红外探测器参数自动计量测试

介绍了我站的红外探测器参数（黑体响应率，噪声、黑体探测率）自动测试系统以及参数测试关键技术的解决分析了这些参数测量不确定度。     

固体火箭发动机专用ICT机械扫描系统

以成熟的组合精密镗床为本体, 研制了固体发动机专用ＩＣＴ机械扫描系统。采用４５０ ｋＶ Ｘ射线源, 设计了准直器系统、探测器系统、机械扫描系统（传动控制系统、夹具及同步台）, 实测证明扫描系统符合精度要求     

Development of in-situ Space Debris Detector

Due to high relative velocities, collisions of spacecraft in orbit with Space Debris (SD) or Micrometeoroids (MM) can lead to payload degradation, anomalies as well as failures in spacecraft operation, or even loss of mission. Flux models and impact risk assessment tools, such as MASTER (Meteoroid and Space Debris Terrestrial Environment Reference) or ORDEM (Orbital Debris Engineering Model), and ESABASE2 or BUMPER II are used to analyse mission risk associated with these hazards. Validation of flux models is based on measured data. Currently, as most of the SD and MM objects are too small (millimeter down to micron sized) for ground-based observations (e.g. radar, optical), the only available data for model validation is based upon retrieved hardware investigations e.g. Long Duration Exposure Facility (LDEF), Hubble Space Telescope (HST), European Retrievable Carrier (EURECA). Since existing data sets are insufficient, further in-situ experimental investigation of the SD and MM populations are required. This paper provides an overview and assessment of existing and planned SD and MM impact detectors. The detection area of the described detectors is too small to adequately provide the missing data sets. Therefore an innovative detection concept is proposed that utilises existing spacecraft components for detection purposes. In general, solar panels of a spacecraft provide a large area that can be utilised for in-situ impact detection. By using this method on several spacecraft in different orbits the detection area can be increased significantly and allow the detection of SD and MM objects with diameters as low as 100 μm. The design of the detector is based on damage equations from HST and EURECA solar panels. An extensive investigation of those panels was performed by ESA and is summarized within this paper. Furthermore, an estimate of the expected sensitivity of the patented detector concept as well as examples for its implementation into large and small spacecraft are presented.     

基于感应传感的位置增量编码器设计

为解决传统编码器的易损坏、可靠性不高、更换价格昂贵的问题,提出采用非接触式、电感感应传感设计位置编码器的方案。用LDC1312数字电感传感器作为感应探头,检测涂有金属物的旋转圆盘,将其感应测量到的数据通过IIC接口送入MSP430F5529处理数据,实现对旋转圆盘位置的检测。该设计与机械编码器相比,具有寿命长、可靠性高,适用于在油渍、潮湿、灰尘等恶劣环境工作的优点。     

Solar X-ray Monitor (XSM) on-board Chandrayaan-2 orbiter

The remote X-ray fluorescence spectroscopy is a powerful technique to investigate the elemental abundances in the atmosphere-less planetary bodies. The experiment involves measuring spectra of fluorescent X-rays from lunar surface using a low energy X-ray detector onboard an orbiting satellite. Since the flux of fluorescent X-ray lines critically depend on the flux and spectrum of the incident solar X-rays, it is essential to have simultaneous and accurate measurement of X-ray from both Moon and Sun. In the context of Moon, this technique has been employed since early days of space exploration to determine elemental composition of lunar surface. However, so far it has not been possible to exploit it to its full potential due to various reasons. Therefore it is planned to continue the remote X-ray fluorescence spectroscopy experiment on-board Chandrayaan-2 which includes both lunar X-ray observations and solar X-ray observations as two separate payloads. The lunar X-ray observations will be carried out by Chandra Large Area Soft x-ray Spectrometer (CLASS) experiment; whereas the solar X-ray observations will be carried out by a separate payload, Solar X-ray Monitor (XSM). Here we present the overall design of the XSM instrument, the present development status as well as preliminary results of the laboratory model testing. XSM instrument will have two packages namely – XSM sensor package and XSM electronics package. XSM will accurately measure spectrum of Solar X-rays in the energy range of 1–15 keV with energy resolution ∼200 eV @ 5.9 keV. This will be achieved by using state-of-the-art Silicon Drift Detector (SDD), which has a unique capability of maintaining high energy resolution at very high incident count rate expected from Solar X-rays. XSM onboard Chandrayaan-2 will be the first experiment to use such detector for Solar X-ray monitoring.     

家用火灾自动报警装置的设计

城市家庭安装火灾自动报警装置非常必要。使用单片机,选用数字化温度传感器和烟雾检测器作为敏感元件,利用多传感器信息融合技术,设计适用于家庭的火灾报警装置,可使整个系统硬件电路设计合理,性能安全可靠。     

新机试飞中的进气道旋流测量

测量新机试飞中的旋流及稳、动态压力畸变，即可全面评审进气道／发动机的相容性。根据进气道流场分析，建立一种适合于空中使用的旋流测量技术，并提出了解决问题的途径，介绍了Ｔ８７探的设计、性能、特点、试验结果。     

等离子体对空间飞行器表面充电效应探测研究

为确保空间飞行器在轨安全，有必要搭载探测器对轨道空间环境进行实时监测，获取表面充电效应数据。在对轨道空间充电环境分析的基础上，确定探测器的任务目标并完成基于电位探头和电流探头的探测器方案设计，包括探头设计和电路设计。探测器设计方案在空间环境特殊效应测量领域迈出的关键一步，为更多空间效应参数的测量奠定了坚实基础。     

波段探测率D_(△λ)~*替代峰值探测率D_(λp)~*的讨论

文中描述了波段探测率D_(Δλ)~*的定义和计算方法,通过对空间应用的长波红外探测器的波段探测率D_(Δλ)~*与目标辐射源温度T的关系讨论,来说明波段探测率D_(Δλ)~*(和波段响应率)替代峰值探测率D_(Δλ)~*(和峰值响应率)的优越性,文中还给出了波段探测率D_(Δλ)~*的测试方法和实验计算。     

激光吸收法辐射测温技术研究

对辐射测温技术的发展进行了回顾，总结了辐射测温中遇到的主要问题，分析了激光吸收法辐射测温技术的发展现状，对激光吸收法辐射测温技术的理论模型进行了公式推导，对本单位建立的实验装置及其测温结果进行了介绍。