硅基光波导芯层材料及波导分束器的制备

本文采用溶胶－凝胶法制备了具有紫外感光性的SiO2/ZrO2/H有机无机复合薄膜,利用分光式椭偏仪测得该薄膜在光纤的常用通信窗口0.85 μm、1.31 μm和1.55 μm波长附近折射率分别为1.556 9、1.548 9和1.547 2,与下包层SiO2的折射率（1.46）相比,其折射率差比δ分别为6.64％,6.09％和5.97％,可作为芯层材料用于光波导的制备.通过控制提拉速率可以制作出厚度分别为1.29,2.20,4.00,5.44和6.82 μm的SiO2/ZrO2/H芯层薄膜,以满足0,1,2,3和4阶导模的传输要求.进而利用该薄膜自身的感光特性结合紫外掩模法,制备出相应厚度的1×8Y分支光功率分配器.通光实验表明,该光功分器能够将1.53～1.56 μm波长的光限制在波导内,实现光的传输和分束功能.     

1感光溶胶-凝胶法制备光波导研究

采用溶胶-凝胶技术与化学修饰相结合的方法,制备了具有紫外感光特性的SiO2/Al2O3溶胶及其凝胶薄膜,并通过在溶胶中加入聚乙二醇使其形成有机-无机复合结构,经一次提拉制膜就可获得18 μm厚的感光性凝胶薄膜.利用薄膜自身的感光性,使紫外光通过掩模照射薄膜,再经过溶洗和200℃、1 h的热处理,就可获得厚度达到15 μm、线宽约为100 μm的波导阵列.对这种波导薄膜的折射率和的透射率进行了研究.     

溶胶-凝胶法制备SiO2-TiO2平板光波导工艺研究

采用溶胶-凝胶法制备了SiO₂-TiO₂平板光波导,计算了平板光波导通光条件,分析了硅/钛溶胶-凝胶材料的热性能,观测了平板光波导的结构形貌,并测试了其通光损耗。结果表明：经过200℃,30 min干燥处理的凝胶薄膜呈疏松多孔状态,对于非对称平板波导,存在芯层通光截止厚度,而且当SiO₂-TiO₂芯层厚度为0.5 μm时,SiO₂下包层厚度至少有6 μm才能防止1550 nm波长光泄露入单晶硅衬底中。制备的光波导对于1550 nm波长光传输损耗最小值为0.34 dB/cm。     

火焰水解法制备Si02—Ge02平面波导材料

本文采用火焰水解法（FHD）在单晶Si片上快速淀积SiO2/SiO2-GcO2厚膜，再经过高温玻璃化处理，获得了玻璃态的平面波导材料。下包层SiO2膜的厚度约为40μm，波长1550nm处的折射率为1.4462，芯层SiO2-GeO2膜的厚度为5μm，折射率为1.4631。分别采用XRD、XPS、SEM和椭偏仪等对波导材料表面特性和折射率等进行了测试分析。     

聚硅氧烷改性及多模光波导制备

采用含氢聚硅氧烷(HPSO)和二乙烯基苯(DVB)的交联体掺入聚二甲基硅氧烷(PDMS)中,使改性的聚二甲基硅氧烷(M-PDMS)折射率发生1%～1.8%的改变。M-PDMS及PDMS薄膜具有良好的光透射率和低的传输损耗,是低成本制备用于高速芯片间光互连聚合物光波导的理想材料。采用软成型和图案转移法,用M-PDMS及PDMS分别作波导的芯层和包层制备了截面为50μm×50μm,长度大于20cm的聚硅氧烷多模光波导。用数字化散射法测量了所制备波导的传输损耗,测得输入光波长为633nm时平均传输损耗为0.137dB/cm。     

对偏振变动和膜厚变动脱敏的高分子波导宽带耦合器

针对高分子光波导制造工艺中波导芯厚度的均匀性难以控制,以及材料较大的折射率各向异性引起的偏振态依赖性的实际问题,提出了采用抗波导芯厚度误差、抗偏振变动的宽带波导耦合器回路结构的解决方案,并给出了优化设计的理论和方法.在实测了含氟聚酰亚胺薄膜的色散特性的基础上,采用该方法做了中心波长为1550 nm、带宽为120 nm的3 dB含氟聚酰亚胺波导耦合器设计.该器件的三维BPM仿真运行结果表明,在上述带宽上,波导芯厚度变动在7～8 μm的范围内,两个正交偏振态均可实现(50±1.0)% 功率输出比的良好特性.     

ZrO_2/SiO_2溶胶-凝胶薄膜膜层间的渗透行为

分别以丙醇锆和正硅酸乙酯为原料,采用溶胶-凝胶工艺制备了性能稳定的ZrO2和SiO2溶胶。用旋转镀膜法在K9玻璃上分别制备了单层SiO2薄膜、单层ZrO2薄膜、ZrO2/SiO2双层膜和SiO2/ZrO2双层膜。采用原子力显微镜观察了薄膜的表面形貌,用椭偏仪测量薄膜的厚度与折射率,用紫外-可见光分光光度计测量了薄膜的透射率。对薄膜的透射光谱和椭偏仪模拟的数据进行分析,发现SiO2/ZrO2双层膜之间的渗透十分明显,而ZrO2/SiO2双层膜之间几乎不发生渗透。利用TFCalc模系设计软件,采用三层膜模型对薄膜的透射率进行模拟,得出的透射曲线与用紫外-可见光分光光度计测量的透射曲线十分符合。     

光波导技术同步测量棱镜及波导薄膜参数

依据全反射理论和棱镜耦合原理,实现了对棱镜折射率及波导薄膜材料折射率和厚度的同步测量。使用高准直半导体激光器激光入射到棱镜内部与波导膜的分界面上,逐步旋转棱镜或改变棱镜的入射角,得到棱镜耦合M线,曲线前面几组的波谷为波导模激发,在M线左侧收尾处有一个不完整波峰,其反射光强随入射角迅速衰减,为全反射时的临界点,由此可实现棱镜及波导薄膜参数的同步测量;用此法测量了棱镜耦合一体化平面波导棱镜的折射率和聚甲基丙烯酸甲酯(PMMA)聚合物波导薄膜的折射率和厚度。测量棱镜折射率精度为±1.9×10-4,波导薄膜折射率和厚度的精度分别为±6.2×10-4 μm和±1.6×10-2 μm。     

有机-无机复合ZrO2-SiO2平面光波导

采用溶胶-凝胶法合成ZrO2-SiO2有机一无机复合光波导材料,通过改变其中ZrO2的含量来调节材料的折射率,使材料分别适用于平面光波导的导光层(ng≈1．497)和衬底层、包层(mb=nc≈1．479)。采用旋转涂膜工艺和相应的热处理,在单晶硅基片上制备衬底层、导光层和包层等薄膜,其中导光层介质因具有感光性而可通过紫外光刻来制备光路图案。所得有机一无机复合ZrO2-SiO2板型平面光波导(衬底层 导光层),用棱镜耦合截断法测试其光损耗在632．8nm波长处约为0．8dB／cm。对板型平面波导的导光层薄膜进行紫外光刻和异丙醇淋洗,制备出脊状光波导通道,在覆盖包层后,即获得埋层沟道式平面光波导。采用端耦合截断法测试了埋层沟道式平面光波导的光损耗(小于0．1dB／cm),并观察了其近场图像以及导光材料在近红外窗口的吸收光谱。     

平面光波导型单纤三向器的研究

利用光束传输法,分析设计了一种只由两个定向耦合器构成、能直接与单模光纤相耦合、易于集成的平面光波导（Planar Lightwave Circuit,PLC）型1.31/1.49/1.55 μm单纤三向器.该器件的输入输出弯曲波导和耦合区平行波导均采用光束传输法进行优化设计,并对器件的折射率进行了容差分析,获得了当两个定向耦合器的耦合长度分别为6 578 μm、3953 μm时,器件对各波长的隔离度均在47 dB以上,且插入损耗小于0.05 dB.     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

Dependence of the Intensity of the Spectral Lines and the Composition of the Sample and the Plasma Parameters of the Unipolar Arc

The investigation was made of the dependence of the intensity of Tl, Ga, Mo, Mg, Mn, Sn, Bi, Ni, Zn, Pt and Au spectral lines and the plasma parameters (temperature T, electron concentration n_e, degree of 6 ionnization α) from concentration of lithium additive.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...