航空发动机滑油系统稳态压力模型研究

以某型发动机滑油系统为研究对象,深入分析了系统的工作原理和部件结构特点。综合应用流体力学,工程热力学理论以及数值计算和实验的方法,建立了滑油系统主要部件的数学模型和管路压力损失的计算模型;在此基础上,依据发动机滑油系统良好状态下采集的数据,建立了滑油系统的稳态压力数学模型,为判断滑油系统性能衰退和故障提供参考依据。      

The Time-of-Flight Energy,Angle, Mass Spectrograph (Teams) Experiment for Fast

The Time-of-flight Energy Angle Mass Spectrograph (TEAMS) is being flown on the FAST Small Explorer mission to measure the 3-dimensional distribution function of the major ion species present in the lower magnetosphere. The instrument is similar to time-of-flight plasma analyzer systems that have been designed and planned for flight as CODIF (COmposition and DIstribution Function analyzer) on the four European Space Agency Cluster-II spacecraft and, as ESIC (Equator-S Ion Composition instrument) on Equator-S. This instrument allows the 3-dimensional distribution functions of individual ion species to be determined within spin period (2.5 s). Two-dimensional distributions are measured in 80 ms. These capabilities are crucial for the study of selective energization processes in the auroral regions of the magnetosphere. The design, operational characteristics, and test and calibration results for this instrument are presented. The sensor consists of a toroidal top-hat electrostatic analyzer with instantaneous acceptance of ions over 360° in polar angle. After post-acceleration of the incoming ions by up to 25 kV, a time-of-flight mass spectrograph discriminates the individual species. It has been demonstrated through calibration that the instrument can easily separate H⁺, He²⁺, He⁺, O⁺ and, for energies after post-acceleration of > 20 keV, even O₂ ⁺ molecules. On-board mass discrimination and the internal accumulation of several distinct data quantities combined with the spacecraft's flexible telemetry formatting allow for instrument data rates from 7.8 kb s^–1 to 315 kb s^–1 to be telemetered to ground through the FAST centralized Instrument Data Processor.     

Decay of Magnetic Field Irregularities Observed by Ulysses

We study the solar cycle, radial, and latitudinal dependence of the characteristics of magnetic field irregularities in the Heliosphere. The frequency of magnetic field discontinuities is determined, using high time resolution magnetic field observations by Ulysses, covering the time interval from 1992 to 2000. The quasi-linear scattering mean free path of particles is also calculated. These investigations aim at understanding/exploring transport properties of energetic charged particles in the Heliosphere. We find that the travel time of solar wind plasma from the Sun to the observer is the key parameter of the process, by controling the decay of the irregularities. This revised version was published online in August 2006 with corrections to the Cover Date.     

Ion Acoustic Waves in the Heliosphere

Observations of ion acoustic waves in the solar wind during the first and second orbit of the Ulysses spacecraft are presented. The observations show variations of the wave activity with the heliolatitude and with the phase of the solar cycle. The interrelationships between the wave intensity and the electron heat flux and the ratio of electron to proton temperature, T _e/T _p, are examined. This revised version was published online in August 2006 with corrections to the Cover Date.     

The FAST Satellite Fields Instrument

We describe the electric field sensors and electric and magnetic field signal processing on the FAST (Fast Auroral SnapshoT) satellite. The FAST satellite was designed to make high time resolution observations of particles and electromagnetic fields in the auroral zone to study small-scale plasma interactions in the auroral acceleration region. The DC and AC electric fields are measured with three-axis dipole antennas with 56 m, 8 m, and 5 m baselines. A three-axis flux-gate magnetometer measures the DC magnetic field and a three-axis search coil measures the AC magnetic field. A central signal processing system receives all signals from the electric and magnetic field sensors. Spectral coverage is from DC to 4 MHz. There are several types of processed data. Survey data are continuous over the auroral zone and have full-orbit coverage for fluxgate magnetometer data. Burst data include a few minutes of a selected region of the auroral zone at the highest time resolution. A subset of the burst data, high speed burst memory data, are waveform data at 2×10⁶ sample s^–1. Electric field and magnetic field data are primarily waveforms and power spectral density as a function of frequency and time. There are also various types of focused data processing, including cross-spectral analysis, fine-frequency plasma wave tracking, high-frequency polarity measurement, and wave-particle correlations.     

The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments

The source region of solar wind plasma is observed to be directly reflected in the compositional pattern of both elemental and charge state compositions. Slow solar wind associated with streamers shows higher freeze-in temperatures and larger FIP enhancements than coronal hole associated wind. Also, the variability of virtually all compositional parameters is much higher for slow solar wind compared to coronal hole associated wind. We show that these compositional patterns persist even though stream-stream interactions complicate the identification based on in situ plasma parameters. This revised version was published online in August 2006 with corrections to the Cover Date.     

气固紊流剪切流中颗粒弥散的拉格朗日模拟

本文提出了一种对于气固两相紊流剪切流中圆形固体颗粒弥散的拉格朗日拟计算方法，其中考虑了颗粒间的磁撞对流体相和颗料相的影响，应用该方法对一气固紊流剪切流场进行了模拟计算，并对有、无颗粒间磁撞情况下的模拟计算结果与Lavieville用大涡模拟方法的研究结果进行了比较，并进行了讨论。     

幂指函数在非线性规划中的应用

给出一种自适应近似函数－幂指函数f^-(x)在非线性规划中的收敛算法。它采用minx∈Enf^-(x)的最优解序列｛x^-｝去逼近原问题minx∈Enf^-(x)的最优解x^*.与传统优化算法相比：该算法最优解｛x^-｝可以通过f^-x(x)=0直接解析得出；该算法不要求序列｛f(x)^k｝具有单调减特性，却能够保证算法的收敛性，该算法的计算量对变量的维数不敏感，从而具有广泛的应用前景，从方法论上，它是采用“特殊非线性”来研究“一般非线性”的一种新方法。     

固体废弃物热解产物的神经网络预测模型

本文采用3层BP神经网络建立了固体废弃物热解产物的产率和特性的预测模型。采用遗传BP算法来优化隐层节点数和学习速率η0与回归方法相比，其预测误差明显小于回归公式的预测误差。     

某型发动机加力燃油总管喷油杆断裂分析

研究了某些发动机在使用中发生的两起加力燃油总管喷油杆断裂故障，通过断口分析，组织检查，喷油杆受力分析等工作，找出喷油杆疲劳断裂失效的根本原因是设计不佳，导致喷油杆根部承受的应力水平较高，另外焊接缺陷是对疲劳裂纹的萌生起到了促进作用，最后提出了预防与改进的措施。