三维钝体结构风压分布与绕流特性的大涡模拟研究

针对风场作用下三维钝体结构的绕流特性与空间风压分布特性,采用大涡模型对其进行了数值模拟研究,以平均风速和脉动风速作为入口边界条件,在稳态分析的基础上对9种不同来流方向的工况进行了瞬态动力分析,再现了钝体绕流的冲撞、分离、重附着等现象,揭示了钝体绕流主、次涡循环区的形成、发展机理,提出了空间风压场分布的一般规律。研究表明:钝体绕流对流场风速剖面影响的强弱程度依次为尾流区、屋顶区、来流区,且对中心区域流场风速剖面的影响要大于两侧流场,并由中心区域向两侧逐渐减小;来流区钝体绕流特性与空间风压分布特性较屋顶区和尾流区稳定,尾流区涡旋的非对称生成、脱落对钝体左右两侧流场的冲撞、分离、重附着等具有重要的影响;来流方向与钝体呈45°或135°夹角时,对尾流风场的影响范围最小,但随着来流方向逐渐垂直于钝体,尾流影响区域也逐渐增大。     

小型二冲程航空发动机燃烧循环变动研究

利用峰值压力、最大压力上升率、燃烧百分率以及它们各自所对应的曲轴转角和相空间重构投影法评价小型二冲程航空发动机的燃烧循环变动.通过比较,认为燃烧百分率所对应的曲轴转角能更好地表征发动机的燃烧循环变动.针对发动机在中速和不同负荷条件下的燃烧循环变动分析,结果表明随负荷的加大,缸内燃烧的循环变动会变小,认为是负荷加大,气体...     

Large geomagnetic storms of extreme solar event periods in solar cycle 23

During extreme solar events such as big flares or/and energetic coronal mass ejections (CMEs) high energy particles are accelerated by the shocks formed in front of fast interplanetary coronal mass ejections (ICMEs). The ICMEs (and their sheaths) also give rise to large geomagnetic storms which have significant effects on the Earth’s environment and human life. Around 14 solar cosmic ray ground level enhancement (GLE) events in solar cycle 23 we examined the cosmic ray variation, solar wind speed, ions density, interplanetary magnetic field, and geomagnetic disturbance storm time index (D_st). We found that all but one of GLEs are always followed by a geomagnetic storm with D_st  −50 nT within 1–5 days later. Most(10/14) geomagnetic storms have D_st index  −100  nT therefore generally belong to strong geomagnetic storms. This suggests that GLE event prediction of geomagnetic storms is 93% for moderate storms and 71% for large storms when geomagnetic storms preceded by GLEs. All D_st depressions are associated with cosmic ray decreases which occur nearly simultaneously with geomagnetic storms. We also investigated the interplanetary plasma features. Most geomagnetic storm correspond significant periods of southward B_z and in close to 80% of the cases that the B_z was first northward then turning southward after storm sudden commencement (SSC). Plasma flow speed, ion number density and interplanetary plasma temperature near 1 AU also have a peak at interplanetary shock arrival. Solar cause and energetic particle signatures of large geomagnetic storms and a possible prediction scheme are discussed.     

Solar Energetic Particle Composition, Energy Spectra, and Space Weather

Recent progress in measuring the composition and energy spectra of solar energetic particles (SEPs) accelerated by CME-driven shocks is reviewed, including a comparison of the observed charge-to-mass dependence of breaks in SEP spectra with model predictions. Also discussed is a comparison of SEP and CME kinetic energies in seventeen large SEP events, and estimates of the SEP radiation dose that astronauts would be subject to once they venture outside the protective cover of Earth’s magnetosphere.     

On the Differences in Composition between Solar Energetic Particles and Solar Wind

Although the average composition of solar energetic particles (SEPs) and the bulk solar wind are similar in a number of ways, there are key differences which imply that solar wind is not the principal seed population for SEPs accelerated by coronal mass ejection (CME) driven shocks. This paper reviews these composition differences and considers the composition of other possible seed populations, including coronal material, impulsive flare material, and interplanetary CME material.     

旋翼塔大型分布式测控系统的顶层设计

本文介绍了旋翼塔大型分布式测控系统的基本原理、结构框图、功能模块的划分以及研制要求等。并对试验软硬件开发流程、顶层设计的目的和内容进行了探讨。     

High-precision RCS measurement of aircraft’s weak scattering source

The radar cross section(RCS) of weak scattering source on the surface of an aircraft is usually less than 40 d Bsm.How to accurately measure the RCS characteristics of weak scattering source is a technical challenge for the aircraft's RCS measurement.This paper proposes separating and extracting the two-dimensional(2D) reflectivity distribution of the weak scattering source with the microwave imaging algorithm and spectral transform so as to enhance its measurement precision.Firstly,we performed the 2D microwave imaging of the target and then used the 2D gating function to separate and extract the reflectivity distribution of the weak scattering source.Secondly,we carried out the spectral transform of the reflectivity distribution and eventually obtained the RCS of the weak scattering source through calibration.The prototype experimental results and their analysis show that the measurement method is effective.The experiments on an aircraft's low-scattering conformal antenna verify that the measurement method can eliminate the clutter on the surface of aircraft.The precision of measuring a 40 d Bsm target is 3–5 d B better than the existing RCS measurement methods.The measurement method can more accurately obtain the weak scattering source's RCS characteristics.     

不同损伤尺寸铝合金结构疲劳寿命分散性研究

飞机损伤结构疲劳寿命分散系数是分析损伤结构疲劳寿命分散程度的重要参数。针对飞机常用铝合金材料，开展预置损伤试验件疲劳测试。采用相关系数比较法，判断损伤结构剩余疲劳寿命分布类型；通过断口观察和数据统计处理，分析损伤与疲劳寿命关系及含损伤结构剩余疲劳寿命分散性规律。结果表明：含损伤结构剩余疲劳寿命更加符合威布尔分布；含预置损伤结构较未预置损伤结构疲劳寿命下降明显，随预置损伤尺寸增加，结构剩余疲劳寿命逐步降低，剩余疲劳寿命分散性增大，不同初始损伤结构疲劳寿命分散性差异较大。本文研究为建立飞机不同损伤尺寸铝合金结构疲劳寿命分散系数模型提供参考依据。     

反高斯分布环境因子估计

研究了反高斯分布环境因子估计。根据指数分布和对数正态分布环境因子的定义及数据折算与综合的方便,给出了反高斯分布环境因子的定义。据此定义,用经典方法和贝叶斯方法推证了环境因子的上、下限,并给出了一些近似式以便于计算。实例计算结果较令人满意。     

一种热电势的简易表达法

当具有不同温度分布的多种导体连接在一个环路中时,按照帕尔贴电势和汤姆逊电势分析环路中的总的热电势是困难的。选择一些导体作为标准电极,就能把总的热电势分成一系列单一导体的独立热电势,用这个方法,分析工作将变得十分简单。