Synthesis and Crystal Structure of N,N′,N″- Tris-（2-aminophenyltriphenylphosphium）- benzene- 1,3,5-tricarboxamide

A new tripodal P,N ligand （C63H48N3O3P3） was prepared and characterized by elemental analysis, IR and single-crystal X-ray diffraction. The crystal belongs to the monoclinic system, space group P21/c with a = 13.013（3）, b = 28.406（6）, c = 14.911（3） A^°, β= 111.04（3）°, V= 5144.6（18） A^°^3 Z = 4, Dc = 1.276 g/cm^3, Mr = 987.95, λ（MoKa） = 0.71073 A^°,μ = 0.17 mm^-1, F（000） = 2064, R = 0.0786 and wR = 0.1545. A total of 43260 unique reflections were collected, of which 5112 with I 〉 2σ（I） were observed. The title compound has a central benzene ring, which is linked by -NH-CO- bonds to three 2-aminophenyltriphenylphosphium moieties, of which two with P（1） and P（2） centers are pointing to the same face of the central aryl ring, while the third one directs oppositely, forming a pseudo-propeller. In the crystal structure, there exist face-to-face π-π stacking interactions which increase the stability of the crystal structure.     

高分子光伏材料聚对苯乙烯撑-喹喔啉共聚物的合成与光学性能研究

高分子光伏材料聚对苯撑乙烯撑(PPV)由于低廉的价格, 容易加工的性能与可调的光学性能, 有可能成为新一代太阳能材料. 然而PPV较宽的带隙阻碍了PPV太阳能电池效率进一步提高. 合成了一种较低带隙的新型高分子光伏材料 PPV-PQ. 用NMR, FT-IR, 元素分析, GPC和TGA与循环伏安法对PPV-PQ进行了结构表征与性能检测, 并对它在氯仿溶液与固态薄膜下的紫外-可见吸收与荧光发射光谱进行了研究. 结果显示, 由于在固态下存在较强的分子间作用, 分子链的共平面性增加, 所以PPV-PQ无论是紫外-可见吸收, 还是荧光发射光谱, 在固态薄膜下都比在氯仿溶液里发生明显红移. 即使在浓溶液中, 分子链间也存在较强的作用力, 使得PPV-PQ荧光发射峰随溶液浓度的增加而发生红移. 紫外-可见光谱显示, PPV-PQ由于大体积的吸电子单元引起了较大的空间位阻, 最大吸收峰比PPV稍微蓝移, 但吸收却比PPV向长波延展, 带隙比PPV低, 只有1.92 eV. 循环伏安法结果表明PPV-PQ与PCBM两者的LUMO之间有足够的能量差异, 加上PPV-PQ与富勒烯衍生物C117共混物薄膜发生荧光猝灭, 都说明PPV-PQ上光激发电子能够转移到富勒烯衍生物上. 因此, PPV-PQ可以用作高分子光伏材料.     

张丝式电工仪表直读误差的建议

根据国家标准《电气测量指示仪表通用技术条例》规定,按最大引用误差的不同,仪表准确度分为0.1、0.2、0.5、1.0、1.5、2.5、5等七个等级.例如0.5级的仪表,它的读数误差在整个量限范围内都是满量限的±0.5%.因此各处的绝对误差是相同的.用这种方法来确定直读误差,对于轴承式仪表是合理的. 例如对于轴承式磁电式仪表,在测量机构的动圈中有电流通过时就产生电磁转矩M1,使动圈得以偏转.同时游丝产生一个与偏转角度α成正比的反作用力矩Mα,在平衡状态下有M1=M2,此时指针应停留在如图1所示的A点. 由于轴尖与轴承之间必然存在摩擦,它导致产生一…     

铁-过氧化氢-变色酸催化动力学光度法测定痕量铁

本文研究了在H3PO4介质中，痕量铁（Ⅲ）催化过氧化氢氧化变色酸的褪色指示反应及最佳实验条件条件和动力学参数，建立了测定痕量铁的新方法。方法的灵敏度为6．18×109g／L；测定范围0～30μg／L。用于各种水平痕量铁的测定获得满意结果。     

钡铁氧体纳米复合材料的制备及其微波吸收性能

采用聚乙二醇(PEG)凝胶法制备了Ba(Zn1－xCox)2Fe16O27复合氧化物纳米材料，用X射线衍射分析对产物进行了表征.将制得的材料与传统的微波吸收剂铁粉结合起来，制成双层复合的吸波涂层，进行测试.实验结果表明，所制材料对微波具有良好的吸收性能.并进一步对纳米复合材料的吸波机理进行了探讨.     

稀土元素的电分析化学研究 Ⅹ.钆-茜素红的极谱配合吸附波的研究

在pH=9.6的0.1MNH_3-NH_4Cl和2×10~(-4)M茜素红溶液中,用单扫示波极谱法可得到钆-茜素红配合物的波,峰电位在-0.69V处。其导数波峰高与钆在1×10~(-7)～6×10~(-6)M范围内的浓度有线性关系,最低检出限6×10~(-8)M。研究确定该波为1∶3钆-茜素红配合物的吸附波。配合物中茜素红经电极反应由醌型还原为氢醌型。     

Flexible Cu（In,Ga）Se2 Thin-Film Solar Cells on Polyimide Substrate by Low-Temperature Deposition Process

The electrical and structural properties of polycrystalline Cu（In, Ga）Se2 films grown on polyimide （PI） substrates below 400℃ via one-stage and three-stage co-evaporation process have been investigated by x-ray diffraction spectra （XRD）, scanning electron microscopy （SEM） and Hall effect measurement. As shown by XRD spectra, the stoichiometric CIGS films obtained by one-stage process exhibit the characteristic diffraction peaks of the （In0.68Ga0.32）2Se3 and Cu（In0.7Ga0.3）2Se. It is also found that the film structures indicate more columnar and compact than the three-stage process films from SEM images. The stoichiometric CIGS films obtained by three-stage process exhibit the coexistence of the secondary phase of （In0.68Ga0.32）2Se3, Cu2-xSe and Cu（In0.7Ga0.3）2Se. High net carrier concentration and sheet conductivity are also observed for this kind of film, related to the presence of Cu2-xSe phase. As a result, when the CIGS film growth temperature is below 400℃, the three-stage process is inefficient for solar cells. By using the one-stage co-evaporation process, the flexible CIGS solar cell on a PI substrate with the best conversion efficiency of 6.38% is demonstrated （active area 0.16cm^2）.     

弹性波散射与多重散射的T矩阵方法

研究弹性波散射与多重散射的T矩阵方法。首先,基于Helmholtz体内和体外公式推导了对应于圆柱型散射体的T矩阵元素的具体表达式;接着分析了在含多个随机分布圆柱型散射体的随机非均匀介质中弹性波的多重散射并给出在统计平均意义下的相干波的定义以及波速和衰减系数计算公式;最后,针对Ge/Al、Sic/Al复合材料用Matlab进行了编程和数值计算;计算单个柱型散射体的散射截面以及随机非均匀介质中相干波的速度和衰减系数,分析了这种介质的频散特性。     

GAMMA-RAY LIGHT CURVE AND PHASE-RESOLVED SPECTRA FROM GEMINGA PULSAR

We calculate the light curve and phase-resolved spectra of Geminga in a three-dimensional pulsar magnetosphere model. The light curve of gamma-rays is consistent with that observed if the magnetic inclination and viewing angle are ～50° and ～86° respectively. We also model the phase-resolved spectra of the Geminga pulsar.     

有机硅聚丙烯酸酯微乳液的合成与性能

有机硅聚丙烯酸酯微乳液的合成与性能;硅氧烷