随机载荷谱下基于声发射的耳片接头疲劳裂纹识别方法

作为航空结构中传递集中载荷的关键部件,耳片接头的失效将会带来灾难性的后果,因此需要通过疲劳试验来验证其是否满足设计要求。声发射（AE）作为一种在线监测手段,能够及时捕捉接头裂纹萌生扩展进程,提升试验质量。然而,在随机载荷谱下,会产生大量极其复杂且毫无规律的声发射信号,致使传统的基于特征提取及参数滤波的声发射数据分析方法难以发挥作用,无法有效识别接头裂纹的萌生。因此,本文提出了一种随机载荷谱下疲劳裂纹的声发射识别方法,该方法利用随机载荷谱的分布特点,通过分析不同载荷谱块下相同循环时段所对应的声发射信号表象差异来发现、锁定异常,并结合定位分析与干扰排除分析,确定裂纹的发生时间及位置。通过疲劳试验,该方法的有效性得到了证实,因而可为随机载荷谱下的相关航空结构试验提供参考。     

基于近似熵谱的碳纤维复合材料层压板拉伸损伤声发射分析

采用近似熵理论分析了碳纤维环氧树脂层压板在拉伸过程中产生的三种典型声发射信号。研究 表明基体开裂、脱胶以及纤维断裂这三种信号的近似熵谱特征不同,结合经验模式分解方法解释了三种损伤破 坏机制。此外,在经验模式分解的基础上考察了三种声发射信号本征模函数的频谱分布,进一步说明了近似熵 在本质上是衡量信号发生新振动模式产生的概率以及在复合材料声发射检测与损伤识别中使用近似熵谱分析 的有效性。     

近地轨道飞行器的光辐射背景环境

文章简要介绍了在可见光和红外波段深空和地球高层大气的光辐射源和辐射特性,包括辐射机制和强度、辐射的各向异性等,通过比较表明空间红外波段的背景辐射明显高出可见光波段近1个数量级;分析了在地球大气外进行对地观测时大气辉光辐射的角分布,指出了辐射的临边增亮特性。以上研究对于研制和开发新型航天器、利用太空资源以及未来的深空探测都具有实用价值。     

HTPB推进剂细观损伤机理的声发射实验研究

采用测定单轴定速拉伸条件下标准哑铃形ＨＴＰＢ推进剂件声发射（ＡＥ）信号的方法,对ＨＴＰＢ复合固体推进剂在载荷作用下细观损伤及其扩展的机理进行了研究。实验结果表明：声发射累计能量对应于细观损伤产生和扩展两个不同阶段,提出了一个描述ＨＴＰＢ复合固体推进剂细观损伤扩展的物理模型,该模型解释了不同拉伸速率下ＨＴＰＢ复合固体推进剂破坏了后出现的不同物理现象。     

Cut-off features in interplanetary solar radio type IV emission

Solar radio type IV bursts can sometimes show directivity, so that no burst is observed when the source region in located far from the solar disk center. This has recently been verified also from space observations, at decameter wavelengths, using a 3D-view to the Sun with STEREO and Wind satellites. It is unclear whether the directivity is caused by the emission mechanism, by reduced radio wave formation toward certain directions, or by absorption/blocking of radio waves along the line of sight. We present here observations of three type IV burst events that occurred on 23, 25, and 29 July 2004, and originated from the same active region. The source location of the first event was near the solar disk center and in the third event near the west limb. Our analysis shows that in the last two events the type IV bursts experienced partial cut-offs in their emission, that coincided with the appearance of shock-related type II bursts. The type II bursts were formed at the flanks and leading fronts of propagating coronal mass ejections (CMEs). These events support the suggestion of absorption toward directions where the type II shock regions are located.     

Use of coated silicon field emitters as neutralisers for fundamental physics space missions

Spacecraft neutralisers are required as part of the ion propulsion system for accurate station keeping in fundamental physics missions. This paper describes the use of thin layers of insulating materials as coatings for the gated silicon field emitter array structure used in a spacecraft neutraliser. These thin coatings are postulated to reduce power consumption and reduce overheating. The power consumption and lifetime of aluminium nitride and amorphous hydrogenated diamond-like carbon coatings have been tested by current–voltage and endurance tests. Diamond-like carbon coatings were promising, performing better in endurance tests than uncoated samples, but further work is required to characterise the coating’s physical properties and its effects on field emission. The thermal conductivity of the coating material had little effect on measured sample lifetimes. Aluminium nitride had reduced power consumption compared to diamond-like carbon coated and uncoated samples. A thin (∼5 nm) layer of aluminium nitride was found to be optimal, meeting European Space Agency specifications for the neutraliser engineering model.     

超高强度钢不同性质缺陷的声发射特性研究

研究了超高强度钢30Si2MnCrMoVE的声发射特性,针对裂纹、夹钨、未焊透等几种常见焊接缺陷的声发射数据进行了分析,为相关产品的声发射检测结果评定提供参考,以此提高声发射技术在超高强度钢产品质量检测上的可靠性。     

低温点源黑体关键技术及国内外发展现状

文章分析了低温点源黑体设备研制中的几项关键技术,包括3种常见发射腔腔形的特点,腔体发射率的计算方法,以及热管,恒温浴和液氮电加热3种恒温方式的原理和技术特性;比较了国内外典型低温黑体设备、产品的性能指标;并简述低温点源黑体设备在红外定标试验中的原理和应用.最后总结出现阶段低温点源黑体的发展水平以及未来的研究重点.     

正激波后OH A~2∑~+──X~2∏瞬态光谱的测量

用光学多道分析仪（OMA光学系统）测量了氢氧燃烧驱动激波管中典型状态下正激波后高温空气不同时刻的瞬态光谱。光谱结果显示高温空气的光谱中有很强的OHA2∑＋─X2∏光谱。通过采用线线合成光谱的方法得到激波后不同时刻高温空气中OH分子的转动温度。     

Limb Viewing Hyper Spectral Imager (LiVHySI) for airglow measurements onboard YOUTHSAT-1

The Limb Viewing Hyper Spectral Imager (LiVHySI) is one of the Indian payloads onboard YOUTHSAT (inclination 98.73°, apogee 817 km) launched in April, 2011. The Hyper-spectral imager has been operated in Earth’s limb viewing mode to measure airglow emissions in the spectral range 550–900 nm, from terrestrial upper atmosphere (i.e. 80 km altitude and above) with a line-of-sight range of about 3200 km. The altitude coverage is about 500 km with command selectable lowest altitude. This imaging spectrometer employs a Linearly Variable Filter (LVF) to generate the spectrum and an Active Pixel Sensor (APS) area array of 256 × 512 pixels, placed in close proximity of the LVF as detector. The spectral sampling is done at 1.06 nm interval. The optics used is an eight element f/2 telecentric lens system with 80 mm effective focal length. The detector is aligned with respect to the LVF such that its 512 pixel dimension covers the spectral range. The radiometric sensitivity of the imager is about 20 Rayleigh at noise floor through the signal integration for 10 s at wavelength 630 nm. The imager is being operated during the eclipsed portion of satellite orbits. The integration in the time/spatial domain could be chosen depending upon the season, solar and geomagnetic activity and/or specific target area. This paper primarily aims at describing LiVHySI, its in-orbit operations, quality, potential of the data and its first observations. The images reveal the thermospheric airglow at 630 nm to be the most prominent. These first LiVHySI observations carried out on the night of 21st April, 2011 are presented here, while the variability exhibited by the thermospheric nightglow at O(¹D) 630 nm has been described in detail.