Speech emotion recognition based on statistical pitch model

A modified Parzen-window method, which keep high resolution in low frequencies and keep smoothness in high frequencies, is proposed to obtain statistical model. Then, a gender classification method utilizing the statistical model is proposed, which have a 98% accuracy of gender classification while long sentence is dealt with. By separation the male voice and female voice, the mean and standard deviation of speech training samples with different emotion are used to create the corresponding emotion models. Then the Bhattacharyya distance between the test sample and statistical models of pitch, are utilized for emotion recognition in speech. The normalization of pitch for the male voice and female voice are also considered, in order to illustrate them into a uniform space. Finally, the speech emotion recognition experiment based on K Nearest Neighbor shows that, the correct rate of 81% is achieved, where it is only 73.85% if the traditional parameters are utilized.     

美国夜视技术的最新进展

美国军方拥有最新的夜视技术，并在继续进一步提高夜视技术，以保持夜战优势。第一代和第二代夜视系统在全世界都可以找到，但是第三代却为美国军方所独有。尽管如此，美国还在继续将高分辨率、传感器融合以及彩色作为其追求目标。     

用高分辩率卫星影像辨识城市建筑物

在对试验区IKONOS卫星高分辨率影像预处理的基础上,采用HIS变换法对1m分辨率全色影像和4m分辨率多光谱影像进行了融合处理;通过建筑物阴影提取了建筑物高程,采用正交小波变换方法提取了图像的纹理信息;采用了四种不同的特征图像组合方式,对试验区高、中、低层建筑物进行了分类.     

Br2分子里德堡态的高分辨转动谱研究

用窄线宽（０．０８ｃｍ＾－＾１）脉冲可调谐紫外激光和（２＋１）多光子电离方法测量了Ｂｒ２的里德堡（Ｒｙｄｂｅｒｇ）态光谱,在７００００－７１５００ｃｍ＾－＾１范围内,获得了溴分子［П３／２］４ｄ振动系列,测量（ｖ＇,ｖ”）＝（１,０）,（２,０）的高分辨振转谱,得到其转动常数Ｂ’７９－８１分别为０．０８８３２和０．０８８０５ｃｍ＾－＾１,并提出此系列的角动量量子数Ω应为１。     

基于能量对称分布相位相关配准的资源三号02星颤振探测

颤振是卫星平台在轨运行的固有现象之一,也是高分辨率对地观测卫星研究的难点和热点。针对资源三号02星在轨运行过程中的平台颤振情况,提出了一种基于能量对称分布的相位相关配准算法。结合多光谱相机各谱段相机之间的安装关系,考虑到平台的线性平滑运动特性,采用二次函数消除系统变化量,得到线性拟合的平台颤振曲线,最后利用星敏陀螺数据联合滤波得到卫星姿态复合验证曲线。实验结果表明:在模拟数据情况下,所提配准算法的配准精度能够达到0.05 pixel,可有效辅助探测卫星平台的颤振,并首次探测到资源三号02星平台存在0.63～0.65 Hz的颤振,振幅为0.41″～1.12″。     

Coherent Vibrational Dynamics and High-resolution Nonlinear Spectroscopy： A Comparison with the Air/DMSO Liquid Interface

We present a comparative study on the C-H stretching vibrations at air/DMSO （dimethyl sulfoxide） interface with both the free-induction decay （FID） coherent vibrational dynamics and the sub-wavenumber high resolution sum-frequency generation vibrational spectroscopy measurements. In principle the frequency-domain and time-domain spectroscopic measurements should generate identical information for a given molecular system. However, when the molecular systems are with several coupled or overlapping vibrational modes, obtain- ing detailed spectroscopic and coherent dynamics information is not as straightforward and rather difficult from either the time-domain or the frequency domain measurements. For the case of air/DMSO interface that is with moderately complex vibrational spectra, we show that the frequency-domain measurement with sub-wavenumber high-resolution sum-frequency generation vibrational spectroscopy is probably more advantageous than the time- domain measurement in obtaining quantitative understanding of the structure and coherent dynamics of the molecular interface.     

细菌感染成像的研究进展

由致病菌或条件致病菌侵入机体繁殖而产生的毒素和其它代谢产物所引起的感染性疾病是目前全球范围内的主要死亡原因之一. 感染性疾病的早期诊断是对其进行有效治疗与控制的重要途径. 分子影像技术的快速发展给体内细菌感染的评估带来了前所未有的变化和机遇. 本文综合评述了计算机断层扫描、 正电子发射断层扫描、 超声成像、 磁共振成像、 荧光成像及光声成像等成像方式在细菌感染体内成像中的研究进展、 不足和发展方向等, 以期为活体细菌感染检测方法的发展提供参考.     

一个改进的三阶WENO-Z型格式

在WENO-Z型格式框架下,基于高阶全局光滑因子,在非线性权建立过程中引入参数,通过收敛性分析确定参数取值范围,兼顾精确性与不振荡性,得到参数最佳取值.最终得到一个低耗散、高分辨率的三阶WENO差分格式,该格式在函数一阶极值点处仍保持预期三阶精度.最后通过精确解算例验证了格式在各种类型极值点处精度恢复情况,并通过一、二...     

基于6S模型的遥感影像逐像元大气纠正算法

大气纠正的目的是从遥感影像中去除大气影响,并反演获取地物真实反射率。介绍了一种逐像元对遥感影像进行大气纠正的算法,该算法基于6S(Second Simulation of the Satellite Signal in the Solar Spectrum)大气辐射传输模型计算建立的查找表(look-up table),并利用地面暗目标(dark object)进行陆地气溶胶光学厚度的自动反演,由于气溶胶的分布具有空间连续性,在获取地面暗目标气溶胶光学厚度值后,通过空间插值的方法计算影像中非暗目标像元的气溶胶光学厚度值,经过查找表二次插值计算,逐像元进行大气纠正并获取像元地表反射率值。以Landsat5遥感影像为例,介绍了算法流程,展示了大气纠正的结果。结果显示,利用查找表逐像元大气纠正的算法,能够在一定程度上去除云雾对影像的影响,更加精确的对遥感影像进行大气纠正并获取地物的真实反射率。     

用于观测细胞培养罐的显微系统设计

由于现有实验室显微镜物距较小,且光源发散角较大,无法实时对培养罐中细胞进行观测,设计了一款用于不同容量细胞培养罐外部观测的显微系统,系统工作距离45mm,NA=0.19,像方分辨率δ=10.8μm,实现在细胞培养罐外部进行检测.设计结果表明子午线与胡矢线重合较好,与理论衍射极限接近,在空间频率881p/mm下,各视场M...