图像平场校正方法的扩展应用研究

对于图像阵列探测器而言,由于各像元响应的不一致使得所获图像中各像元灰度存在差异（响应的非均性现象）,而图像的平场校正可以非常有效地消除图像中各像元响应的不一致性.如果将图像背景或光路中影响成像的一些因素在一定程度上看作是图像探测器的响应,认为它是响应非均匀的组成部分,根据平场校正的原理对其进行处理,则可以获得较好的效果.     

Ga1-xAlxAs/GaAs光阴极光谱响应向短波延伸的机理分析和实验研究

为了实现光阴极光谱响应向短波延伸，分析了Ga1-xAlxAs/GaAs三代微光光阴极光谱响应向短波延伸的机理，提出了准禁带宽度的概念，讨论了Ga1-xAlxAs的禁带宽度随铝组份x值的增加而逐渐变宽的变化规律，计算了不同铝组份下光阴极光谱响应的短波限。通过提高光阴极材料的铝组份，做出了宽光谱响应像管，并给出了相应的光谱响应曲线。通过与标准三代微光像管光谱响应对比，发现：所得光谱响应曲线不仅向短波方向得以延伸，而且理论设计与实验结果吻合很好。     

Research on calibration method in lab of direct solar channels of Sun photometer

We develop a new calibration method in lab by measuring the absolute spectral irradiance responsivity of Sun photometer sun channel. The absolute power responsivity of Sun photometer is obtained when a white laser double monochromator system serve as a source, and a standard transfer detector calibrated against cryogenic absolute radiometer is assembled to measure the absolute power of laser beam. The effective area of aperture is measured through laser raster scanning method, and the relative spectral irradiance responsivity of the corresponding channel is obtained by using tungsten-halogen lamps double monoehromator system. On the basis of the above results, the top of the atmosphere responsive constants V0 （500, 675, and 870 nm） are obtained by integration with extraterrestrial solar spectral irradiance data. Comparing the calibration results with that of CIMEL, France in November 2011, the relative differences are 4.38%, 2.23%, and 2.45%, respectively. The calibration uncertainty reaches to 2.048×10^-2, which shows a remarkable consistency with the Langley plot method. Further, our scheme can overcome the limits of space and atmospheric conditions which are only available at a high-altitude calibration site in particular date. The advantages lie in not only shortening the experiment period but also being of high precision. This new scheme definitely plays an important role in supporting the current and future sun photometry calibration activities which are significant to earth observation.     

气体开关抖动对单模块快脉冲直线型变压器驱动源输出特性的影响

分析了快脉冲直线型变压器驱动源(FLTD)气体开关触发击穿延时的分布规律,利用MAT-LAB软件生成随机序列模拟开关击穿延时和抖动,在FLTD简化二阶电路的基础上,利用MATLAB分析了开关抖动对40个支路并联1 MA,100 ns FLTD模块输出电流脉冲前沿和幅值的影响。模拟计算结果表明:开关理想时,即抖动为0,输出电流峰值为996 kA,峰值时间为90 ns,10%~90%脉冲前沿为54 ns;开关自身抖动与开关之间分散性之和为10 ns时,输出电流脉冲前沿增加约14%,电流峰值下降约2%;开关自身抖动与开关之间分散性之和为20 ns时,输出电流脉冲前沿增加约38%,电流峰值下降约5%。     

响应曲面法提取水松总黄酮的工艺研究

采用响应曲面法,优化了提取水松总黄酮的提取工艺条件为:微波时间3.8min,乙醇浓度69%,固液比1∶31,在此条件下,水松总黄酮的产率为1.88%。     

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。     

Changes in Repetitive Firing Rate Related to Phase Response Curves for Andronov-Hopf Bifurcations

We study specific changes in repetitive firing in the two-dimensional Hindmarsh-Rose （2dHR） oscillatory sys- tem that undergoes a bifurcation transition from the supercritical Andronov-Hopf （All） type to the subcritical Andronov-Hopf （SAH） type. We identify dynamical mechanisms which are responsible for changes of the repeti- tive firing rate during the AH to SAH bifurcation transitions. These include frequency-shift functions in response to small perturbations of a timescale parameter, its multiplicative parameter, and an external input current in the 2dHR oscillatory system. The frequency-shift functions are explicitly represented as functions relating to the phase response curves （PRCs）. Then, we demonstrate that when the timescale is normal and relatively fast, the repetitive firing rate slightly increases and decreases respectively during the AH to SAH bifurcation transition with a change of the intrinsic parameter, whereas it decreases during the SAH to AH bifurcation transition with an increase in the timescale. By analyzing the three different frequency-shift functions, we show that such changes of the repetitive firing rate depend largely on changes of the PRC size. The PRC size for the SAH bifurcation shrinks to the PRC size for the AH bifurcation.     

基于光谱响应定标的辐射测温方法

辐射测温是通过测量物体发出的辐射来反演温度,辐射测量方程中含有与空间位置相关的非光谱参数,通常需通过辐射标定予以确认。而该研究将非光谱参数归入有限项级数形式的光谱发射率中,这既不会影响多通道测温方程组的封闭性,又不会影响真温求解,从而在无需测量数据归一化的条件下,实现了无需空间位置标定的辐射测温,该方法仅需要标定仪器的绝对光谱响应或相对光谱响应,但不能解得发射率。以两个特例分别对多波长测温方法和多谱段测温方法的求解特性进行了研究。结果表明：对于任意的测量矢量,有效波长不相同的多波长测温唯一解是存在的;而多谱段测温时,存在无解区域,双解直线,甚至可能存在三解直线。     

Hg2CuTi型Mn2NiGe合金的电子结构、磁性对压力、四方变形的响应

运用基于密度泛函理论的第一性原理方法,研究了Hg2CuTi型 Mn2NiGe合金的电子结构对外加压力的响应以及Mn2NiGe的电子结构、磁性对四方变形的响应．结果表明：i）随着外加压力的增加,因Ni、Mn原子间距的减小而导致杂化程度的增强,使得态密度整体向低能区域移动,同时,态密度幅度整体略有减小;ii）在由奥氏体相到马氏体相的变形中,同样因Ni、Mn原子间距的减小而导致杂化程度的增强,占据态的态密度向低能区域移动,体系的能量降低,同时,成键态向低能方向移动,反键态向高能方向移动,能带变宽,成键作用加强,最终导致在马氏体相中的稳定性增大;iii）在四方变形过程中,Mn2NiGe总磁矩的变化主要由Ni原子磁矩的变化所产生．     

量子材料中的超快光谱学

亚皮秒激光脉冲能够选择性地激发强关联体系中的激发模式,操控材料从一个有序态进入另外的有序态． “量子材料的超快光谱学”,这仅仅是个老生常谈,还是一个可以促进设计和发现新材料的全新领域？本文列举的一些最新的进展都指向了后者．表面上,超快激光和量子材料是两个在特征和文化上有很大差别的领域,因为量子材料的传统实验是在屏蔽和寂静的低温实验室进行,而激光实验室则会让人联想起视频游戏厅．