不同产地亚麻籽矿物质元素及脂肪酸组成的主成分分析

亚麻籽是一种具有食用与药用价值的生物质,富含多种营养物质与矿物质元素。我国是亚麻籽的主要产地之一,为探讨不同产地亚麻籽中矿物质元素与脂肪酸组成的主要特征成分,采用电感耦合等离子体质谱法(ICP-MS)分析了10个产地亚麻籽中的17种矿物质元素,利用气相色谱-质谱联用法(GC-MS)分析了于相同条件下提取的10个产地亚麻籽油脂中的脂肪酸组成。采用主成分分析法对10个产地亚麻籽中的矿物质元素及脂肪酸组成进行了分析,探讨了不同产地亚麻籽矿物质元素及脂肪酸组成的差异,分析了矿物质元素及脂肪酸的主要特征成分。结果表明,K,Sr,Mg,Ni,Co,Cr,Cd,Se,Zn和Cu是亚麻籽的主要特征矿物质元素,C16∶0,C18∶0,C18∶2,C18∶3,C20∶0,C20∶1是亚麻籽油脂的主要特征脂肪酸。ICP-MS和GC-MS结合主成分分析,可有效揭示不同产地亚麻籽中矿物质元素与脂肪酸组成的特征与差异,进而为亚麻籽的合理、有效利用提供重要的理论依据。     

非晶InGaZnO薄膜晶体管驱动OLED像素电路的仿真研究

为解决非晶InGaZnO薄膜晶体管(a-IGZO TFT)因其阈值电压漂移而导致的OLED电流衰减的问题,本文研究了基于a-IGZO TFT的有源矩阵有机发光显示(AMOLED)像素电路的阈值电压补偿问题。利用实验室制备的a-IGZO TFT器件进行参数提取后建立的SPICE仿真模型并进行仿真计算,对电压驱动型2T1C和4T1C的像素电路进行稳定性的比较研究,证明了4T1C电路对阈值漂移有非常好的补偿效果,并指出增加存储电容值和驱动TFT的宽长比可有效提高OLED电流的保持能力。     

A tunable infrared plasmonic polarization filter with asymmetrical cross resonator

A tunable infrared plasmonic polarization filter is proposed and investigated in this paper. The filter is based on the sandwich absorption structure which consists of three layers. The top layer is an array of asymmetrical cross resonator.The middle and bottom layers are dielectric spacer and metal film respectively. By absorbing specific wavelength of the incident light perfectly, the reflection spectrum of the structure shows filter performance. The calculated results show that the absorption wavelength is strongly dependent on the length of branch of the asymmetrical cross resonator which is parallel to the light polarization and independent of the length of the vertical one. Therefore, the asymmetrical cross resonator filter structure opens the way for freely tuning the filtering wavelength for a different light polarization. We can fix a resonant wavelength(absorption wavelength) corresponding to one polarization and change the resonant wavelength for the other polarization by adjusting the corresponding branch length of the asymmetrical cross resonator, or change the two resonant wavelengths of both two polarizations at the same time.     

Remote excitation and remote detection of a single quantum dot using propagating surface plasmons on silver nanowire

Using propagating surface plasmons(SPs) on a silver nanowire(NW), we demonstrate that a focused laser light at the end of the silver NW can excite a single quantum dot(QD) microns away from the excitation spot. The QD–NW interaction allows the excited QD convert part of its energy into propagating SPs, which then can be detected at remote sites.Simultaneous multi-QD remote excitation and remote detection can also be realized. Furthermore, the tight confinement of the propagating SPs around the NW surface enables the selective excitation of QDs very close in space, which cannot be realized under the conventional excitation condition. This remote excitation and remote detection approach may find applications in optical imaging and the sensing of chemical and biological systems.     

基于光谱响应差异的HJ-1B热红外通道星上定标系数验证

HJ-1B卫星热红外通道自发射以来共进行了7次星上黑体定标,然而针对星上定标系数的验证工作开展较少。通过半高宽法、矩方法和查找表法计算得到2009年9月14日星上定标系数。以具有较高定标精度的MODIS为参考源,基于MODIS第31,32通道和HJ-1B热红外通道的光谱响应特性,改进对应热红外通道的光谱匹配算法,建立两传感器表观辐亮度的匹配关系,进而通过Planck公式计算出HJ-1B热红外通道的等效水表亮温,通过与HJ-1B热红外通道基于星上定标系数得到的反演水表亮温进行比较,实现对星上定标系数的验证。以光谱响应差异计算的等效亮温值为285.97 K,半高宽法、矩方法和查找表法星上定标系数反演亮温值分别为288.77,274.52和285.97 K。结果显示,半高宽法、矩方法和查找表法星上定标系数反演亮温与光谱响应差异计算的等效亮温偏差分别为2.8,-11.46和0.02 K。结果表明,HJ-1B热红外通道星上定标方法中以查找表法星上定标系数计算结果精度较高。同时证明了基于光谱响应差异的HJ-1B热红外通道星上定标系数验证方法有效可行。     

Hadronic Scenarios for Gamma-Ray Emission from Three Supernova Remnants Interacting with Molecular Clouds

GeV γ-rays detected with the large area telescope on board the Fermi Gamma-ray space telescope in the direc- tion of HB21, MSH 17-39 and G337.0-0.1 have been recently reported. The three supernova remnants （SNRs） show interactions with molecular clouds, and they are effective gamma-ray emitters as the relativistic protons accelerated by the SNR shocks inelastically colliding with the dense gas in the clouds. The origin of the observed γ-rays for the three remnants is investigated in the scenario of the diffusive shock acceleration. In the model, a part of the SNR shock transmits into the nearby molecular clouds, and the shock velocity is greatly reduced. As a result, a shock with a relatively low Alfven Mach number is generated, and the spectra of the accelerated protons and thee＇γ-ray photons produced via proton-proton interaction can be obtained. The results show that the observed γ-ray spectra for the three SNRs interacting with the molecular clouds can be reproduced. It can be concluded that the hadronic origin of the γ-rays for the three SNRs is approved, and the ability of SNR shocks to accelerate protons is also supported.     

Stochastic resonance in a single-mode laser driven by quadratic pump noise and amplitude-modulated signal

This paper investigates the phenomenon of stochastic resonance in a single-mode laser driven by quadratic pump noise and amplitude-modulated signal. A new linear approximation approach is advanced to calculate the signal-to-noise ratio. In the linear approximation only the drift term is linearized, the multiplicative noise term is unchangeable. It is found that there appears not only the standard form of stochastic resonance but also the broad sense of stochastic resonance, especially stochastic multiresonance appears in the curve of signal-to-noise ratio as a function of coupling strength λ between the real and imaginary parts of the pump noise.     

Controlled growth and field emission of vertically aligned AlN nanostructures with different morphologies

The controllable growth of three different morphologies of AlN nanostructures (nanorod, nanotip and nanocrater) arrays are successfully realized by using chemical vapour deposition (CVD) technology. All three nanostructures are of single crystal h-AlN with a growth orientation of [001]. Their growth is attributed to the vapour-liquid-solid (VLS) mechanism. To investigate the factors affecting field emission (FE) properties of AlN nanostructures, we compare their FE behaviours in several aspects. Experimental results show that AlN nanocrater arrays possess the best FE properties, such as a threshold field of 7.2~V/μm and an emission current fluctuation lower than 4%. Moreover, the three AlN nanostructures all have good field emission properties compared with a number of other excellent cathode nanomaterials, which suggests that they are future promising FE nanomaterials.     

制备工艺对Zn1-xMgxO薄膜结构及光学性能的影响

采用脉冲激光沉积（PLD）方法在单晶Si（100）衬底上沿c轴方向生长单晶Zn_1-xMg_xO薄膜,通过X射线衍射（XRD）、原子力显微镜（AFM）、扫描电镜（SEM）和荧光光谱（PL）研究了膜厚、Mg含量、退火温度及氧气氛等制备工艺对Zn_1-xMg_xO薄膜的结构、形貌和光学性质的影响.实验结果表明,Mg含量x≤0.15时, Zn_{关键词： 1-x}Mg_xO薄膜')" href="#">Zn_1-xMg_xO薄膜 制备工艺 结构 光学性质     

立方铂纳米粒子的形状变化与熔化特性的分子动力学研究

采用分子动力学方法结合嵌入原子多体势,对立方铂纳米粒子的热稳定性进行了模拟研究.计算结果表明,立方纳米粒子在升温过程中首先转变为由{111}和{100}面所构成的十四面体,然后再转变为球形,最后熔化为液态.通过计算立方铂钠米粒子的统计半径,发现形状转变温度在1250 K左右.尽管形状不同,立方纳米粒子和球形纳米粒子的熔点是相同的. 关键词： 纳米粒子 热稳定性 分子动力学