双背景法扣除溶剂水峰及蛋白质热变性的研究

研究蛋白质水溶液的红外光谱(IR)谱时,由于溶剂水的强吸收与蛋白质的吸收峰会发生严重重叠,极大地干扰对蛋白质吸收峰的识别、定性、定量和结构分析.尝试利用杂化光谱法扣除溶剂水峰.采用双背景方法,用空白ATR晶体(背景样品1)与ATR水层(背景样品2)合成了单光束杂化背景谱,通过控制对背景样品1和背景样品2的扫描次数,合成...     

高光谱成像的煤与矸石分类

煤与矸石分选是煤矿生产的必要工序,现有的人工分选与机械分选,存在效率低,易造成资源浪费以及环境污染等问题.鉴于可见/近红外高光谱成像具有分析速度快、样品无需预处理、无污染等诸多优势,旨在探讨基于可见/近红外高光谱成像对黑色背景下块状煤与矸石准确分类的可行性,并基于特征波长筛选算法简化模型,为构建多光谱煤与矸石分选系统提...     

Effective Action for Noncommutative U（1） Gauge Theory with Higher Dimensional Terms

In this paper we apply the assumption of our recent work in noncommutative scalar models to the noncommutative U（1） gauge theories. This assumption is that the noneommutative effects start to be visible continuously from a scale ANC and that below this scale the theory is a commutative one. Based on this assumption and using background field method and loop calculations, an effective action is derived for noncommutative U（1） gauge theory. It will be shown that the corresponding low energy effective theory is asymptotically free and that under this condition the noncommutative quadratic IR divergences will not appear. The effective theory contains higher dimensional terms, which become more important at high energies. These terms predict an elastic photon-photon scattering due to the noncommutativity of space. The coefficients of these higher dimensional terms also satisfy a positivity constraint indicating that in this theory the related diseases of superluminal signal propagating and bad analytic properties of S-matrix do not exist. In the last section, we will apply our method to the noncommutative extra dimension theories.     

室温下低温背景红外场景生成方法实验研究

针对高空红外场景模拟的需要,提出了模拟低温背景红外场景的新物理概念和半实物仿真实验装置.将锗单晶制作的初始透明的半导体屏放置于低温系统前端,通过控制其小于禁带宽度的局部辐射系数,在室温下(≥27℃)得到低温背景(≥-30℃)的红外场景.对液氮槽和半导体致冷器生成的冷背景的效果、辐射功率差随写入光功率的变化及低温背景和目标的温度对比度进行了实验测试.实验结果表明,液氮生成的冷背景可达-30℃,半导体致冷器为3℃;在一定范围内增大写入光的功率可以提高半导体屏的转换效率,写入光功率过高会造成辐射功率值的饱和;随着写入光功率的增加,温度对比度也大幅升高.     

基于背景运动补偿的红外目标运动分析

 介绍了基于运动补偿的红外目标运动分析方法。阐述了运动补偿的必要性、过程原理和实现方法，并用之于对红外运动目标的视频跟踪，通过用背景运动量补偿目标的相对运动量，得到明确而直观的目标运动轨迹，有效地揭示了目标运动的内在规律，为红外目标的轨迹预测与跟踪提供了更有效的分析依据。     

国际地下实验室发展综述

地下实验室是开展粒子物理学、天体物理学及宇宙学等领域一些重大基础性前沿课题的重要研究场所和良好的低本底环境,建设和发展地下实验室对于一个国家的基础科学研究具有重要科学意义.目前,国际上许多国家都已经建立起地下实验室,而中国一直没有很好的地下实验室,特别是极深地下实验室.2009年,清华大学与二滩水电开发有限责任公司开展战略合作,利用锦屏山隧道建立中国首个世界最深的地下实验室--中国锦屏地下实验室(China Jinping Underground Laboratory,CJPL),并于2010年12月12日正式启用.中国锦屏地下实验室的建成,标志着中国已经具备开展物理学重大基础前沿科学研究的自主地下实验平台,对于推动我国相关领域的重大基础前沿课题的自主研究意义重大.文章对国际上一些重要地下实验室的情况进行了介绍,并对中国锦屏地下实验室的基本情况进行了介绍.     

Study of radiation background at the north crossing point of the BEPCⅡ in collision mode

Understanding the radiation background at the north crossing point (NCP) in the tunnel of BEPCII is crucial for the performance safety of the High Purity Germanium (HPGe) detector, and in turn of great significance for long-term stable running of the energy measurement system. Therefore, as the first step, a NaI(Tl) detector is constructed to continuously measure the radiation level of photons as background for future experiments. Furthermore, gamma and neutron dosimeters are utilized to explore the radiation distribution in the vicinity of the NCP where the HPGe detector will be located. Synthesizing all obtained information, the shielding for neutron irradiation is studied based on model-dependent theoretical analysis.     

基于八叉树颜色量化和链表统计的背景主色提取方法

背景主色的确定是迷彩伪装的关键问题,针对现有提取方法的不足,提出一种基于八叉树颜色量化和链表统计的背景主色提取算法.首先对图像进行八叉树颜色量化,然后统计量化后图像的颜色,并用链表存储,最后依据人眼视觉特性和相应准则确定背景主色.该算法可以对多 幅图像进行处理且运算时间较短.实验表明这种方法能够满足迷彩伪装颜色确定的要...     

Statistical isotropy of the cosmic microwave background

The breakdown of statistical homogeneity and isotropy of cosmic perturbations is a generic feature of ultra-large scale structure of the cosmos, in particular, of non-trivial cosmic topology. The statistical isotropy (SI) of the cosmic microwave background temperature fluctuations (CMB anisotropy) is sensitive to this breakdown on the largest scales comparable to, and even beyond the cosmic horizon. We propose a set of measures,K _l (l = 1, 2,3,...) which for non-zero values indicate and quantify statistical isotropy violations in a CMB map. We numerically compute the predictedK _l spectra for CMB anisotropy in flat torus universe models. Characteristic signatures of different models in theK _l spectrum are noted.