肯尼迪航天中心的雷电防护系统

本文是美国NASA/肯尼迪航天中心(KSC)于1990年6月公布的雷电与空间计划。它全面地介绍了NASA/KSC研究雷电与大气电场的概况。NASA/KSC应用了综合的、先进的监测技术手段,制定了广泛的、严谨的和有效的防护措施,确保了飞行器及发射场地的安全。文章还介绍了雷电探测、预报、防护和研究的前景。     

怎样写好学术论文

首先阐明学术论文的重要性和它的作用，接着主要阐明纲要拟制和反复修改是撰写论文的主要工作；介绍怎样拟制纲要；详细列出纲要所包含的内容及拟制中的要点。作者没有就论文的全文撰写作专门的阐述，只是在拟制纲要的阐述中点拔一二。最后作者提出可从三类参考文献中得到拟定论文的启发。     

广播内存实时网节点卡的LabVIEW驱动开发

广播内存实时网技术是一种高效的网络数据传输技术。本文向读者介绍了LabVIEW环境下利用CIN技术的网络内存节点卡驱动模块的设计方法。     

运用进化算法优化中等PRF雷达的脉冲重复频率

本文运用进化算法选择最佳脉冲重复频率（PRF）组，在中PRF雷达的模型中使距离-多普勒盲区最小。介绍了8个和9个PRF的两个方案，该算法能确保得到的所有结果是完全可解码的并且没有盲速。我们考虑了旁瓣杂波的详细影响以及在以中等PRF模式运行的实际机载火控雷达中影响雷达PRF选择的多个技术因素。     

复合推进剂热降解机理的研究

为了系统地研究氧化剂在复合推进剂热降解过程中的作用曾作过试验计划。主要分析工具是扫描式电子显微镜(SEM),用以检测推进剂试样热降解破裂部位。试验配方变量为氧化剂纯度、粒度和氧化剂一粘合剂的粘结剂。整个试验期间粘合剂保持不变,均为饱和碳氢化合物。氧化剂为纯高氯酸铵、含氯酸盐的高氯酸铵、含砷酸盐的高氯酸铵和含磷酸盐的高氯酸铵。氧化剂粒度分布为:粗粒度60%,细粒度40%,采用两种二级配混合物;125—175 μ/<44 μ和175—250 μ/44—88 μ。用粘结剂时,其用量为0.15%左右。试验变量为温度和应力,温度用100℃、135℃和170℃,应力用0.29公斤/厘米~2和0.61公斤/厘米~2。试验数据表明,氧化剂纯度和粒度对热降解过程有显著影响。在高温和应力作用下,氧化剂粒度影响较大。用扫描式电子显微镜检查推进剂破裂部位表明,大颗粒氧化剂的破碎导致推进剂龟裂。     

MX导弹喷管用先进材料评论

目前正在进行研制石墨材料,准备用于MX 第一级和第二级固体火箭喷管的入口部,喉部,后喉部,出口锥和可延伸出口锥。这些材料必须经受住新型洲际弹道导弹(ICBM)喷管系统的苛刻的结构、化学侵蚀,粒子冲刷和高温环境。该系统的燃烧室压力可达127公斤/厘米~2,火焰温度为3700°K 至3922°K。叙述了第一级和第二级全尺寸试验喷管的现状。还提出了在喷管设计、石墨材料研制以及预期性能改进方面进一步工作的方向。     

现代谱分析技术综述

本文综述了最近20年推出的有关离散时序谱分析的新方法。对每个方法所假设的基本时序模型作的分析,构成本文了解各种谱分析方法之间差别的共同基础。所讨论的方法包括经典的周期图法、经典的 Blackman-Tukey 法、自回归(最大熵)法、滑动平均法、自回归滑动平均法、最大似然法、Prony 法和 Pisarenko 法。正文中的一览表对所有方法作了简要的评述,包括基本的参考文献和计算每一谱估计的相应公式     

SQL Server对XML文档的数据抽取方法的分析与实现

XML正在逐步成为新一代Web数据描述和数据交换标准,将XML文档中的数据抽取到关系数据库中进行管理,可以极大的提高数据的使用效率。本文针对SQL Server对XML文档的数据抽取方法的原理进行了分析,并提出了具体的实现方法。     

Research priorities and plans for the International Space Station-results of the 'REMAP' Task Force

Recent events in the International Space Station (ISS) Program have resulted in the necessity to re-examine the research priorities and research plans for future years. Due to both technical and fiscal resource constraints expected on the International Space Station, it is imperative that research priorities be carefully reviewed and clearly articulated. In consultation with OSTP and the Office of Management and budget (OMB), NASA's Office of Biological and Physical Research (OBPR) assembled an ad-hoc external advisory committee, the Biological and Physical Research Maximization and Prioritization (REMAP) Task Force. This paper describes the outcome of the Task Force and how it is being used to define a roadmap for near and long-term Biological and Physical Research objectives that supports NASA's Vision and Mission. Additionally, the paper discusses further prioritizations that were necessitated by budget and ISS resource constraints in order to maximize utilization of the International Space Station. Finally, a process has been developed to integrate the requirements for this prioritized research with other agency requirements to develop an integrated ISS assembly and utilization plan that maximizes scientific output.     

Climate model studies of synchronously rotating planets

M stars constitute 75% of main sequence stars though, until recently, their star systems have not been considered suitable places for habitable planets to exist. In this study the climate of a synchronously rotating planet around an M dwarf star is evaluated using a three-dimensional global atmospheric circulation model. The presence of clouds and evaporative cooling at the surface of the planet result in a cooler surface temperature at the subsolar point. Water ice forms at the polar regions and on the dark side, where the minimum temperature lies between -30 degrees C and 0 degrees C. As expected, rainfall is extremely high on the starlit side and extremely low on the dark side. The presence of a dry continent causes higher temperatures on the dayside, and allows accumulation of snow on the nightside. The absence of any oceans leads to higher day-night temperature differences, consistent with previous work. The present study reinforces recent conclusions that synchronously rotating planets within the circumstellar habitable zones of M dwarf stars should be habitable, and therefore M dwarf systems should not be excluded in future searches for exoplanets.