自由空间法测量电磁材料电磁参数

基于对自由空间法测试材料电磁参量原理的研究,对传统方法进行分析及改进,解决了测试过程

中透射系数存在的相位模糊性和由于S11 →0 时导致的半波谐振问题,最后搭建了测试系统,并使用该系统对

常见的微波介质材料在2 ~18 GHz 频带下进行了电磁参数的测试。结果表明,由于天线性能特性的限制,此测

试系统4 ~14 GHz 范围内具有良好的效果。此测试系统具有测试速度快、结构简单、方便准确的定位、测试精

度高等特点。

     

Shock protection of penetrator-based instrumentation via a sublimation approach

It is often necessary for space-borne instrumentation to cope with substantial levels of shock acceleration both in the initial launch phase, as well as during entry, descent and landing in the case of planetary exploration. Current plans for a new generation of penetrator-based space missions will subject the associated on-board instrumentation to far greater levels of shock, and ways must therefore be found to either ruggedize or else protect any sensitive components during the impact phase. In this paper, we present an innovative method of shock protection that is suited for use in a number of planetary environments, based upon the temporary encapsulation of said components within a waxy solid which may then be sublimated to return the instrument back to its normal operation. We have tested this method experimentally using micromachined silicon suspensions under applied shock loads of up to 15,000g, and found that these were able to survive without incurring damage. Furthermore, quality factor measurements undertaken on these suspensions indicate that their mechanical performance remains unaffected by the encapsulation and subsequent sublimation process.     

A statistical study of C IV regions in 20 Oe-stars

In this paper, using the Gauss-Rotation model (GR model), we analyse the UV C IV resonance lines in the spectra of 20 Oe-stars of different spectral subtypes, in order to detect the structure of C IV region. We study the presence and behavior of absorption clouds and analyse their characteristics. From this analysis we can calculate the values of a group of physical parameters, such as the apparent rotational and radial velocities, the random velocities of the thermal motions of the ions, the Full Width at Half Maximum (FWHM), the optical depth, as well as the absorbed energy and the column density of the independent regions of matter, which produce the main and the satellite clouds of the studied spectral lines. Finally, we present the relations between these physical parameters and the spectral subtypes of the studied stars and we give our results about the structure of the C IV region in their atmosphere.     

PVA浓度对电纺制备ZnO纳米纤维吸波性能的影响

采用静电纺丝法制备ZnO纳米纤维,研究聚乙烯醇(PVA)浓度对ZnO纳米纤维微观形貌、介电性能和吸波性能的影响规律。结果表明:随着PVA浓度从6%增至10%,ZnO纳米纤维直径变细,但珠结增加,粗细不均。当PVA浓度为8%时,ZnO纳米纤维直径较细、粗细均匀、表面光滑、珠结较少,形貌最好。此时,其介电常数达到最高值,实部为15.4~20.8,虚部为3.6~4.7,并在较薄的厚度下具有最优的吸波性能。当70%(质量分数/%,下同)ZnO纳米纤维/石蜡样品的厚度为1.3 mm时,反射率低于–5 dB的吸收带宽达到5.4 GHz(12.6~18 GHz),最小反射率为–16.6 dB。此外,石蜡含量也对样品的介电性能和吸波性能具有重要影响,随着石蜡含量的增加,样品的介电常数降低,当石蜡含量为30%和20%时,样品具有较好的吸波性能。     

某机第4级压气机转子叶片榫头折断故障分析

阐明了某机第4级压气机转子叶片在榫头部位断裂的故障特点。故障分析表明：经长期使用的叶片在修理厂大修时，为满足叶片摆动量要求在榫头底面涂尼龙胶，会使叶片自振频率有较大幅度下降；为排除3级叶片折断故障而提高的慢车转速又缩小了4级叶片的共振裕度，结果造成少数4级叶片落入慢车共振。共振发生时，不规则的尼龙胶和装配过程不规范引起的非正常接触容易导致微动磨损的加剧，从而大大降低了疲劳寿命，这是引起榫头断裂故障的主要原因。     

喷气动力装置的红外辐射源及其抑制

本文分析喷气动力装置的红外辐射源,并讨论抑制红外辐射的技术途径.喷气动力装置的红外辐射来源于燃烧引起的高温,并可区分为两大类:固体表面的辐射和热喷流的辐射.一般而言,抑制红外辐射可从以下三个方面着手:(1)用冷却或绝热的方法降低辐射表面的温度,或通过蔽挡阻止红外辐射的传播;(2)加速喷气流与周围空气的混合,使喷流温度快速降低;(3)降低燃烧产物中辐射成分的浓度.     

Alfvénic Electron Acceleration in Aurora Occurs in Global Alfvén Resonosphere Region

Auroral emission caused by electron precipitation (Hardy et al., 1987, J. Geophys. Res. 92, 12275–12294) is powered by magnetospheric driving processes. It is not yet fully understood how the energy transfer mechanisms are responsible for the electron precipitation. It has been proposed (Hasegawa, 1976, J. Geophys. Res. 81, 5083–5090) that Alfvén waves coming from the magnetosphere play some role in powering the aurora (Wygant et al., 2000, J. Geophys. Res. 105, 18675–18692, Keiling et al., 2003, Science 299, 383–386). Alfvén-wave-induced electron acceleration is shown to be confined in a rather narrow radial distance range of 4–5 R _E (Earth radii) and its importance, relative to other electron acceleration mechanisms, depends strongly on the magnetic disturbance level so that it represents 10% of all electron precipitation power during quiet conditions and increased to 40% during disturbed conditions. Our observations suggest that an electron Landau resonance mechanism operating in the “Alfvén resonosphere” is responsible for the energy transfer.     

直升机尾桨/尾梁耦合稳定性分析研究

单桨带尾桨直升机的尾旋翼设计成摆振柔软型后,带来了新的动力学问题:尾桨与尾梁耦合动不稳定性问题。本文简述了它与主旋翼/机体耦合动不稳定问题的差别,主要介绍了尾桨与尾梁耦合动不稳定性问题的分析方法,通过算例分析,为消除这种不稳定性,对一些关键设计参数提出了设计要求。     

一种惯性导航用减振器的低温工作特性

使用带有环境温湿度箱的电磁振动台进行一种航空惯性导航用减振器(JZ-2）的低温动态性能测试,研究了该型减振器的低温(-70℃~20℃）工作特性,得到该减振器的谐振频率以及放大倍数在温度降低条件下的变化规律,并将谐振频率与温度的关系推广至压剪型硅橡胶减振器,为航空器用惯性导航设备在高寒地区的设计以及使用提供参数依据。研究结果表明,当温度低于室温,压剪型橡胶减振器的低温谐振频率与温度的关系符合一阶指数衰减函数。     

不同当量比下氢气体积分数对甲烷-氢混合气预混火焰燃烧不稳定性的影响

在可调振幅的正弦波声场作用下,以甲烷-氢混合气预混钝体火焰为实验对象,通过火焰传递函数表征整个燃烧系统的燃烧不稳定性特征,借助CH基自发荧光图像描述火焰锋面运动及演化过程,研究了在声激励下不同当量比（0.8、1.0、1.2）下氢气体积分数的变化（0、10%、20%）对火焰燃烧不稳定的影响。结果表明: 对于当量比为0.8和1.0的预混火焰,氢气的加入使得火焰传递函数幅值增大,热释放波动变大,整体火焰的不稳定性增强;对于当量比为1.2的富燃预混火焰,随着氢气体积分数的增加,火焰传递函数幅值先减小后增加,火焰稳定性较强。