起落架油气式缓冲器设计中压缩比的选取

从理论上探讨缓冲器压缩比的选择范围。提出当缓冲器压缩比(静态对全伸展之比q_(so)、全压缩对静态之比q_(ms))的取值范围为2.5～4.5时,既可以较大限度地减少缓冲器体积,又可以把起落架的动载荷限制在较低的范围内,并为以往经验地选取压缩比提供理论基础。     

Global dynamics of high area-to-mass ratios GEO space debris by means of the MEGNO indicator

In this paper we provide an extensive analysis of the global dynamics of high-area-to-mass ratios geosynchronous (GEO) space debris, applying a recent technique developed by Cincotta and Simó [Cincotta, P.M., Simó, C.Simple tools to study global dynamics in non-axisymmetric galactic potentials–I. Astron. Astrophys. (147), 205–228, 2000.], Mean Exponential Growth factor of Nearby Orbits (MEGNO), which provides an efficient tool to investigate both regular and chaotic components of the phase space.     

基于知识辅助的海面目标航迹起始方法

针对海环境下不同雷达观测测量准确度存在差异而导致观测数据质量存在差异的问题,提出了一种基于知识辅助的海面目标航迹起始方法。该方法首先利用先验知识幅度信息计算幅度似然比,并以幅度似然比的大小来表示观测数据质量的高低;然后,利用幅度似然比辅助Hough空间参数积累,并对航迹初选参数进行初值修正,提高Mean Shift多尺度聚类滤波初值的准确性,减少迭代次数,再通过最优筛选的方法分析得到目标的真实航迹起始数目和航迹起始参数;最后,通过仿真数据证明了本文所提方法的有效性和优越性。     

Isotopic Composition of the Solar Wind Inferred from In-Situ Spacecraft Measurements

The Sun is the largest reservoir of matter in the solar system, which formed 4.6 Gyr ago from the protosolar nebula. Data from space missions and theoretical models indicate that the solar wind carries a nearly unfractionated sample of heavy isotopes at energies of about 1 keV/amu from the Sun into interplanetary space. In anticipation of results from the Genesis mission’s solar-wind implanted samples, we revisit solar wind isotopic abundance data from the high-resolution CELIAS/MTOF spectrometer on board SOHO. In particular, we evaluate the isotopic abundance ratios ¹⁵N/¹⁴N, ¹⁷O/¹⁶O, and ¹⁸O/¹⁶O in the solar wind, which are reference values for isotopic fractionation processes during the formation of terrestrial planets as well as for the Galactic chemical evolution. We also give isotopic abundance ratios for He, Ne, Ar, Mg, Si, Ca, and Fe measured in situ in the solar wind.     

异构多星编队的脉冲构型保持控制方法

近地轨道的双星编队通常设计具有自稳定性的编队构型参数初值,通过保持编队构型参数形成长期稳定的相对周期运动。针对编队中卫星数量增多产生的相对运动耦合问题,提出了基于Hill坐标和三角函数公式的多星相对运动分析方法。基于SAR载荷测量基线定义,结合多星编队构型参数的相对运动特性,提出了编队构型参数的设计方法,能够实现多星编队的最大有效基线组合。通过分析J2项摄动和大气阻力摄动的长期影响,研究了异构多星编队的相对运动衍化规律,提出了主从形式的脉冲偏置控制,能够有效保持针对异构多星编队设计的编队构型。通过面质比异构的四星编队控制仿真,验证了脉冲偏置控制形式下异构多星编队构型保持控制方法的有效性。     

基于江门地下中微子实验的地球中微子信号研究

地球中微子是帮助人类认识地球内部结构和成分的一种可行手段。由于目前液闪探测器的体积太小,无法区分地幔的模型。江门地下中微子实验(JUNO)的液闪达到了20 kt,具有很强的观测优势。本研究基于LITHO1.0地球模型预测出JUNO的地球中微子事例率是(34.50±4.78)TNU。同时,研究结果显示地壳的放射性元素丰度误差对全球地壳中微子信号的影响显著大于地壳密度、地壳厚度误差所带来的影响。     

Fractionation of SI, NE, and MG Isotopes in the Solar Wind as Measured by Soho/Celias/MTOF

Using the high-resolution mass spectrometer CELIAS/MTOF on board SOHO we have measured the solar wind isotope abundance ratios of Si, Ne, and Mg and their variations in different solar wind regimes with bulk velocities ranging from 330 km/s to 650 km/s. Data indicate a small systematic depletion of the heavier isotopes in the slow solar wind on the order of (1.4±1.3)% per amu (2σ-error) compared to their abundances in the fast solar wind from coronal holes. These variations in the solar wind isotopic composition represent a pure mass-dependent effect because the different isotopes of an element pass the inner corona with the same charge state distribution. The influence of particle mass on the acceleration of minor solar wind ions is discussed in the context of theoretical models and recent optical observations with other SOHO instruments. This revised version was published online in June 2006 with corrections to the Cover Date.     

复合材料结构系统的可靠性分析方法

 <正> This paper presents a full quantity loading method for reliability analysis of composite structural systems in consideration of degradation of the structural Stiffness. According to the value of utilization ratios of members, critical members can be found out. The way of composing the critical members in groups is used to enumerate and identify significant failure modes. Some kinds of principles of deletion and mergence of failure modes are adopted. Some illustrative examples show that the method is vety efficient, especially for large scale composite structural system.     

Symplectic integration of space debris motion considering several Earth’s shadowing models

In this work, we present a symplectic integration scheme to numerically compute space debris motion. Such an integrator is particularly suitable to obtain reliable trajectories of objects lying on high orbits, especially geostationary ones. Indeed, it has already been demonstrated that such objects could stay there for hundreds of years. Our model takes into account the Earth’s gravitational potential, luni-solar and planetary gravitational perturbations and direct solar radiation pressure. Based on the analysis of the energy conservation and on a comparison with a high order non-symplectic integrator, we show that our algorithm allows us to use large time steps and keep accurate results. We also propose an innovative method to model Earth’s shadow crossings by means of a smooth shadow function. In the particular framework of symplectic integration, such a function needs to be included analytically in the equations of motion in order to prevent numerical drifts of the energy. For the sake of completeness, both cylindrical shadows and penumbra transitions models are considered. We show that both models are not equivalent and that big discrepancies actually appear between associated orbits, especially for high area-to-mass ratios.     

行星际尘粒中锂同位素丰度与太阳星云演化的关系

1引言构成太阳系的大多数元素都经历过恒星演化过程，但3种轻元素Li，Be和B极为脆弱，在绝大多数恒星内部的高温、高密度和剧烈变动的条件下，很快就会分解．太阳系的早期阶段，太阳星云可能是由大爆炸产生的1H、2H、3He、4He和7Li及附近超新星爆发产生的C、N、O等构成[1]，而6Li、Be、B是以后由宇宙射线粒子轰击附近星际和行星际的C、N、O等的核产生[2]．因为Li的同位素丰度的一部分是由大爆炸生成，一部分是由宇宙射线与星际介质核反应产生，因此它的丰度与宇宙射线暴露时间有关．1991年，文献间报导过在行星际尘粒中发现Li、Be和…