CE-2)卫星进入环绕日地拉格朗日L2点的李萨如轨道后卫星喷气卸载所产生的影响进行了研究.提出了一种利用光压力矩辅助卫星太阳电池翼角度调整进行角动量管理的方法.在轨试验表明,太阳光压强度足够对飞行在L2点环绕轨道上的CE-2卫星进行角动量管理,可以大幅度减少动量轮在轨喷气卸载的次数,有利于CE-2卫星的轨道维持.     

数控机床加工一体化课程改革研究

数控机床加工“一体化”课程主要是从教学内容“一体化”、教师素质“多元化”及教学与管理“一体化”等方面进行改革。课程内容根据工业生产中常见的回转体和结构件为工作任务,根据知识能力的递进关系再细化任务,使学生在学习过程中容易接受。     

高焓风洞中钝体近尾流红外辐射测试技术

介绍在JF-10氢氧爆轰驱动高焓激波风洞中开展再人流场红外辐射测量的实验技术。风洞试验状态的驻室总压为19．6MPa，驻室总温为7920K。实验以球头钝锥体为试验模型，测量其近尾流红外辐射能量通量的横向分布。测量采用插入式锑化铟多元红外成像系统，波段范围为2．27-6．0μm。试验数据呈现明显的规律性。试验结果表明：利用这一测量技术能够提供高焓条件下有较高空间分辨率的、较为准确的红外实验数据。     

装有多孔介质的封闭腔体中热驱动换热的数值研究

以涡轮叶片超级冷却技术为研究背景,用数值计算的方法,模拟了离心力场下装有多孔介质的封闭腔体中的热驱动换热现象。计算结果表明,在封闭腔体中加入大孔隙率多孔介质后确实能起到强化换热的效果,采用的固体介质的导热性越好,封闭腔体中流体的热驱动能力越强,换热效果越好。而且采用导热性比较好的固体介质时,在大孔隙率范围内,随着孔隙率的减少,封闭腔体中流体的热驱动能力和换热均得到增强。     

Gravity wave momentum flux generation close to mid-latitude Andes in mesoscale simulations of late 20th and 21st centuries

Adequate representations of diverse dynamical processes in general circulation models (GCM) are necessary to obtain reliable simulations of the present and the future. The parameterization of orographic gravity wave drag (GWD) is one of the critical components of GCM. It is therefore convenient to evaluate whether standard orographic GWD parameterizations are appropriate. One alternative is to study the generation of gravity waves (GW) with horizontal resolutions that are higher than those used in current GCM simulations. Here we assess the seasonal pattern of topographic GW momentum flux (GWMF) generation for the late 20th and 21st centuries in a downscaling using the Rossby Centre regional atmospheric model under the Intergovernmental Panel on Climate Change A1B emission conditions. We focus on one of the world’s strongest extra-tropical GW zones, the Andes Mountains at mid-latitudes in the Southern Hemisphere. The presence of two GCM sub-grid scale structures locally contributing to GWMF (one positive and one negative) is found to the East of the mountains. For the late 21st century the strength of these structures during the GW high season increases around 23% with respect to the late 20th century, but the GWMF average over GCM grid cell scales remains negative and nearly constant around −0.015 Pa. This constitutes a steady significant contribution during GW high season, which is not related to the GWMF released by individual sporadic strong GW events. This characteristic agrees with the fact that no statistically significant variation in GWMF at source level has been observed in recent GCM simulations of atmospheric change induced by increases in greenhouse gases.     

多自由度动量交换技术研究的新进展

航天器三轴姿态控制常用的多飞轮控制方案中,反作用飞轮的单自由度动量交换属性使系统的功能重复部件和冗余件数目增多,严重影响了姿控系统的重量、体积、功耗及成本;由于原理和结构的限制,传统多自由度动量交换技术无法充分发挥其“多自由度”的固有优势,而新型多自由度动量交换技术的研究与发展则为这一优势的发挥提供了空间。本文综述了国内外多自由度动量交换技术研究的新进展,分析了其特点、关键技术和研究方向,并展望其应用前景。     

一种新型空间微小碎片超高速碰撞试验地面模拟方法

文章简要叙述了空间微小碎片环境及其对航天器的影响,同时介绍了一种新型空间微小碎片超高速碰撞地面模拟方法——激光驱动飞片技术。     

基于双框架控制力矩陀螺的航天器动量管理

为减小维持大型航天器的姿态稳定和降低能量消耗的动量管理中的扰动力矩对姿态稳定的干扰,设计了周期性抑制滤波器。姿态控制的执行机构采用双框架控制力矩陀螺群（DGCMGs）,应用KENNEL操纵率,使航天器执行机构的角动量在本体系的x轴分量和偏航角可达稳定,同时角动量在本体系的z轴分量和滚转角可在较小的范围内振荡。数值仿真结果验证了方案的可行性。     

Stellar winds of massive stars in M31

We have obtained the first UV high resolution spectra of hot luminous stars in M31 with the FOS onHubble Space Telescope. The spectra, combined with optical spectroscopic and photometric observations, enable us to study their stellar winds and photospheric parameters. We derive mass-loss rates and velocity laws from the wind line profiles, with the SEI method, as well as information on abundances. The wind lines and photospheric spectra are compared with galactic stars of the same spectral type.The spectra analyzed so far indicate that the stars have mass-loss rates comparable or slightly lower than galactic stars of the same spectral type, but possibly different velocity laws in their winds. The spectra of two stars are discussed here.