概率论教学方法改革与实践

本文作者结合教学实践,介绍了六种教学方法,即趣味性教学、应用性教学、对比式教学、讨论式教学、多媒体教学和双语教学。     

Characterization of a nitrogenase CrFe protein from a mutant UW3 of Azotobacter vinelandii grown on a Cr-containing medium

Biological nitrogen fixation is one of the most im-portant biochemical reactions in nature. It is catalyzed by an anaerobic metalloenzyme complex-nitrogenase. Three genetically distinct nitrogenase systems exist in Azotobacter vinelandii (A. vinelandii): Mo-containing nitrogenase, V-containing one and “Fe only” nitro-genase[1―4]. They are composed of two separable com-ponent proteins. For example, conventional Mo-con- taining nitrogenase is composed of component I (MoFe protein) and com…     

A new measure to characterize multifractality of sleep electroencephalogram

Traditional methods for nonlinear dy-namic analysis,such as correlation dimension,Lyapunov exponent,approximate entropy,detrended fluctuation analysis,using a single parameter,cannot fully describe the extremely sophisticated behavior of electroencephalogram (EEG). The multifractal for-malism reveals more “hidden” information of EEG by using singularity spectrum to characterize its nonlin-ear dynamics. In this paper,the zero-crossing time intervals of sleep EEG were studied using multifractal analysis. A new multifractal measure Δasα was pro-posed to describe the asymmetry of singularity spec-trum,and compared with the singularity strength range Δα that was normally used as a degree indi-cator of multifractality. One-way analysis of variance and multiple comparison tests showed that the new measure we proposed gave better discrimination of sleep stages,especially in the discrimination be-tween sleep and awake,and between sleep stages 3 and 4.     

Effects of specific surface area of metallic nickel particles on carbon deposition kinetics

Carbon deposition on nickel powders in methane involves three stages in different reaction temperature ranges. Temperature programing oxidation test and Raman spectrum results indicated the formation of complex and ordered carbon structures at high deposition temperatures. The values of I(D)/I(G) of the deposited carbon reached 1.86, 1.30, and 1.22 in the first, second, and third stages, respectively. The structure of carbon in the second stage was similar to that in the third stage. Carbon deposited in the first stage rarely contained homogeneous pyrolytic deposit layers. A kinetic model was developed to analyze the carbon deposition behavior in the first stage. The rate-determining step of the first stage is supposed to be interfacial reaction. Based on the investigation of carbon deposition kinetics on nickel powders from different resources, carbon deposition rate is suggested to have a linear relation with the square of specific surface area of nickel particles.     

我国石油工业可持续发展的探讨

针对世界石油峰值及我国油气供需预测,结合我国实际情况,提出以立足国内为主、加强国内油气资源的勘探开发、构建节约型社会、实现能源发展的多元化战略,以及开拓海外油气资源、建立石油储备体系等对策建议。     

好氧颗粒污泥对水中橘黄的吸附特性

利用好氧颗粒污泥(AGS)对碱性染料橘黄(SY)进行吸附试验,研究了不同p H值、吸附剂用量、SY初始浓度和温度对吸附过程的影响.发现:溶液的p H值是影响吸附效果的一个重要因素,p H值为2、AGS用量为2 g/L和温度为35℃时吸附效果最好;平衡吸附量与SY染料初始浓度呈正相关;Langmuir吸附模型能够较好地描述整个吸附过程,饱和吸附量为142.86 mg/L,吸附动力学符合准二级动力学模型.热力学分析表明吸附是一个自发的吸热过程,且低浓度比高浓度时的吸附亲合力好.实验结果表明AGS可以作为吸附SY染料的低成本吸附剂.     

基于改进布谷鸟算法结合电导增量法的最大功率点追踪

动态遮阴下,光伏阵列的输出P-U曲线会出现多个功率极值点,传统最大功率点追踪会陷入局部最优。为此,本文提出基于自适应差分进化的改进布谷鸟(ICS)算法与电导增量法(INC)相结合的复合算法(ICS-INC)。该算法提出自适应抛弃概率和自适应步长因子,结合差分变异进行随机偏好游走,使算法的搜索开发能力得到提升,避免陷入局部最优。通过改进Lévy飞行公式减小其随机性,减小算法的迭代次数来缩短跟踪时间,由INC实现局部快速搜索,稳定输出最大功率。仿真结果表明,与其他算法相比,该算法的追踪速度,全局搜索性以及环境变化的适应能力均得到提升。     

基于神经网络的容错控制在CSTR对象中的应用

将扩展卡尔曼滤波用于RBF网络的权值更新,使该网络能满足动态建模的要求,不仅很好地逼近正常工况下的对象,也能及时有效地重构故障工况模型。基于Lyapunov稳定性推导得到的PID参数自整定算法,保证了基于RBF网络的PID控制算法使跟踪误差收敛。在CSTR系统中,仿真实例说明该方法用于对象元部件故障的检测是有效的。     

适于IP设计的定点DSP软件开发系统

描述了一种本实验室开发的适合于IP(IntellectualProperty)设计的DSP(DigitalSignalProcess)处理器核WDSP(以主要开发者姓Wu命名Wu′sDSP)的软件开发系统。这一开发系统将使根据不同DSP应用产生不同DSP处理器核成为可能。此外,WDSP还将作为一个核心部件应用于本实验室正在开发的称为FDP(FPGAforDataPath)的FPGA(FieldProgrammableGateArrays)系统中,以适应当前普遍采用的IP和SoC(SystemonChip)设计方法。     

低红移活动星系核中大质量黑洞与核球质量关系研究

采用活动星系核图像的核球/盘分解数据得到核球R波段光度值,计算了一个X射线活动星系核样本的中心大质量黑洞质量与核球质量之比(Mbh/Mbulge),其中包括15个窄线塞弗特1星系(NLS1 s)和18个宽线塞弗特1星系(BLS1 s).我们发现log(Mbh/Mbulge)的平均值,对15个窄线塞弗特1星系为:-3.81±0.11;而对18个宽线塞弗特1星系,则为:-2.91±0.13.这表明:窄线塞弗特1星系相对于宽线塞弗特1星系而言有较低的Mbh/Mbulge.