Hamilton圈问题的DNA算法

基于目前可以使用的DNA实验技术并采用试管与表面相结合的方式,设计了解决H am ilton圈问题的DNA算法;详细地介绍了对图的顶点和边的分子编码;描述了算法的生物化学实现过程。由于采用了有控的部分穷举策略,因而既提高了解的可靠性,又抑制了大量伪解的产生。最后,讨论了算法的性能特点并指出进一步的研究方向。     

铸造诚信 职业之魂

我国诚信文化传统与社会现实中的信用缺失现象均表明诚信教育的必要性，现代企业文化建设展示了加强诚信教育的现实性，职业教育必须适应现代企业的客观需要，大力加强诚信教育。努力构建诚信的社会、和谐的社会。     

复合固体推进剂颗粒相互作用的增强效应分析

应用Ｅｓｈｅｌｂｙ－Ｍｏｒｉ－Ｔａｎａｋａ的细观力学理论，考虑两种类型颗粒之间相互作用的影响，从颗粒与基体的本构关系出发，计入更多的微细观信息，从而建立了更加合理的复合固体推进剂线粘弹本构方程。     

应用粒子激光散射测量混合反应器分散相浓度场分布

研究了圆管反应器中四束侧向对撞射流与轴向流形成的混合流动.应用激光粒子散射成像测量了侧向分散相在混合流中的浓度场分布,得到了不同的浓度分布图形随侧向流与轴向流速比关系,揭示了内在有规律的独特的浓度分布结构.     

星载QPSK解调器热环境试验性能分析及改进

文章首先给出热学环境试验下解调器主要性能指标如误码率、时钟环及载波环捕获带的变化,然后通过试验进行分析,最后提出改进措施。     

CCSDS高级在轨系统复接业务性能的分析

本论文分析了空间链路子网上的异步业务特别是复接业务的性能，建立了一种异步信息模型，从而解决了平均包延迟，帧效率的问题。这个结果也适用于各种不同的信息配置下可获得的系统性能的上、下限。而且，本文还讨论了一组与执行相关的参数，如帧完成暂停时间（ｆｒａｍｅｃｏｍｐｌｅｔｉｏｎｔｉｍｅ＿ｏｕｔｐｅｒｉｏｄ），分析了它们对系统性能的影响     

Project Icarus: Optimisation of nuclear fusion propulsion for interstellar missions

The Daedalus spacecraft design was a two-stage configuration carrying 50,000 tonnes of DHe³ propellant. Daedalus was powered by electron driven Inertial Confinement Fusion (ICF) to implode the pellets at a frequency of 250 Hz. The mission was to Barnard's star 5.9 light years away in a duration of around 50 years. This paper is related to the successor Project Icarus, a theoretical engineering design study that began on 30 September 2009 and is a joint initiative between the Tau Zero Foundation and The British Interplanetary Society. In the first part of this paper, we explore ‘flyby’ variations on the Daedalus propellant utilisation for two different mission targets: Barnard's star and Epsilon Eridani, 10.7 light years away. With a fixed propellant mass a number of staged configurations (1–4) are derived for an optimal configuration but then moving to an off-optimal configuration due to the requirement for a high final science payload mass. Some comments are then made on the ICF pellet configuration compared to the typical pellets fielded at the National Ignition Facility (NIF) and those proposed for the Vista and Longshot fusion based propulsion designs. This is a working progress report, which aims to study perturbations of the Daedalus baseline design as part of a trade study. This is a submission of the Project Icarus Study Group.     

航空发动机燃油分布器故障分析与参数优化

燃油分布器对供给发动机的燃油流量进行调节,进而改变发动机的转子转速、涡轮前温度等状态参数,它的工作特性也影响着发动机的加速性、稳定性等性能参数。在发动机地面台架试车过程中,发动机出现了转速下掉的故障,初步认为是燃油分布器工作不正常导致的。在对该型燃油分布器工作原理分析的基础上,利用AMESim软件构建相应的仿真模型,再现了工程实践中出现的发动机转速掉转的故障现象,分析并对其结构参数进行了优化。仿真结果为排故、系统的性能了解和改善提供了技术依据,本项研究已经成功应用于工程实践。     

吸气式脉冲爆震发动机壁温试验

为了探索各频率下管壁温度随时间的变化趋势及爆震管外壁面的温度分布规律,对爆震室内径68mm,长2 000mm,以汽油为燃料、空气为氧化剂的吸气式脉冲爆震发动机进行试验,用热成像仪对稳定工作在10Hz,20Hz,40Hz下的管壁温度进行了监测。结果表明:同一频率下随时间的增加壁面温度增加速度减小;热平衡时壁面温度随频率的增加而增长,10Hz,20Hz,40Hz热平衡时外壁面最高温度分别在726℃,1011.5℃,1159.5℃以上;热平衡前管壁温度的增长速度随频率的增加而增加,管壁温度的增长速度跟频率约成正比;爆震室上沿着压缩波叠加至形成爆震的方向,温度在外壁面上递增分布,在爆震形成区温度最高,从爆震形成区到发动机出口处,温度在外壁面上逐渐降低;各频率下最高温度区位置基本不变,距点火位置1 350mm左右;同一轴向位置上的外壁面温度随频率的增加而增加,温度的增长幅度随频率的增加而减小。     

Large-scale Bright Fronts in the Solar Corona: A?Review of?��EIT waves��

??EIT waves?? are large-scale coronal bright fronts (CBFs) that were first observed in 195 Å images obtained using the Extreme-ultraviolet Imaging Telescope (EIT) onboard the Solar and Heliospheric Observatory (SOHO). Commonly called ??EIT waves??, CBFs typically appear as diffuse fronts that propagate pseudo-radially across the solar disk at velocities of 100?C700 km?s^?1 with front widths of 50?C100 Mm. As their speed is greater than the quiet coronal sound speed (c _s ??200 km?s^?1) and comparable to the local Alfvén speed (v _A ??1000 km?s^?1), they were initially interpreted as fast-mode magnetoacoustic waves ( $v_{f}=(c_{s}^{2} + v_{A}^{2})^{1/2}$ ). Their propagation is now known to be modified by regions where the magnetosonic sound speed varies, such as active regions and coronal holes, but there is also evidence for stationary CBFs at coronal hole boundaries. The latter has led to the suggestion that they may be a manifestation of a processes such as Joule heating or magnetic reconnection, rather than a wave-related phenomena. While the general morphological and kinematic properties of CBFs and their association with coronal mass ejections have now been well described, there are many questions regarding their excitation and propagation. In particular, the theoretical interpretation of these enigmatic events as magnetohydrodynamic waves or due to changes in magnetic topology remains the topic of much debate.