GRIB数据及其在航迹预测中的应用

四维航迹预测的准确性是轨迹运行与空管决策支持的基础,而高空风数据支持下的气象建模是提高航迹预测准确性的关键。通过解析GRIB格式的风数据,获取各高度层的风速和风向,同时依据风对地速、航向的影响进行四维航迹预测建模,利用浦东机场的进场航班实现仿真验证,将预测结果与实际雷达轨迹对比,验证了风影响下四维航迹预测的准确性。     

苏通大桥实测强风湍流积分尺度的对比研究

湍流积分尺度是体现风特性的重要指标之一,而现场实测是获得工程结构准确可靠的风特性的唯一有效手段.本文利用苏通大桥结构健康监测系统(SHMS)采集的风特性数据库,选取该桥址区2008年夏季的“凤凰”、“海鸥”台风及冬季北风为样本进行强风特性分析.其中采用4种常用计算方法重点研究了桥址区强风的积分尺度,并对比了不同方法的计算结果以验证其可靠性.最后分析了湍流积分尺度随高度和平均风速等的变化规律.结果表明:湍流积分尺度与风速之间无确定关系,塔顶湍流积分尺度较跨中大.分析结果充实了苏通大桥风特性数据库,可为湍流积分尺度的分析计算提供参考,并为苏通大桥的强风环境和抗风评估提供了实测依据.     

基于FFT含有饱和环节的非线性等效系统的方法研究

基于快速傅里叶变换(FFT)方法,对系统的输入和输出信号进行快速傅里叶变换,对含有高次谐波的输出信号进行滤波,得到期望主频率的傅里叶频谱,然后进行傅里叶反变换,求得在各主频率下的幅值和相位.利用MATLAB中的非线性最小二乘拟配方法得到含有非线性环节的飞机纵向飞行控制系统的频域等效线性模型.这种方法也为含有非线性环节的飞机纵向飞行控制系统的飞行品质评估提供了一种可行的方法.     

Spatial heterogeneity in the radiogenic activity of the lunar interior: Inferences from CHACE and LLRI on Chandrayaan-1

In the past, clues on the potential radiogenic activity of the lunar interior have been obtained from the isotopic composition of noble gases like Argon. Excess Argon (40) relative to Argon (36), as compared to the solar wind composition, is generally ascribed to the radiogenic activity of the lunar interior. Almost all the previous estimates were based on, ‘on-the-spot’ measurements from the landing sites. Relative concentration of the isotopes of ⁴⁰Ar and ³⁶Ar along a meridian by the Chandra’s Altitudinal Composition Explorer (CHACE) experiment, on the Moon Impact Probe (MIP) of India’s first mission to Moon, has independently yielded clues on the possible spatial heterogeneity in the radiogenic activity of the lunar interior in addition to providing indicative ‘antiquity’ of the lunar surface along the ground track over the near side of the moon. These results are shown to broadly corroborate the independent topography measurements by the Lunar Laser Ranging Instrument (LLRI) in the main orbiter Chandrayaan-1. The unique combination of these experiments provided high spatial resolution data while indicating the possible close linkages between the lunar interior and the lunar ambience.     

Improved interpretation of solar wind ion measurements via high-resolution magnetic field data

The Wind   spacecraft’s Faraday cups (FC) continue to produce high-quality, in situ observations of thermal protons (i.e., ionized hydrogen) and α$\alpha$-particles (i.e., fully ionized helium) in the solar wind. By fitting a Wind/FC ion spectrum with a model velocity distribution function (VDF) for each particle species, values for density, bulk velocity, and temperature can be inferred. Incorporating measurements of the background magnetic field from the Wind Magnetic Field Investigation (MFI) allows perpendicular and parallel temperature components to be separated. Prior implementations of this analysis averaged the higher-cadence Wind/MFI measurements to match that of the Wind/FC ion spectra. However, this article summarizes recent and extensive revisions to the analysis software that, among other things, eliminate such averaging and thereby account for variations in the direction of the magnetic field over the time taken to measure the ions. A statistical comparison reveals that the old version consistently underestimates the temperature anisotropy of ion VDF’s: averaging over fluctuations in the magnetic field essentially blurs the perpendicular and parallel temperature components, which makes the plasma seem artificially more isotropic. The new version not only provides a more accurate dataset of ion parameters (which is well suited to the study of microkinetic phenomena), it also demonstrates a novel technique for jointly processing particle and field data. Such methods are crucial to heliophysics as wave-particle interactions are increasingly seen as playing an important role in the dynamics of the solar wind and similar space plasmas.     

跨超声速风洞大开角段设计技术研究

跨超声速风洞大开角段设计技术研究对于提高大开角段的安全性能与改进稳定段入口气流质量有着重大意义.由于影响大开角段性能的参数较多,完全通过试验方法进行设计的成本过高.本文通过数值模拟方法,结合适当的边界条件,对不同参数的大开角段进行了模拟,从数值模拟的结果可以看到,孔板开孔率和扩开角对大开角段性能有显著影响,通过比较得出了较为合理的参数匹配.这表明本文所用的方法用于大开角段气动设计是可行的,这为数值模拟方法应用于风洞部段气动设计创造了一定的条件.     

双三角机翼前缘涡襟翼的试验研究

通过风洞试验对双三角翼的内涡襟翼及外涡襟翼进行了研究。探讨了影响涡襟翼效率的各种因素及其规律,其中包括机翼前缘区状态、涡襟翼形状、涡襟翼偏度、内、外涡襟翼的搭配以及后缘襟翼效率等。尤其是根据内外翼涡场的不同研究了复合平面形状机翼内涡襟翼与外涡襟翼设计上的特点,为设计双三角翼的涡襟翼提供了参考数据。研究结果表明,正确设计前缘涡襟翼与后缘襟翼可以优化大后掠双三角机翼的低速性能。     

出口封闭的冲压发动机进气道激波振荡现象

采用计算流体力学和风洞试验两种手段,对冲压发动机出口封闭的多种超声速进气道内通道气流振荡现象进行了研究。结果表明,在一定的超声速范围内,封闭的进气道内通道发生了较强气流振荡现象,振荡频率、幅值和内通道长度、飞行马赫数有关,该振荡现象是一种自激振荡现象。利用亥姆霍兹共振器频率公式可以对封闭的进气道内通道振荡频率进行预估,并对其归纳出一种修正方法,可以结合模型试验结果对进气道和燃烧室内流振荡频率和幅值进行分析,为飞行试验提供预估和参考。     

可移动式风蚀风洞的设计与研究

可移动式风蚀风洞是对土壤进行抗风蚀能力测试研究的一种有力工具。所设计的风蚀风洞全长15.9 m,其中实验段长7.7 m,平均分为7段,入口截面长宽均为0.9 m;收缩段长1.2 m,收缩比为2;风洞内风速在0～20 m/s范围内连续可调,转角段的创新设计能够是风洞有均匀的流场。风洞的各个部分易于连接和拆分,以便于野外科学研究时移动和运输的功能。经过运行测试和风速廓线实验,空风洞下风洞的各项气动性能指标已经达到设计标准,该风洞已经投入到科研实验中。     

可变体机翼多物理场分布式光纤集成测试技术

介绍了可变体机翼技术和可变体机翼多物理场光纤集成测试技术的研究现状.