浅谈陶瓷基复合材料无损检测方法及其进展

陶瓷基复合材料由于其具有耐高温、密度低、抗氧化性好等多种优良特性目前已广泛地应用于航空航天领域。采用无损检测方法对陶瓷基复合材料进行相关检测对保证材料产品质量以及提高产品使用的可靠性等都具有重要意义。综述了陶瓷基复合材料无损检测发展现状,阐述了太赫兹、X射线、工业CT、红外热成像、超声波及声发射技术等常用陶瓷基复合材料检测手段的原理并介绍了其在陶瓷基复合材料无损检测方面的应用实例。     

EBAA：An efficient broadcast authentication scheme for ADS-B communication based on IBS-MR

Automatic dependent surveillance-broadcast （ADS-B） systems can broadcast satellitebased aircraft position, identification, etc., periodically, and are now on track to replace radar to become the backbone of next-generation air traffic management （ATM） systems. However, ADS-B systems suffer severe cyber-security problems due to the broadcast-type data link and the lack of designed-in security measures. Especially, since ADS-B messages are unauthenticated, it is easy to insert fake aircraft into a system via spoofing or insertion of false messages. Unfortu- nately, the authentication for ADS-B messages has not yet been well studied. In this paper, based on identity-based signature with message recovery （IBS-MR）, an efficient broadcast authentication scheme for ADS-B messages is proposed. The security analysis demonstrates that the scheme can achieve authenticity and integrity of ADS-B broadcast messages, as well as adaptive evolution of broadcasters＇ private keys. The performance evaluation shows that the scheme is computationally efficient for typical avionics devices with limited resources. Furthermore, the scheme achieves low communication overhead since broadcast messages can be recovered from signatures, and thus it is suitable for low-bandwidth ADS-B data link.     

降低表面温度和发射率抑制排气系统红外辐射的研究

为了降低涡扇发动机轴对称排气系统的红外辐射特征,研究了降低排气系统腔体表面温度和发射率抑制红外辐射的规律。首先通过模拟实验研究了对中心锥进行冷却和涂覆低发射率涂层的红外抑制效果;然后用实验数据对本文使用的红外辐射特征计算方法和程序进行了验证;最后通过数值计算研究了典型尺寸的涡扇发动机排气系统降温和发射率分布对红外辐射特征的影响规律。结果表明：降低中心锥等部件的温度和发射率可明显降低排气系统在α〈15°范围内的红外辐射强度;若中心锥的温度降低100K,中心锥、涡轮和径向稳定器等部件的表面发射率降至0.2,则排气系统尾向的红外辐射强度可降低40%以上,探测距离缩短20%左右。     

CO_2激光焊接TC4熔池红外光辐射信号与焊接参数的关系

利用CCD摄像机以及红外光辐射信号监测系统系统地研究了钛合金TC4激光焊接过程中红外光辐射信号的特征以及焊接线能量与熔池红外光辐射信号熔池面积的关系。研究表明,(1)对应整条焊缝,红外光辐射信号可明显分为3个阶段,分别对应焊接起始阶段、准稳态阶段及焊接收弧阶段(;2)当线能量增加(功率不变焊接速度降低)时,熔池面积变大,红外光辐射信号相对强度随之增强;(3)熔池面积与红外光辐射信号相对强度之间存在相同的变化规律,因此利用红外光辐射信号可以相当准确地监测焊接过程的熔池面积变化,进而监测焊接过程的稳定性。     

基于均值漂移算法的冷空炽热体红外目标跟踪

Mean Shift（均值漂移）算法对彩色序列图像目标跟踪是有效的,而对红外目标跟踪是不稳健的。本文对Mean Shift算法做适当改进,将其用于冷空炽热体红外目标跟踪。先对红外图像做伽马变换,把目标从背景中分离出来;用直方图非均匀量化改进传统Mean Shift算法量化方式,提高目标定位准确性。仿真结果表明,该方法对冷空炽热体红外目标跟踪是有效的和稳健的。     

Status of the Stratospheric Observatory for Infrared Astronomy (SOFIA)

The Stratospheric Observatory for Infrared Astronomy (SOFIA), a joint US/German project, is a 2.5-m infrared airborne telescope carried by a Boeing 747-SP that flies in the stratosphere at altitudes as high as 45,000 ft (13.72 km). This facility is capable of observing from 0.3 μm to 1.6 mm with an average transmission greater than 80% averaged over all wavelengths. SOFIA will be staged out of the NASA Dryden Flight Research Center aircraft operations facility at Palmdale, CA. The SOFIA Science Mission Operations (SMO) will be located at NASA Ames Research Center, Moffett Field, CA. First science flights began in 2010 and a full operations schedule of up to one hundred 8 to 10 hour-long flights per year will be reached by 2014. The observatory is expected to operate until the mid-2030s. SOFIA’s initial complement of seven focal plane instruments includes broadband imagers, moderate-resolution spectrographs that will resolve broad features due to dust and large molecules, and high-resolution spectrometers capable of studying the kinematics of atomic and molecular gas at sub-km/s resolution. We describe the SOFIA facility and outline the opportunities for observations by the general scientific community and for future instrumentation development. The operational characteristics of the SOFIA first-generation instruments are summarized. The status of the flight test program is discussed and we show First Light images obtained at wavelengths from 5.4 to 37 μm with the FORCAST imaging camera. Additional information about SOFIA is available at http://www.sofia.usra.edu and http://www.sofia.usra.edu/Science/docs/SofiaScienceVision051809-1.pdf.     

Infrared detection,review of existing and future devices

I present the current status of arrays of detectors operating in the 1–200 micron range, restricted to mature devices, and two recent concepts of infrared detection which could lead to future developments.     

涡扇发动机最小红外特征模式性能寻优控制研究

为抑制涡扇发动机排气系统的红外特征,提出一种基于红外预测模型的最小红外特征模式性能寻优控制。首先,建立一种排气系统正后向红外辐射强度简化预测模型,该预测方法考虑了排气系统内高温部件和尾喷流的红外辐射,以及尾喷流对高温部件红外辐射的吸收作用,具有可信的仿真精度;其次,基于涡扇发动机部件级实时仿真模型,增加了从外涵引气冷却中心锥和尾喷管扩张段内壁的冷却结构和红外预测模块;最后,基于该模型探索了最小红外特征模式的优化原理,并选用可行序列二次规划(FSQP)算法,通过控制高温壁面冷却气的流量,主燃烧室的燃油量以及尾喷管喉道面积,对两个亚声速巡航状态的工作点进行实时优化。仿真结果表明:在满足发动机推力恒定以及其他约束条件的前提下,发动机通过最小红外特征模式性能寻优控制,其排气系统后向红外辐射下降了30%以上,红外抑制效果显著。