基于执行时段滑动调整策略的中继卫星任务规划算法设计

针对中继卫星任务规划问题开展研究,提出一种基于执行时段滑动调整策略的任务规划算法。首先分析了中继卫星资源调度过程,并对任务申请的时间特征进行形式化描述,然后归纳出任务分配的主要约束,从而完成问题建模。在此基础上,对优化算法进行设计,给出了执行时段滑动调整步骤。通过调整已规划任务执行时段的方法,使部分原本无法执行任务具备执行可能,提升了任务执行率和资源利用率。在仿真实验中,通过大规模测试分析对比不同算法的优化效果,验证了文中所提方法的有效性。     

涡轴发动机分布式控制系统传感器故障诊断技术

为满足航空发动机分布式控制系统的故障诊断需求,重点解决分布式控制系统中总线通信时延对传统故障诊断措施效果的影响,提出了一种新的航空发动机分布式控制系统故障诊断方法.针对航空涡轴发动机,搭建了包含随机时延的分布式控制系统数学模型,利用等价空间法(PSM)设计故障诊断滤波器组.并将改进的故障诊断方法与传统的基于Kalman...     

XN－1040轻型汽车后桥壳体三维有限元应力计算

对ＸＮ－１０４０轻型汽车后桥壳体进行三维有限元应力计算，并分析计算结果，得到该型后桥壳体的应力大小，位移大小，应力分布状况，并通过Ａｎｔｏ－ＣＡＤ１１．０构造变形前后的三维线框模型．从而直观的分析后桥壳体的变形．     

Fine scale temporal structures in solar hard X-ray bursts observed by PHEBUS

We report here on preliminary results of a systematic study of fast temporal fluctuations in impulsive and extended solar X-ray bursts observed by PHEBUS at energies around 100 keV. Subsecond timescales are quite common in the impulsive events and are not observed in extended ones.     

数据采集系统通道采集速率评价中的几个问题

介绍了一种简单实用的数据采集系统采集速率的方法，讨论了评价过程的误差来源，以及减小其评价误差的几种对策；同时，给出了评价过程的计算机仿真结果。     

全测速测元弹道计算的数据融合算法与应用

针对“全测速”测元条件下弹道计算的数据融合问题,就数据融合中初值的确定、最优节点的搜索、样条基函数的选取、数据融合模型的数值解法等方面进行了分析与讨论,并给出一种适用于“全测速”测元条件下弹道计算的数据融合算法,经试用表明：该算法不仅具有良好的收敛性、稳定性,而且有着很好的数据融合效果,弹道计算的精度与“测距-测速”混合条件下数据融合弹道的精度相当。     

风洞试验数据管理平台设计与研究

针对国内民用飞机风洞试验数据体量大、种类多、高时效、更新快等特点,引入了矩阵存储模式替代了原有的分层存储模式对现有风洞试验数据进行了重新划分与归类,优化了数据文件存储结构。仔细分析该平台在存储规模、管理规范及使用功能等方面的需求后,拟选择IBMx366型或同等级别的工作站及配套设备作为硬件基础,同时明确了该平台的面向对象、使用规范及管理办法。该平台所含写入/查询/更新等常规功能采用Labview8.6软件开发平台及SQL语句脚本实现。该数据管理平台已具备了一定实际功能,基本满足对风洞试验数据管理的需求。     

The Composition of the Solar Wind in Polar Coronal Holes

The solar wind charge state and elemental compositions have been measured with the Solar Wind Ion Composition Spectrometers (SWICS) on Ulysses and ACE for a combined period of about 25 years. This most extensive data set includes all varieties of solar wind flows and extends over more than one solar cycle. With SWICS the abundances of all charge states of He, C, N, O, Ne, Mg, Si, S, Ar and Fe can be reliably determined (when averaged over sufficiently long time periods) under any solar wind flow conditions. Here we report on results of our detailed analysis of the elemental composition and ionization states of the most unbiased solar wind from the polar coronal holes during solar minimum in 1994–1996, which includes new values for the abundance S, Ca and Ar and a more accurate determination of the ²⁰Ne abundance. We find that in the solar minimum polar coronal hole solar wind the average freezing-in temperature is ∼1.1×10⁶ K, increasing slightly with the mass of the ion. Using an extrapolation method we derive photospheric abundances from solar wind composition measurements. We suggest that our solar-wind-derived values should be used for the photospheric ratios of Ne/Fe=1.26±0.28 and Ar/Fe=0.030±0.007.     

Johannes Geiss’ Investigations of Solar, Heliospheric and Interstellar Matter

Johannes Geiss is a world leader and foremost expert on measurements and interpretation of the composition of matter that reveals the history, present state, and future of astronomical objects. With his Swiss team he was first to measure the composition of the noble gases in the solar wind when in the late 1960s he flew the brilliant solar wind collecting foil experiments on the five Apollo missions to the moon. Always at the forefront of the art of composition measurements, he with his colleagues determined the isotopic and elemental composition of the solar wind using instruments characterized by innovative design that have provided the most comprehensive record of the solar wind composition under all solar wind conditions at all helio-latitudes. He discovered heavy interstellar pickup ions, from which the composition of the neutral gas of the Local Interstellar Cloud is determined, and the “Inner Source” of pickup ions. Johannes Geiss played a key role both in the in-situ measurements and modeling of molecular ions in comets, and the interpretation of these data. He and co-workers measured the composition of plasmas in the magnetospheres of Earth and Jupiter. Here we highlight Johannes Geiss’ many discoveries and seminal contributions to our knowledge of the composition of matter of the Sun, solar wind, interstellar gas, early universe, comets and magnetospheres.     

An Update on Ultra-Heavy Elements in Solar Energetic Particles above 10 MeV/Nucleon

Measurements below several MeV/nucleon from Wind/LEMT and ACE/ULEIS show that elements heavier than Zn (Z=30) can be enhanced by factors of ∼100 to 1000, depending on species, in ³He-rich solar energetic particle (SEP) events. Using the Solar Isotope Spectrometer (SIS) on ACE we find that even large SEP (LSEP) shock-accelerated events at energies from ∼10 to >100 MeV/nucleon are often very iron rich and might contain admixtures of flare seed material. Studies of ultra-heavy (UH) SEPs (with Z>30) above 10 MeV/nucleon can be used to test models of acceleration and abundance enhancements in both LSEP and ³He-rich events. We find that the long-term average composition for elements from Z=30 to 40 is similar to standard solar system values, but there is considerable event-to-event variability. Although most of the UH fluence arrives during LSEP events, UH abundances are relatively more enhanced in ³He-rich events, with the (34<Z<40)/O ratio on average more than 50 times higher in ³He-rich events than in LSEP events. At energies >10 MeV/nucleon, the most extreme event in terms of UH composition detected so far took place on 23 July 2004 and had a (34<Z<40)/O enhancement of ∼250–300 times the standard solar value.