中国散裂中子源快循环同步加速器主准直器的设计与研究

为满足强流加速器对准直器高散热性能、高抗辐射性能、超高真空、高定位精度、高稳定性和在线实时调整等特殊要求,在CSNS/RCS主准直器设计时针对结构方案和控制方案进行了详细设计和研究,针对关键部件:刮束器、真空盒、驱动装置和远程快速拆卸装置等设计难点进行了阐述,在设计中使用ANSYS完成了刮束器的热分析及支架强度和变形校核,用FLUKA程序对辐射屏蔽进行了分析和设计,确保主准直器设计的可靠性。     

红外双谱段傅里叶变换成像光谱仪光学设计

提出了一种基于静态干涉系统的中长波红外双谱段时空联合调制傅里叶变换成像光谱仪(FTIS),分别对前置望远系统及后置成像系统进行了设计。根据像差理论,通过添加约束的方式计算了反射式前置望远系统的初始结构,通过光学设计软件优化,矫正了系统中倾斜分束器和补偿器带来的大数量级像散和彗差;在中波和长波双谱段范围内,前置系统的调制传递函数(MTF)均接近衍射极限。该光谱仪的两个后置成像系统均采用透射式结构,点列图结果显示,后置系统成像像斑均方根(RMS)值在双谱段范围均小于7.0μm。将前置望远系统和后置成像系统进行对接,最终得到了视场角为1.5°,中波通道F数为4,长波通道F数为2的整体光学系统。在双谱段范围内,整体系统的点列图RMS值小于10.7μm,MTF在探测器的特征频率17lp/mm处大于0.5,具有良好的成像效果。     

不同比例的MEH-PPV与PCBM共混体系光电池性能研究

以MEH-PPV(poly(2-methoxy-5-(2^/-ethylhexoxy)-1,4-phenylene vinylene)为电子给体材料(donor,D), PCBM(1-(3-methoxycarbonyl)-propyl-1-1-phenyl-(6,6)C₆₁)为电子受体材料(acceptor,A),制成了不同比例的共混体系太阳电池.从不同比例的D/A材料共混体系的原子力图、光荧光谱、器件的单电荷传输的暗导J-V图、太阳电池的光敏图及器件双电荷传输的光、暗导J-V图方面,详细分析了不同比例的D/A材料对器件性能影响.得出了当D/A材料比例为1∶4时,器件中活性层能形成良好的互穿网络,光生激子能有效地分离,被分离的电荷能有效地传输,太阳电池的性能最好.其光电池在100mW/cm²强度光照下,其开路电压V_oc为0.8V,短路电流密度J_sc为3.47mA/cm²,填充因子FF为55.9%,能量转换效率η为1.55%. 关键词： 太阳能电池 聚合物 性能     

藻蓝蛋白(C-Pc)的三阶光学非线性和激发态弛豫

藻蓝蛋白（Ｃ－Ｐｃ）的三阶光学非线性和激发态弛豫＊刘志斌彭俊彪ａ）李文连（中国科学院长春物理研究所，长春１３００２１）ａ）（中国科学院激发态物理开放研究实验室，长春１３００２１）邓湘君（吉林省生物研究所，长春１３００１２）关键词藻蓝蛋白，χ（３）值，...     

New robust chaotic system with exponential quadratic term

This paper proposes a new robust chaotic system of three-dimensional quadratic autonomous ordinary differential equations by introducing an exponential quadratic term. This system can display a double-scroll chaotic attractor with only two equilibria, and can be found to be robust chaotic in a very wide parameter domain with positive maximum Lyapunov exponent. Some basic dynamical properties and chaotic behaviour of novel attractor are studied. By numerical simulation, this paper verifies that the three-dimensional system can also evolve into periodic and chaotic behaviours by a constant controller.     

激光陀螺光电探测器光窗的设计

用平面波计算拍频条纹间距时,因激光器中存在衍射效应,且实际光强分布为高斯型,故给光电探测器光窗尺寸计算带来很大误差(40%),导致系统不能正常工作。为此,以高斯光束为基础,利用光电探测器测得2路信号的相位差,通过数值计算得到2束光拍频条纹间距,由此计算得到理想相位差光电探测器的尺寸。最后,用实验验证了该设计方法的可行性,为RLG光电探测器光窗尺寸的设计提供了一种简单准确的方法。     

Light scattering of nanocrystalline TiO2 film used in dye-sensitized solar cells

This paper studies the light scattering and adsorption of nanocrystalline TiO2 porous films used in dye-sensitized solar cells composed of anatase and/or rutile particles by using an optical four-flux radiative transfer model. These light properties are difficult to measure directly on the functioning solar cells and they can not be calculated easily from the first-principle computational or quantitative theoretical evaluations. These simulation results indicate that the light scattering of 1 25 nm TiO2 particles is negligible, but it is effective in the range of 80 and 180 nm. A suitable mixture of small particles （10 nm radius）, which are resulted in a large effective surface, and of larger particles （150 nm radius）, which are effective light scatterers, have the potential to enhance solar absorption significantly. The futile crystals have a larger refractive index and thus the light harvest of the mixtures of such larger rutile and relatively small anatase particles is improved in comparison with that of pure anatase films. The light absorption of the 10μm double-layered films is also examined. A maximal light absorption of double-layered film is gotten when the thickness of the first layer of 10 urn-sized anatase particles is comparable to that of the second larger rutile layer.     

测量气体分子平均速率的一种简易方法

用一种简易的方法测量了常温下气体分子运动的平均速率.根据易挥发性液体的质量随时间逐渐减少的特点和盛放液体的容器加盖前后挥发的气体分子对容器作用力的变化,通过分析天平测量液体质量的改变得到挥发出来的气体分子对容器的作用力,利用变质量物体的动量守恒定理,测量得到了易挥发性气体分子的平均速率,实验结果较好地与理论值符合.     

非线性一维光子晶体波导光双稳

利用非线性折射率系数较大且非线性时间响应较快的CdS_xSe_1-x玻璃为材料,设计并制备了非线性一维光子晶体波导光双稳器件,该器件的折射率空间分布呈正弦形式。实验测得双稳开关的阈值功率密度为1.60×10⁵W/cm²,开关时间为63ps。采用时域有限差分方法讨论了光子晶体带隙随入射光强变化而移动的情况,随着入射光功率密度的增加,光子晶体的带隙中心向短波方向移动。同时计算了该器件的双稳特性,理论计算得到双稳开关的阈值功率密度为1.40×10⁵W/cm²,开关时间约为50ps。获得了理论与实验基本一致的结果。     

A novel 2-dimensional cosmic ray position detector based on a CsI(Na) pixel array and an ICCD camera

A novel 2-D cosmic ray position detector has been built and studied. It is integrated from a CsI(Na) crystal pixel array, an optical fiber array, an image intensifier and an ICCD camera. The 2-D positions of one cosmic ray track is determined by the location of a fired CsI(Na) pixel. The scintillation light of these 1.0× 1.0 mm CsI(Na) pixels is delivered to the image intensifier through fibers. The light information is recorded in the ICCD camera in the form of images, from which the 2-D positions can be reconstructed. The background noise and cosmic ray images have been studied. The study shows that the cosmic ray detection efficiency can reach up to 11.4%, while the false accept rate is less than 1%.