硅光电倍增探测器温度特性分析与实验

SiPM(Silicon Photo-multiplier,硅光电倍增探测器)是近年来逐渐兴起的一种用于光探测领域的光电探测器件。与传统的PMT(Photo-multiplier tube,光电倍增管)相比,它有着尺寸小、工作电压低、几乎不受磁场影响等优点,但其缺点是对环境温度变化较敏感。为了掌握SiPM性能指标随环境温度的变化规律,搭建了SiPM温度特性实验系统,通过改变环境温度来实时测量记录SiPM的雪崩临界电压和增益,从而定量得出SiPM的温度特性,并通过理论计算对实验数据进行分析。结果表明,当环境温度降低时,SiPM的雪崩临界电压随之线性下降,增益随之线性增大。     

空间用硅太阳电池带通滤波器的研究

为改善硅太阳电池在轨工作期间的性能,通过对空间用太阳电池带通滤波器结构设计和制备工艺的研究,研制出一种空间用硅太阳电池的带通滤波器并对其性能进行了测试,结果表明,采用该带通滤波器可使硅太阳电池在轨工作温度降低6°C～12°C,输出功率增加1.8%～4.1%.带通滤波器的研制对于促进高效硅太阳电池的空间应用具有积极意义.     

Dispersion-free quantum clock synchronization via fiber link

We proposed a fiber-based quantum clock synchronization protocol by employing the dispersion cancellation feature of the frequency anti-correlated entangled source under the quantum interference measurement. It is shown that, the accuracy of the synchronization is mainly dependent on the bandwidth of the frequency entangled biphoton spectrum and on the temperature variation induced fluctuations in both the reference fiber coiling and the fiber link. With this proposal, synchronization between two clocks at a distance of ten kilometers can be implemented with an accuracy below a picosecond.     

聚碳硅烷/纳米钛粉的热裂解

运用ＩＲ、ＸＲＤ和ＴＧ等分析手段研究了掺混纳米钛粉的聚碳硅烷的热裂解过程。发现热解过程可分为有机硅聚合物转化为无机无定形态和无定形态生长为微晶成。裂解产物中钛的存在形态随保护气氛不同而不同,保护气氛为氮气或氨气时钛的裂解产物为ＴｉＮ,氩气时为ＴｉＣ。     

一锅法合成SiC-ZrC复相陶瓷前驱体及其性能

以甲基三氯硅烷、二氯二甲基硅烷、二氯二茂锆以及金属钠为原料,通过一锅反应合成出一种全新的SiC-ZrC复相陶瓷前驱体(HBZS)。利用TG、FTIR、XRD及SEM等对HBZS的热解行为、分子结构以及热解产物的微观形貌与结构进行了全面分析。结果表明:HBZS在900℃时可以完全裂解转化成SiC-ZrC复相陶瓷,陶瓷收率可达60%以上;裂解产物中ZrC相晶粒尺寸极小(10～45 nm)且均匀分散于连续的SiC相中。该前驱体可用于制备SiC-ZrC陶瓷纤维及陶瓷基复合材料。     

航空微机电系统非硅材料微纳加工技术

随着对航空飞行器智能控制的迫切需求,硅基微机电系统MEMS(Micro-electromechanical Systems)传感器和执行器难以满足飞行器恶劣的运行环境,因而以碳化硅、氮化铝等为代表的多种MEMS特种材料被不断研究和使用.概述这些特种材料的机电特性有利于缩小特种传感器研发的材料选择范围;而针对兼具机械和电学两方面应用的碳化硅、氮化铝和聚合物前驱体陶瓷开展微纳加工技术的综述,有利于全面了解这3种材料的成型成性关键工艺,进而揭示从航空特种材料到MEMS器件的加工技术发展规律,为普遍使用电信号的航空特种传感器的研发提供加工手段借鉴.     

碳化硅陶瓷基复合材料加工技术研究进展

碳化硅陶瓷基复合材料(CMC-SiC)是一种新型战略性热结构材料,在航空、航天、核能等高新技术领域具有广阔应用前景.但CMC-SiC材料硬度高、不导电等特性决定了实现其高精度、高质量加工较为困难.综述了CMC-SiC材料的传统加工和特种加工工艺的研究现状与进展,重点阐述了激光加工陶瓷及CMC-SiC材料的加工机理和加工效果.最后,指出了CMC-SiC材料加工技术的发展趋势.     

大尺寸轻型SiC光学反射镜研究进展

本文比较了光学玻璃、硅、铍，碳化硅等太空反向镜片材料的物理性能和机械性能，着重介绍了新型光学反向镜片材料碳化硅的种类、制造和应用，并讨论了碳化硅作为太空反向镜片材料目前存在的问题及发展方向。     

识别大学生心理咨询言语隐藏性的快捷方法--从表情"测谎"

通过表情反映情绪变化的论述，说明了表情可以“测谎”。表情“测谎”又分为面部表情“测谎”，体态表情“测谎”和言语表情“测谎”，它已成为识别大学生心理咨询言语隐藏性的快捷方法。     

Advanced Technologies Demonstrated by the Miniature Integrated Camera and Spectrometer (MICAS) Aboard Deep Space 1

MICAS is an integrated multi-channel instrument that includes an ultraviolet imaging spectrometer (80–185 nm), two high-resolution visible imagers (10–20 μrad/pixel, 400–900 nm), and a short-wavelength infrared imaging spectrometer (1250–2600 nm). The wavelength ranges were chosen to maximize the science data that could be collected using existing semiconductor technologies and avoiding the need for multi-octave spectrometers. It was flown on DS1 to validate technologies derived from the development of PICS (Planetary Imaging Camera Spectrometer). These technologies provided a novel systems approach enabling the miniaturization and integration of four instruments into one entity, spanning a wavelength range from the UV to IR, and from ambient to cryogenic temperatures with optical performance at a fraction of a wavelength. The specific technologies incorporated were: a built-in fly-by sequence; lightweight and ultra-stable, monolithic silicon-carbide construction, which enabled room-temperature alignment for cryogenic (85–140 K) performance, and provided superb optical performance and immunity to thermal distortion; diffraction-limited, shared optics operating from 80 to 2600 nm; advanced detector technologies for the UV, visible and short-wavelength IR; high-performance thermal radiators coupled directly to the short-wave infrared (SWIR) detector optical bench, providing an instrument with a mass less than 10 kg, instrument power less than 10 W, and total instrument cost of less than ten million dollars. The design allows the wavelength range to be extended by at least an octave at the short wavelength end and to ∼50 microns at the long wavelength end. Testing of the completed instrument demonstrated excellent optical performance down to 77 K, which would enable a greatly reduced background for longer wavelength detectors. During the Deep Space 1 Mission, MICAS successfully collected images and spectra for asteroid 9969 Braille, Mars, and comet 19/P Borrelly. The Borrelly encounter was a scientific hallmark providing the first clear, high resolution images and excellent, short-wavelength infrared spectra of the surface of an active comet’s nucleus.