能量和协方差检验的联合频谱感知算法研究

快速准确的频谱感知是认知无线电系统有效通信的前提。现有的能量检测算法易受噪声波动影响,为提高频谱感知的性能,采用了联合频谱感知算法。方法利用双门限的能量检测法进行粗检,并使用协方差检测算法对中间混淆区域进行二次判决。在噪声不确定的情况下,对联合频谱感知算法性能进行了仿真分析。仿真结果表明,在噪声波动较大时,算法有效地提高频谱检测的性能,而且计算复杂度得到降低,并优于能量检测法和协方差检测法。     

ISO Observations of Pre-Stellar Cores and Young Stellar Objects

We summarize the observations of the Infrared Space Observatory (ISO) concerning the earliest stages of the stellar formation. The observations of samples of sources in different evolutionary stages are reviewed, addressing in particular how the physical and chemical properties of the protostellar environments change from the pre-stellar cores to the protostars at the end of their accretion phase. In addition, the mid-IR surveys in nearby star-forming regions are discussed, showing their implications for the understanding of the stellar initial mass function. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

Deriving remote sensing reflectance from turbid Case II waters using green-shortwave infrared bands based model

The objectives of this study are to validate the applicability of a shortwave infrared atmospheric correction model (SWIR-based model) in deriving remote sensing reflectance in turbid Case II waters, and to improve that model using a proposed green-shortwave infrared model (GSWIR-based model). In a GSWIR-based model, the aerosol type is determined by a SWIR-based model and the reflectance due to aerosol scattering is calculated using spectral slope technology. In this study, field measurements collected from three independent cruises from two different Case II waters were used to compare models. The results indicate that both SWIR- and GSWIR-based models can be used to derive the remote sensing reflectance at visible wavelengths in turbid Case II waters, but GSWIR-based models are superior to SWIR-based models. Using the GSWIR-based model decreases uncertainty in remote sensing reflectance retrievals in turbid Case II waters by 2.6–12.1%. In addition, GSWIR-based model’s sensitivity to user-supplied parameters was determined using the numerical method, which indicated that the GSWIR-based model is more sensitive to the uncertainty of spectral slope technology than to that of aerosol type retrieval methodology. Due to much lower noise tolerance of GSWIR-based model in the blue and near-infrared regions, the GSWIR-based model performs poorly in determining remote sensing reflectance at these wavelengths, which is consistent with the GSWIR-based model’s accuracy evaluation results.     

《高频电子线路》课程“相乘器”教学策略

相乘器是高频电子线路课程中的一个重要单元电路。掌握相乘器的组成、基本原理、分析方法以及器件特点是通信电子信息类学生学好调制、检波以及混频电路的关键所在,讨论非线性器件二极管在开关状态下组成"相乘器"的教学策略对教学活动具有重要意义。     

特型钝体绕流动态特性的低速实验研究

在低速自由射流风洞上 ,利用热线及相关设备对由半球头部、颈部及旋成体构成的特型钝体周围非定常流动的基本特性、联合特性及湍流度分布进行了测试与分析 ,实验工况为迎角α=- 1 5°～ 1 5°、侧滑角 β =0°～ 1 0°。结果表明 ,在上述工况范围内 ,该钝体周围流场中速度脉动的能量分布平坦 ,属宽频带随机信号 ,流场中没有发生明显的流动分离 ,流场动态品质良好 ;凹陷区内气流的脉动以不同的速度向下游空间传播 ;在上述α、β变化范围内 ,钝体颈部凹陷区的最大湍流度高达 1 0 .9～ 2 4.8%。     

考虑高度参数的摆动式红外地球敏感器模型研究

本文考察了摆动式红外地球敏感器测量的工作原理,在介绍敏感器两种数学模型—圆盘模型和三维模型的基础上,增加卫星轨道高度参数为变量,讨论了在不同轨道高度下,敏感器数学模型的变化.利用小角度条件下的一阶近似处理,对敏感器模型所关心的弦宽与姿态角转换关系给出了解答.通过进行带有高度参数的修正,把敏感器的圆盘模型和三维模型推广到了其他轨道高度下.     

一种红外焦平面阵列相对光谱响应自动测试系统

目前测试红外焦平面阵列相对光谱响应参数时，需要人工测量波段中每个波长点的光谱响应，针对测试过程繁琐和测试时间长的问题，在基于现有的不同开发平台开发的单色仪和数据采集系统的基础上，利用动态链接库技术，研制了一种红外焦平面阵列相对光谱响应自动测试系统，该系统测试过程简化，自动化程度提高。经过对比分析，自动测试与人工测试结果具有较好的一致性，自动测试比人工测试更加可靠。     

卷簧式柔性取样器的取样头-岩石接触原位辨识(英文)

取样头和岩石接触问题与月壤取样的成功与否直接相关,基于小型卷簧式月壤取样器的柔性取样臂结构,提出了振动取样法:在取样过程中采集振动信号进行数字信号处理与分析,达到对取样头-岩石接触的辨识。首先对振动信号进行采集、消除趋势项,然后利用小波多分辨分析去噪,采用现代功率谱中基于AR模型的Burg法对振动信号进行特征提取,最后采用二分类支持向量机对取样头是否接触到岩石进行识别。实验结果证明,卷簧式取样器的振动信号分析能够对取样头-岩石接触问题进行较好的辨识。     

关于飞机结构疲劳载荷谱低载截除水平选取的探讨

低载截除作为飞机结构疲劳载荷谱简化的重要内容之一，可以大幅节省疲劳试验的时间与成本，然而目前对于低载截除水平的选取尚无公认的标准方法。本文对文献中已有的低载截除水平进行广泛地搜集，将低载截除水平划分为基于材料疲劳极限与基于谱最大载荷的两种选取方式，探究两种选取方式之间的联系，建立低载截除水平关系模型。结果表明：两种低载截除水平选取方式本质上是一致的，基于谱最大载荷的选取方式结合了飞机载荷与结构材料的特点，是对基于材料疲劳极限选取方式的延伸，所建立的低载截除水平关系模型能够为实际工程中疲劳载荷谱简化时低载截除水平的确定提供参考。     

On bandwidth of solar subsecond bursts in cm-range

The goal is to study parameters of drifting type III bursts, and find out the emission mechanism of these bursts and understand what factors affect instantaneous spectral bandwidth of these bursts.