航天飞行器中舷窗温度场及换热的研究：外部界面处于第三类非线性边界条件

本文采用控制容积法,光线踪迹法结合谱带模型,研究航天飞机返回大气层时舷窗硅玻璃的非稳态复合换热。文章给出了界面S_2处于第三类非线性边界条件下,舷窗硅玻璃内部的温度场和进入机舱内部的热流密度。计算结果表明,如不考虑硅玻璃内部的辐射作用,对温度场影响不太大,但对进入机舱内的热流密度将会产生很大的误差。     

《液压与气动》课程教学的方法的探讨

文章结合实际课程特点、教学对象和培养目标,以《液压传动与气动》的课堂教学为例,浅谈几点课程教学方法:精选教学内容;采用动画教学;采用引导教学和理论和实例结合等,这些方法有助于提高教学质量,推动现代课堂教学改革。     

用高速纹影摄影技术观测自由面微物质的喷射

本文介绍了适于爆轰实验研究的透射式高速纹影仪。该设备具有较高的测试灵敏度。应用它观测了铅和钢样品自由面的微物质喷射现象,取得了好的结果。     

高教机天线布局影响通讯距离研究与改进

某型高级教练机在试飞中,出现空地通讯距离不满足战技指标要求的问题。经过分析发现,由于超短波电台天线作为单极天线,其安装布局未满足天线本身要求,即接地面尺寸过小、近场区环境复杂等,导致天线辐射性能受到影响。本文对天线阻抗和方向性系数进行了研究分析,并根据飞机情况制定相应的改进方案。     

The Role of Magnetic Reconnection in CME Acceleration

Observations carried out from the coronagraphs on board space missions (LASCO/SOHO, Solar Maximum and Skylab) and ground-based facilities (HAO/Mauna Loa Observatory) show that coronal mass ejections (CMEs) can be classified into two classes based on their kinematics evolution. These two classes of CMEs are so-called fast and slow CMEs. The fast CME starts with a high initial speed that remains more or less constant; it is also called the constant-speed CME. On the other hand, the slow CME starts with a low initial speed, but shows a gradual acceleration; it is also called the accelerated and slow CME. Low and Zhang [Astrophys. J. 564, L53–L56, 2002] suggested that these two classes of CMEs could be a result of a difference in the initial topology of the magnetic fields associated with the underlying quiescent prominences. A normal prominence magnetic field topology will lead to a fast CME, while an inverse quiescent prominence results in a slow CME, because of the nature of the magnetic reconnection processes. In a recent study given by Wu et al. [Solar Phys. 225, 157–175, 2004], it was shown that an inverse quiescent prominence magnetic topology also could produce a fast CME. In this study, we perform a numerical MHD simulation for CMEs occurring in both normal and inverse quiescent prominence magnetic topology. This study demonstrates three major physical processes responsible for destabilization of these two types of prominence magnetic field topologies that can launch CMEs. These three initiation processes are identical to those used by Wu et al. [Solar Phys. 225, 157–175, 2004]. The simulations show that both fast and slow CMEs can be initiated from these two different types of magnetic topologies. However, the normal quiescent prominence magnetic topology does show the possibility for launching a reconnection island (or secondary O-line) that might be thought of as a “CME’’.     

大口径远程榴弹气动力-外弹道综合优化设计

在大口径远程榴弹设计中,在保证弹丸具有足够的威力,飞行稳定性和发射强度的前提下,使弹丸具有最大射程是一个很有意义的问题。本文给出了大口径远程榴弹气动力一外弹道综合优化设计数学模型,本文还首次涉及了底部排气弹外形优化问题。     

硝化纤维素溶冰冻过程中的折光指数增量

用定量体积排斥色谱（ＳＥＣ）的方法,以示差分析检测器的响应为基础,测定了硝化纤维素溶液冰冻及其加热以后的折光指数增量,结果表明,冰冻后,由于分子链发生链内聚聚（缠结）硝化纤维素分子链周围溶剂化溶剂分子数减少,使硝化纤维素溶液的示差折光指数增量增加,加热后,由于硝化纤维素分子链获得能量,链内缠结点解开,溶剂化溶剂分子数增加,造成硝化纤维素溶液的折光指数增量降低,由此建立了以折光指数增量为基础,估算经     

催化点火器高空点火性能的实验研究

介绍国产催化点火器高空点火性能模拟试验,主气流温度为５００℃左右、加力室压力为０．０４—０．１２ＭＰａ,对催化点火器的着火延迟时间和贫富油点火极限进行了测量。试验结果表明：当飞行高度为１７０００—１７５００ｍ,飞行马赫数Ｍａ＝１．０时,催化点火器可以正常点燃某型发动机加力燃烧室。