舰载机前起落架突伸的动力学分析

研究了舰载机前起落架的突伸运动，针对这个问题，文中建立了一个两自由度的质量－弹簧－阻尼器的力学模型。推导出突伸运动方程以及两种不同形式的双气室缓冲器的非线性气体弹簧力和油液阻尼力的计算公式，并通过对已有试验结果的验算说明了本模型的可行性，利用该模型，用数值方法分析，校核了某舰载机的初步设计方案，计算得到了前起落架突伸运动的位置，速度曲线，并给出突伸期间飞机在甲板上的滑行距离和攻角的增量。文中还讨论     

空天飞机的边界层转捩

本文概述了边界层转捩对空天飞机性能的影响。在介绍确定边界层转捩起始点的线性稳定性理论和简单关联公式之后，又从噪声影响、头部钝头影响和钝锥飞行试验结果等几方面，讨论了线性稳定性理论的应用。接着介绍了采用转捩函数来确定转捩区的方法。从飞行试验、理论计算和风洞试验等三方面，探讨了进一步研究高超声速边界层转捩的途径。重点介绍了ＮＡＳＡＬａｎｇｌｅｙ研究中心的超声速、高超声速静风洞技术的发展。最后，对今后空天飞机边界层转捩的研究工作提出了建议。     

双圆柱斜向排列时旋涡脱落频率的实验研究

本研究用热线风速仪测量了斜向排列双圆柱的尾迹,并分析了尾迹中某些特征点上的速度频谱,从旋涡脱落频率的规律来研究双圆柱绕流相互之间的干扰。当两圆柱间距较远时,速度振荡的频率与单圆柱卡门涡街的频率相接近,随着两圆柱间距的接近,前、后圆柱各有其不同的旋涡脱落频率,且都不同于单圆柱旋涡脱落的频率。特别是当两圆柱处于某一相对位置时,出现双峰值的功率谱,其中一个峰值的频率大大地高于另一个峰值对应的频率,而且这两个峰值谁主谁副是不确定的,呈现出不稳定流动的特性。     

一种改进的数字式波束形成的快速自适应算法

提出了一种改进的数字式波束形成的快速自适应算法,即具有严格约束最小功率的抽样矩阵梯度算法(CSMG)。它综合了传统抽样矩阵梯度、算法和具有严格约束的最小功率自适应算法的优点。计算机模拟表明,此算法波束方向随约束角度而变,自适应调零能力较强,收敛速度也较快。     

GPS定时校频应用技术的基础研究

针对利用GPS进行定时校频技术开展了一系列的应用基础研究,包括GPS定时校频的方法及其不确定度、定时校频数据的处理等。在给出实验结果的同时,对影响GPS定时精度的各种因素(包括SA影响)进行了讨论;同时对提高GPS定时精度的途径作了初步探讨。     

Energetic ion emission for active spacecraft control

Future space missions aiming at the accurate measurement of cold plasmas and DC to very low frequency electric fields will require that the potential of their conductive surfaces be actively controlled to be near the ambient plasma potential. In the near-Earth space these spacecraft are usually solar-cell powered; consequently, parts of their surface are most of the time exposed to solar photons. Outside the plasmasphere, a positive surface potential due the dominance of surface-emitted photoelectrons over ambient plasma electrons is to be expected. Photo- and ambient electrons largely determine the potential and positive values between a few Volts up to 100 V have been observed. Active ion emission is the obvious solution of this problem. A liquid metal ion emitter and a saddle field ion emitter are nearing the stage of flight unit fabrication. We will attempt to clamp the spacecraft potential to values close to the plasma potential. We present first results from vacuum chamber tests and describe the emission behaviour and characteristics of emitters producing, respectively, In⁺ and N₂⁺ beams with an energy of ≥ 5 keV.     

The detection of energetic cometary and solar particles by the EPONA instrument on the Giotto mission

EPONA is an energetic particle detector system incorporating totally depleted silicon surface barrier layer detectors. Active and passive background shielding will be employed and, by applying various techniques, particles of different species, including electrons, protons, alpha particles and pick-up ions of cometary origin may be detected over a wide spectrum of energies extending from the tens of KeV into the MeV range.

The instrument can operate in two modes namely (a) in a cruise phase or storage mode and (b) in a real time mode. During the real time mode, observations at high spatial (octosectoring) and temporal (0.5s) resolution in the cometary environment permit studies to be made of accelerated particles at the bow shock and/or in the tail of the comet. In conjunction with magnetic field measurements on board Giotto, observations of energetic electrons and their anisotropies can determine whether the magnetic field lines in the cometary tail are open or closed. Further, the absorption of low energy solar particles in the cometary atmosphere can be measured and such data would provide an integral value of the pertaining gas and dust distribution. Solar particle background measurements during encounter may also be used to correct the measurements of other spacecraft borne instruments potentially vulnerable to such radiation.

Solar particle flux measurements, obtained during the cruise phase will, when combined with simultaneous observations made by other spacecraft at different heliographic longitudes, provide information concerning solar particle propagation in the corona and in interplanetary space.     

Charged-particle mutagenesis II. Mutagenic effects of high energy charged particles in normal human fibroblasts.

The biological effects of high LET charged particles are a subject of great concern with regard to the prediction of radiation risk in space. In this report, mutagenic effects of high LET charged particles are quantitatively measured using primary cultures of human skin fibroblasts, and the spectrum of induced mutations are analyzed. The LET of the charged particles ranged from 25 KeV/micrometer to 975 KeV/micrometer with particle energy (on the cells) between 94-603 MeV/u. The X-chromosome linked hypoxanthine guanine phosphoribosyl transferase (hprt) locus was used as the target gene. Exposure to these high LET charged particles resulted in exponential survival curves; whereas, mutation induction was fitted by a linear model. The Relative Biological Effect (RBE) for cell-killing ranged from 3.73 to 1.25, while that for mutant induction ranged from 5.74 to 0.48. Maximum RBE values were obtained at the LET of 150 keV/micrometer. The inactivation cross-section (alpha i) and the action cross-section for mutant induction (alpha m) ranged from 2.2 to 92.0 micrometer2 and 0.09 to 5.56 x 10(-3) micrometer2, respectively. The maximum values were obtained by 56Fe with an LET of 200 keV/micrometer. The mutagenicity (alpha m/alpha i) ranged from 2.05 to 7.99 x 10(-5) with the maximum value at 150 keV/micrometer. Furthermore, molecular analysis of mutants induced by charged particles indicates that higher LET beams are more likely to cause larger deletions in the hprt locus.     

The characteristics of sharp (small-scale) boundaries of solar wind plasma and magnetic field structures

We investigate properties of large (>20%) and sharp (<10 min) solar wind ion flux changes using INTERBALL-1 and WIND plasma and magnetic field measurements from 1996 to 1999. These ion flux changes are the boundaries of small-scale and middle-scale solar wind structures. We describe the behavior of the solar wind velocity, temperature and interplanetary magnetic field (IMF) during these sudden flux changes. Many of the largest ion flux changes occur during periods when the solar wind velocity is nearly constant, so these are mainly plasma density changes. The IMF magnitude and direction changes at these events can be either large or small. For about 55% of the ion flux changes, the sum of the thermal and magnetic pressure are in balance across the boundary. In many of the other cases, the thermal pressure change is significantly more than the magnetic pressure change. We also attempted to classify the types of discontinuities observed.     

非平稳信号的双重中值容错平滑算法

平滑是消除或削弱测量数据随机误差时常用的数据处理手段。文章建立了一组新的非平稳数据序列容错平滑算法，其采用两阶段两次滑动中值与滑动均值平滑组合，实现了数据简化与平滑的统一。理论分析和仿真计算结果证实，算法可有效避免斑点型异常数据的不利影响，有效削弱随机误差的影响，改进数据处理精度和数据处理结果可靠性。