高分辨大视场紫外-可见光偏振成像融合处理技术

采用蒙特卡罗方法对水云下大气的偏振态分布进行了仿真分析,所建立的水云大气环境在紫外360～400 nm波段的偏振度响应最大。采用紫外-可见光偏振成像技术对同一视场下的楼房、云和天空进行了偏振成像实验,并用霍夫变换分割方法对图像中的每个区域进行了统计分析,发现观测区域内无云区与云区的偏振角均值相对差为1.6%,偏振度均值相对差为-14%,证明了大气偏振角较偏振度稳健。紫外光和可见光在对云目标的偏振观测中存在互补性,采用拉普拉斯金字塔图像融合技术能够提高对大气目标的探测能力,验证了大视场高分辨紫外-可见光偏振成像技术在大气探测中的可行性和有效性。     

磁控溅射技术制备ZnO透光薄膜

采用RF磁控溅射方法,在玻璃衬底上制备了择优取向的ZnO薄膜;通过台阶仪、X射线衍射技术、原子力显微镜和分光光度计分别测量了不同溅射功率条件下淀积的ZnO薄膜厚度(淀积速率)、结晶质量、表面形貌与粗糙度、透光光谱,报道了该薄膜结晶质量、薄膜粗糙度与其在可见光区透光率的关系.     

Measurements of AIM for Visible Wavelength Based on Individual Eye Model

We measure and calculate the aerial image modulation （AIM） of human retina for visible wavelengths based on the individual eye model. By employing the optical design software ZEMAX, we obtain the modulation transfer function （MTF） of human eye in visible wavelengths. Using CSV-1000 and VAF-1000, the contrast sensitivity function （CSF） and the visual acuity （VA） for the same eye are measured. Then the AIM of human retina could be acquired by the relations between MTF and CSF and between MTF and VA. The AIM of human retina is independent of MTF, and the values of AIM for normal eyes （without retina disease） are similar, so the assembly average for large numbers of normal eyes can be a standard AIM curve, which is helpful for the diagnosis of diseases in the retina system.     

HL-1和HL-1M装置等离子体可见光谱实验

总结HL-1和HL-IM装置等离子体的可见光谱实验，给出了各种放电条件下等离子体参数的可见光谱测量结果，讨论了杂质减少、加料、约束改善、等离子体旋转及边缘辐射特性等可见光谱实验结果，展望了HL2A装置上要开展的可见光谱研究内容。     

HL-2A装置等离子体可见光成像系统

为了配合HL-2A装置的工程联调和首次等离子体放电，需要一种可靠和直观的诊断手段，以确认产生了所谓的“First plasma”(初始等离子体)放电。为此我们研制了一套新的诊断系统，即等离子体可见光成像。等离子体成像是近年来发展起来的一项先进诊断手段。目前在托卡马克装置上广泛采用。     

New BCN Fibres for Strong Ultraviolet and Visible Light Luminescence

Novel B3CN3 fibres with a special structure have been synthesized by a pyrolysis process. High-resolution TEM analysis shows that the as-prepared B3CN3 fibres can be described as a nanofibre-interweaved network. Strong photoluminescence at 370 nm and 700 nm from the as-prepared B3 CN3 fibres are observed at room temperature, which suggests that B3 CN3 is a promising ultraviolet- and visible-light-emitting material.     

WOx/TiO2光催化剂的可见光催化活性机理探讨

采用磁控溅射技术在用浸渍提拉法制得的TiO2薄膜上，溅射氧化钨层,通过气相反应中光催化降解二甲苯的实验表明，WOx/TiO2薄膜具有可见光活性.通过UV-Vis吸收光谱、X射线光电子能谱（XPS）等方法对其可见光活性的机理进行探索.UV-Vis吸收光谱表明WOx,TiO2对可见光响应的范围有一定的扩展,吸收强度增加.XPS表明WOx/TiO2薄膜表面形成了明显的W杂质能级和Ti缺陷能级,这是WOx/TiO2在可见光范围有一吸收的主要原因,也是光催化剂具有可见光活性的必要条件之一，同时杂质能级的存在使半导体费米能级上移,载流子增加,光催化效率提高.     

5''''-鸟苷酸与茜素红S的反应及其在分析化学中的作用

采用UV-Vis光谱法研究了茜素红S(ARS)与5'-鸟苷酸(5'-GMP)在pH 4.80的弱酸性缓冲溶液中生成络合物的结合反应.与试剂比较,络合物的最大吸收峰红移92 nm,测得络合物和表观摩尔吸光系数为ε＝1.3×104 L·mol-1·cm-1;最大结合数n=10;浓度线性范围0.2～16 mg/L;检出限为6.1×10-8 mol/L.研究了ARS与5'-GMP是分子间作用力的结合反应,并对时间、温度、离子强度对结合反应的影响,以及无机物、生物物质对反应体系的干扰情况进行了初步研究.     

N掺杂可见光化催化剂的研究

The N-doped, yellow colored titanium oxide photocatalysts were prepared with Ti(SO4)2 and NH4HCO3 as precursors by precipitation method. The photocatalytic ability under the irradiation of UV or visible light for the catalysts prepared was studied by degradation of styphnic acid. The materials were characterized by EDS, XRD, FTIR, UV-Vis DRS, and XPS. The results indicate that the photocatalytic ability of catalysts is improved, especially the ability of visible light response. The results of UV-Vis DRS show that the response wavelength range of N-dopped nitrogen is red shifted, the absorption region is expanded to 476 nm.