IEEE488总线在动量轮测试中的应用

叙述了资源卫星动量轮的一般结构和开环测试原理。详细介绍了应用ＩＥＥＥ４８８总线构成的动量轮开环性能自动测试系统。说明了这个自动测试系统的系统构成以及测试项目、测试流程和获得的测试结果。并据此提出这个系统在卫星研制工作中具有推广价值。     

基于目标操作化的多引擎协作体系结构研究

基于目标操作化的域原子操作模型,研究分析了面向应用目标的系统设计与实现的基本问题,通过引入解释引擎,提出了面向目标的形式模型与应用软件设计实现的一体化机制;在系统级应用中间件之上,引入组件服务,提出了一个通过处理操作作业流实现目标的、多个操作服务引擎协作的体系结构,通过构造组件适配器,以满足操作服务引擎对异构组件服务的一致性访问.     

地中式混凝土油罐的数值模拟

对正在开展的战略石油储备,提出用地中预应力混凝土罐进行石油储存.应用结构分析软件ANSYS对巨型混凝土单壁罐和双壁罐进行弹性分析,指出罐壁环向应力几乎全部由温度荷载造成,罐壁温度场和温度应力具有明显时间性,储油初期罐壁温差最大,96?h后罐壁顶部拉应力达到最大;设置中间保温层后,内罐应力减小,外罐应力增大,应对内、外罐连接支墩做特殊设计,以满足罐壁温度变形.     

部分开放多极磁场中的日冕磁绳灾变

采用球坐标下二维三分量理想MHD模型，研究部分开放多极背景磁场中日冕磁绳的灾变现象．背景磁场由含3个闭合双极场的冕流和带赤道中性电流片的开放场构成，磁绳位于中心双极场的下方，其特性由环向磁通和轴向磁通表征．对给定的环向磁通，存在轴向磁通的一个临界值；对给定的轴向磁通，也存在环向磁通的一个临界值．在该临界值以下，磁绳附着于太阳表面，系统处于平衡状态；该临界值一旦被超越，磁绳将脱离太阳表面向上喷发，说明部分开放多极背景磁场中的日冕磁绳系统存在灾变现象．本文算例表明，灾变点对应的磁能阈值超过对应部分开放场(中心双极场开放，两侧的双极场仍维持闭合)能量约15％，其超过部分可为日冕物质抛射一类太阳爆发提供能源．     

Changes in spectral reflectance of wheat leaves in response to specific macronutrient deficiency.

In wheat (Triticum aestivum L.) plants, deficiency of an essential element may drastically affect growth, appearance, and most importantly yield. Wheat, the focus of this study, is one of the crops studied in the CELSS program. Information about nutrient deficiencies in crops grown in controlled environment is essential to optimize food productivity. The main objective of this study was to determine whether deficiency of Nitrogen (N), Phosphorus (P), Potassium (K), Calcium (Ca) and Magnesium (M) alters spectral reflectance properties of wheat leaves. Plants were grown in the greenhouse and growth chamber, in a modified Hoagland's nutrient solution. Spectral reflectance of fully expanded wheat leaves from 280 to 1100 nm, nutrient concentrations (N, P, K, and Ca) and chlorophyll (Chl) were determined when deficiency symptoms were first evident (approximately 6-7 weeks). Chlorophyll content and fresh and dry weight, were used to assess the severity of the nutrient stress. All nutrient deficiencies affected chlorophyll content and generally increased reflectance in the visible (VIS) 400-700 nm and infrared (IR) 700-1100 nm ranges. Magnesium and nitrogen deficiencies had the most pronounced effect on chlorophyll concentration height, and reflectance. All macronutrient deficiencies tested reduced chlorophyll concentration, increase reflectance in the visible range and caused a shift in the position of the red edge (the point of maximum slope on the reflectance spectrum of vegetation between red and near-infrared wavelengths) toward shorter or longer wavelengths; depending upon the element. In the greenhouse, N and Mg induced the greatest increase in reflectance of 33% and 25% in the VI range and 86% and 53% in the IR range, respectively. However, in the growth chamber, an increase of 97% and 25% occurred in the VI range, and 20% and 33% in the IR range, respectively. In the IR range in the growth chamber, P, K, and Ca deficiency caused a reduction in reflectance (412-770 nm). This research indicates that mineral deficiencies and reflectance are not specific to one environment and could have important implications for the design of CELSS in space, and perhaps the future of terrestrial agriculture.     

过失速飞机最速指向目标机动研究

基于飞机质点动力学模型建立了指向活动目标的终端条件,并进行最速指向机动动作的数值优化,其中用共轭梯度法寻优,用罚函数处理约束条件.计算结果表明,优化可以指导寻找对应于不同战术要求的有利机动过程;在近距空战中,具有快速改变航迹方向并进入过失速超大迎角机动的能力非常有利于快速指向目标、争取首攻机会,而改变航迹方向倾向于使用最大升力区迎角.     

汽车模拟覆盖件的相位法测量

简述了相位法曲面全场无接触三维测量的基本原理，针对为汽车车顶抗凹性能研究而制作的模拟覆盖件的外形测量要求，设计了相位法三维测量的光学成象系统与图象处理系统，并应用到汽车模拟覆盖件的外形测量，测量结果与三坐标所测结果相近，说明了该测量系统的精确性。     

南极长城站电离层变化的数值模拟

南极长城站夏季电离层日变化具有Weddell海异常现象．本文利用一个一维时变理论模式，对长城站夏季电离层f0F2和hm日变化进行了数值模拟.我们讨论了中性风和顶部输运通量对f0F2和hm的影响，认为模拟计算得到的f0F2值比实测值要大的一个主要原因是国际参考电离层给出的上边界值偏大.文章最后介绍了一个获得实际的f0F2和hm的方法.     

空间飞行体与等离子体在压缩区内的非稳态相互作用研究

研究了空间飞行体在运动过程中，其前端压缩区内飞行体与等离子体的、非稳态相互作用问题，得到了在强天线辐射源高频场作用下的控制方程．通过计算表明，飞行体上的天线可作为调制不稳定性的激发源，在等离子体中激发起很强的电磁孤波．     

HZE-dosimetry on MIR92, IML-1 and D-2

Nuclear track detectors were used to measure the integral Linear Energy Transfer (LET) spectra above 1 GeV per cm water behind the complex material shielding inside a spacecraft. The measurements are compared with predictions of the contribution of high charge, high energy HZE particles of the galactic cosmic radiation taking into account the influence of solar and geomagnetic modulation and shielding by matter.