原子氧对红外干扰材料消光性能的影响研究

为探索大气中的红外干扰材料可否应用于外层空间, 利用原子氧效应地面模拟装置对铜粉和石墨粉两种红外干扰材料样品进行了原子氧暴露实验, 并对样品进行了质量分析、XRD分析和红外透过率测试. 结果表明, 原子氧累积通量达到5.0×1019cm-2时, 铜粉样品质量增加0.004mg•cm-2,石墨粉样品质量损失0.117mg•cm-2; 原子氧暴露后, 铜粉对3~5μm与8~12μm红外质量消光系数由3.64 m2•g-1与2.74 m2•g-1变为3.14 m2•g-1与2.65 m2•g-1, 消光能力降低; 石墨粉对3~5μm和8~12μm红外的质量消光系数由6.54 m2•g-1和5.78 m2•g-1减小为2.38 m2•g-1和2.27 m2•g-1, 消光能力明显减弱.      

基于NMF、ICA和复Contourlet变换的红外小目标检测

针对存在背景干扰和噪声情况下的红外弱小目标检测问题,提出了一种基于非负矩阵分解(NMF)、独立分量分析(ICA)和复Contourlet变换的检测方法。首先通过非负矩阵分解和独立分量分析分别抑制原始图像的背景,得到不同的小目标残差图像;接着采用复Contourlet变换对残差图像进行去噪;再对上述去噪后的小目标残差图像求和,得到了预处理图像;最后提出基于模糊灰度熵阈值选取方法分割预处理图像,从而实现了复杂背景下的红外弱小目标检测。针对红外小目标图像进行了大量实验,并与基于新型Top-hat变换、基于快速独立分量分析的目标检测方法进行了比较,结果表明所提出的方法抗噪性强,具有更为优越的检测性能。     

大口径低温黑体标定装置研制

为了实现更大范围的辐射测量,研制了一套大口径低温黑体标定装置。该装置采用工质制冷技术,避免了大量液氮消耗;采用辐射面竖直放置,有利于红外测量设备标定使用;采取了双参数联动PID控制方案,实现了宽温区辐射体的高稳定性控温。该装置研制中使用了低温黑体的防结霜技术、低温黑体辐射定标温度修正技术、低温黑体校准技术等,为建立低温黑体辐射标准打下基础。     

外场用烟幕遮蔽效果测量系统

首先明确了烟幕透过率、有效遮蔽面积、形成时间与有效持续时间的概念;然后介绍了一套外场试验用烟幕遮蔽效果测量系统,可以同时实现多点、多波段、多波长的红外和激光透过率测量;最后对其主要测量参数作了分析。     

Experimental and numerical study of chaff cloud kinetic performance under impact of high speed airflow

To solve the kinetic and diffusion problem of surface-type infrared decoy, multi-chaff kinetic models are established and chaff cloud holistic kinetic performance are analyzed under the impact of high speed airflow in this work. Chaffs rotate rapidly during the motion under the impact of high speed airflow. The rotation speed is correlated with lift, position of pressure center and aerodynamic damping. Computational Fluid Dynamics (CFD) is used to compute the aerodynamic coefficients of chaff. It is found that there exists serious aerodynamic interference which mainly relates to the overlapping area and distance among chaffs during the diffusion of chaff cloud. The chaff wind tunnel test and rocket sled experiment are carried out to verify the credibility of the models in this work. Then, the variation of chaff cloud expectation and extremum are analyzed to achieve the holistic kinetic and diffusing performance of chaff cloud. Simulation results demonstrate that the chaffs diffuse rapidly under the impact of high speed airflow and chaff cloud can be formed rapidly within 0.5?s. The shape of the chaff cloud is similar to cone that forms a certain angle with the horizontal plane and most chaffs focus on the second half.     

空间拦截红外末制导中的状态估计

本文首先简要地介绍了基于两种规范型的非线性状态观测器的设计方法，然后用该法解决了空间拦截红外末制导中拦截器与目标相对距离的估计问题，仿真结果表明估计的效果良好。     

M导弹制导规则分析

通过分析实测的M导弹制导指令信号数据，给出了该导弹的比例导航系数及其他一些修正系数的变化规律，并根据弹上单片计算机在不同的输入口状态下和其输出口输出数据随时间变化的情况，分析了计算机程序的运行流程及其功能。     

Kinetic temperature and carbon dioxide from broadband infrared limb emission measurements taken from the TIMED/SABER instrument

The Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) experiment is one of four instruments on NASA’s Thermosphere–Ionosphere–Energetics and Dynamics (TIMED) satellite. SABER measures broadband infrared limb emission and derives vertical profiles of kinetic temperature (Tk) from the lower stratosphere to approximately 120 km, and vertical profiles of carbon dioxide (CO₂) volume mixing ratio (vmr) from approximately 70 km to 120 km. In this paper we report on SABER Tk/CO₂ data in the mesosphere and lower thermosphere (MLT) region from the version 1.06 dataset. The continuous SABER measurements provide an excellent dataset to understand the evolution and mechanisms responsible for the global two-level structure of the mesopause altitude. SABER MLT Tk comparisons with ground-based sodium lidar and rocket falling sphere Tk measurements are generally in good agreement. However, SABER CO₂ data differs significantly from TIME-GCM model simulations. Indirect CO₂ validation through SABER-lidar MLT Tk comparisons and SABER-radiation transfer comparisons of nighttime 4.3 μm limb emission suggest the SABER-derived CO₂ data is a better representation of the true atmospheric MLT CO₂ abundance compared to model simulations of CO₂ vmr.     

A new window on the cosmos: The Stratospheric Observatory for Infrared Astronomy (SOFIA)

The Stratospheric Observatory for Infrared Astronomy (SOFIA) is a joint US/German Project to develop and operate a gyrostabilized 2.5-m telescope in a Boeing 747-SP. This observatory will allow astronomical observations from 0.3 μm to sub-millimeter wavelengths at stratospheric altitudes as high as 45,000 ft where the atmosphere is not only cloud-free, but largely transparent at infrared wavelengths. The dynamics and chemistry of interstellar matter, and the details of embedded star formation will be key science goals. In addition, SOFIA’s unique portability will enable large-telescope observations at sites required to observe transient phenomena and location specific events. SOFIA will offer the convenient accessibility of a ground-based telescope for servicing, maintenance, and regular technology upgrades, yet will also have many of the performance advantages of a space-based telescope. Initially, SOFIA will fly with nine first-generation focal plane instruments that include broad-band imagers, moderate resolution spectrographs that will resolve broad features from dust and large molecules, and high resolution spectrometers capable of studying the chemistry and detailed kinematics of molecular and atomic gas. First science flights will begin in 2010, leading to a full operations schedule of about 120 8–10 h flights per year by 2014. The next call for instrument development that can respond to scientifically exciting new technologies will be issued in 2010. We describe the SOFIA facility and outline the opportunities for observations by the general scientific community with cutting edge focal plane technology. We summarize the operational characteristics of the first-generation instruments and give specific examples of the types of fundamental scientific studies these instruments are expected to make.     

基于红外热成像的TC4钛合金光纤激光焊接接头拉伸力学性能研究

对光纤激光焊接2.5mm厚TC4对接接头的拉伸力学性能进行研究,其研究方法为在常规的拉伸试验中,附加同步的红外热像测量,实时记录拉伸全过程中试样在力作用下温度场的变化。常规测试结果表明:接头与母材的强度相当,延伸率只达到母材的59.53%。试样温度场测试结果表明:当接头和母材受到的轴向载荷低于屈服强度对应载荷时,接头在热影响区部位会产生较大的应力集中,但接头和母材均未产生明显的塑性变形;当载荷等于屈服强度对应载荷时,均在宏观屈服点之前发生了微观的塑性变形;当载荷等于抗拉强度对应载荷时,接头发生剧烈塑性变形区域的长度只达到母材的35%,且接头与母材发生剧烈塑性变形区域的长度随拉伸过程的进行逐渐增加。