基于同步移相技术的1/4波片快轴方位角的实时测量

提出了一种基于同步移相技术的1/4波片快轴方位角的实时测量方法。由正交光栅、光阑、检偏器组和四象限探测器实现同步移相功能。检偏器组由4个不同方位角的检偏器组成。通过检偏器组的四束光束的光强由四象限探测器同时测量。1/4波片的快轴方位角由这四光束的光强得到。由于该方法不需旋转偏振器件，从而实现的1/4波片的快轴方位角的实时测量。

Relativistic velocity - potential hydrodynamics and stellar stability

The equations of relativistic, perfect-fluid hydrodynamics are cast in Eulerian form using six scalar "velocity-potential" fields, each of which has an equation of evolution. These equations determine the motion of the fluid through the equation

U_ʋ=µ^-1 (ø,_ʋ + αβ,_ʋ + ƟS,_ʋ).

Einstein's equations and the velocity-potential hydrodynamical equations follow from a variational principle whose action is

I = (R + 16π p) (-g)^1/2 d⁴x,

where R is the scalar curvature of spacetime and p is the pressure of the fluid. These equations are also cast into Hamiltonian form, with Hamiltonian density –T₀⁰ (-g^oo)^-1/2.

The second variation of the action is used as the Lagrangian governing the evolution of small perturbations of differentially rotating stellar models. In Newtonian gravity this leads to linear dynamical stability criteria already known. In general relativity it leads to a new sufficient condition for the stability of such models against arbitrary perturbations.

By introducing three scalar fields defined by

ρ ᵴ = ∇λ + ∇x(xi + ∇xɣi)

(where ᵴ is the vector displacement of the perturbed fluid element, ρ is the mass-density, and i, is an arbitrary vector), the Newtonian stability criteria are greatly simplified for the purpose of practical applications. The relativistic stability criterion is not yet in a form that permits practical calculations, but ways to place it in such a form are discussed.

Using Earth Deformation Caused by Surface Mass Loading to Constrain the Elastic Structure of the Crust and Mantle

Surface mass loads come in many different varieties, including the oceans, atmosphere, rivers, lakes, glaciers, ice caps, and snow fields. The loads migrate over Earth's surface on time scales that range from less than a day to many thousand years. The weights of the shifting loads exert normal forces on Earth's surface. Since the Earth is not perfectly rigid, the applied pressure deforms the shape of the solid Earth in a manner controlled by the material properties of Earth's interior. One of the most prominent types of surface mass loading, ocean tidal loading (OTL), comes from the periodic rise and fall in sea-surface height due to the gravitational influence of celestial objects, such as the moon and sun. Depending on geographic location, the surface displacements induced by OTL typically range from millimeters to several centimeters in amplitude, which may be inferred from Global Navigation and Satellite System (GNSS) measurements with sub-millimeter precision. Spatiotemporal characteristics of observed OTL-induced surface displacements may therefore be exploited to probe Earth structure. In this thesis, I present descriptions of contemporary observational and modeling techniques used to explore Earth's deformation response to OTL and other varieties of surface mass loading. With the aim to extract information about Earth's density and elastic structure from observations of the response to OTL, I investigate the sensitivity of OTL-induced surface displacements to perturbations in the material structure. As a case study, I compute and compare the observed and predicted OTL-induced surface displacements for a network of GNSS receivers across South America. The residuals in three distinct and dominant tidal bands are sub-millimeter in amplitude, indicating that modern ocean-tide and elastic-Earth models well predict the observed displacement response in that region. Nevertheless, the sub-millimeter residuals exhibit regional spatial coherency that cannot be explained entirely by random observational uncertainties and that suggests deficiencies in the forward-model assumptions. In particular, the discrepancies may reveal sensitivities to deviations from spherically symmetric, non-rotating, elastic, and isotropic (SNREI) Earth structure due to the presence of the South American craton.

On the Lyapunov transformation for stable matrices

The matrices studied here are positive stable (or briefly stable). These are matrices, real or complex, whose eigenvalues have positive real parts. A theorem of Lyapunov states that A is stable if and only if there exists H ˃ 0 such that AH + HA* = I. Let A be a stable matrix. Three aspects of the Lyapunov transformation L_A :H → AH + HA* are discussed.

1. Let C₁ (A) = {AH + HA* :H ≥ 0} and C₂ (A) = {H: AH+HA* ≥ 0}. The problems of determining the cones C₁(A) and C₂(A) are still unsolved. Using solvability theory for linear equations over cones it is proved that C₁(A) is the polar of C₂(A*), and it is also shown that C₁ (A) = C₁(A^-1). The inertia assumed by matrices in C₁(A) is characterized.

2. The index of dissipation of A was defined to be the maximum number of equal eigenvalues of H, where H runs through all matrices in the interior of C₂(A). Upper and lower bounds, as well as some properties of this index, are given.

3. We consider the minimal eigenvalue of the Lyapunov transform AH+HA*, where H varies over the set of all positive semi-definite matrices whose largest eigenvalue is less than or equal to one. Denote it by ψ(A). It is proved that if A is Hermitian and has eigenvalues μ₁ ≥ μ₂…≥ μ_n ˃ 0, then ψ(A) = -(μ₁-μ_n)²/(4(μ₁ + μ_n)). The value of ψ(A) is also determined in case A is a normal, stable matrix. Then ψ(A) can be expressed in terms of at most three of the eigenvalues of A. If A is an arbitrary stable matrix, then upper and lower bounds for ψ(A) are obtained.

磷酸盐激光玻璃聚（CH3）2Si（OC2H5）2防潮膜

以（CH3）2Si（OC2H5）2为前驱体，采用溶胶-凝胶与有机合成相结合的方法，制得稳定性良好的涂膜液。采用旋转涂膜法在掺钕磷酸盐激光玻璃棒端面涂制防潮膜，膜层固化后透过率达96．5％，获得的膜层表面粗糙度优良，均方根表面粗糙度（RMS）为1．659nm，平均粗糙度（RA）平均为1．321nm；在激光波长1053nm，脉冲宽度1 ns条件下膜层的激光破坏闽值可达10～14 J／cm^2。经过“神光Ⅱ”高功率激光器物理实验运行，膜层使用期为五年，并且已经在我国“神光Ⅲ”原型装置上试用。

环形抛光中工件形状对抛光速度的影响

本文基于库仑摩擦模型，模拟了不同形状的工件在环形抛光的运动。从结果可知，（1）如果工作环处于自由转动状态，工件的角速度在环形抛光中比抛光盘的角速度大；（2）可通过控制工作环的角速度使工件和抛光盘的角速度同步。工作环的角速度依赖于工作环和工件的半径、抛光盘－工件和抛光盘－工作环的摩擦系数，以及抛光盘的角速度；（3）有尖角的工件与工作环的接触处于不连续状态，导致二者的接触状态发生变化和工件角速度的波动。

Avaliação numérica de estabilidade lateral de vigas casteladas

Restrições de espaço e altura são frequentemente impostas às edificações residenciais, comerciais, industriais, depósitos e galpões com um ou diversos pavimentos em função de aspectos de regulamentos regionais, técnicos, econômicos ou ainda de natureza estética. A fim de proporcionar a passagem de tubulações e dutos de grande diâmetro sob vigas de aço, grandes alturas são normalmente requeridas, demandando por vezes, magnitudes de altura inviáveis entre pavimentos de edificações. Diversas soluções estruturais podem ser utilizadas para equacionar tais obstáculos, onde dentre outras, pode-se citar as vigas com inércia variável, stub-girders, treliças mistas, vigas misuladas e vigas com uma ou múltiplas aberturas na alma com geometrias variadas. No que tange às vigas casteladas, solução estrutural pautada neste estudo, a estabilidade é sempre um motivo de preocupação tipicamente durante a construção quando os contraventamentos laterais ainda não estão instalados. De qualquer forma, o comprimento destravado em geral alcançado pelos vãos destas vigas, são longos o suficiente para que a instabilidade ocorra. Todavia, o acréscimo substancial da resistência à flexão de tais membros devido ao aumento da altura oriundo de seu processo fabril em relação ao perfil matriz, aliada a economia de material e utilidade fim de serviço, garante a atratividade no aproveitamento destas, para grandes vãos junto aos projetistas. Não obstante, este aumento proporcional no comprimento dos vãos faz com que a instabilidade lateral ganhe importância especial. Neste contexto, o presente trabalho tem por objetivo desenvolver um modelo numérico que permita a realização de uma avaliação paramétrica a partir da calibração do modelo com resultados experimentais, efetuar a análise do comportamento de vigas casteladas e verificar seus mecanismos de falha, considerando comportamento elasto-plástico, além das não-linearidades geométricas. Também é objetivo deste trabalho, avaliar, quantificar e determinar a influência das diferenças geométricas características das vigas casteladas em relação às vigas maciças com as mesmas dimensões, analisando e descrevendo o comportamento estrutural destas vigas de aço para diversos comprimentos de vãos. A metodologia empregada para tal estudo baseou-se em uma análise paramétrica com o auxílio do método numérico dos elementos finitos.

Ecologia térmica e comportamento de construção de abrigos de Liolaemus lutzae (Lacertilia, Liolaemidae) em três áreas de restinga no estado do Rio de Janeiro, sudeste do Brasil: os efeitos de fatores extrínsecos e intrínsecos

Fatores extrínsecos afetam a ecologia térmica e o comportamento de lagartos no habitat, com as características ambientais locais podendo ocasionar alterações na temperatura corpórea (Tc) e no comportamento destes animais. Entretanto, fatores intrínsecos também representam uma importante influência para sua biologia, assim como fatores filogenéticos (históricos). Liolaemus lutzae (Liolaemidae) é uma espécie de lagarto com ocorrência restrita a restingas do estado do Rio de Janeiro (entre a Restinga da Marambaia no município do Rio de Janeiro e a restinga da Praia do Peró no município de Cabo Frio), vivendo exclusivamente na zona de vegetação halófila-psamófila-reptante a chamada área-de-praia da restinga (sujeita a altas temperaturas ambientais e ventos intensos constantes). Nessa área, onde vivem restritos a uma faixa de poucos metros de restinga, os indivíduos se abrigam escavando abrigos no substrato arenoso. Avaliei a importância de fontes ambientais de calor, da intensidade dos ventos, do sexo, da ontogenia, do comprimento rostro-cloacal (CRC) e da massa corpórea para a Tc e a taxa de atividade de lagartos L. lutzae (observando a ocorrência de variações sazonais), em estudos conduzidos no município de Arraial do Cabo, estado do Rio de Janeiro, sudeste do Brasil. Além disso, eu analisei se o comportamento de L. lutzae, direcionando as aberturas de seus abrigos foi afetado por fatores ambientais nas restingas da Reserva Ecológica Estadual de Jacarepiá e do Parque Natural Municipal de Grumari, ambas no estado do Rio de Janeiro. A atividade dos lagartos se estendeu durante o dia (0600h às 1800h), com máximo entre 1100h e 1300h (com variações sazonais). A Tc dos indivíduos foi 31,7  3,4 C, e variou ao longo do dia e sazonalmente. Em ambas as estações a Tc dos lagartos relacionaram-se às temperaturas do microhabitat (substrato e ar). A intensidade do vento influenciou a Tc dos lagartos (causando seu decréscimo), e a intensidade média do vento afetou o número de lagartos ativos (causando redução da atividade). Houve diferenças intersexuais no CRC, com os machos maiores do que as fêmeas, embora as fêmeas tenham tido maior massa corpórea relativa ao CRC correspondente, comparado aos machos. A Tc também diferiu inter-sexualmente (com machos mais quentes do que fêmeas) e ontogeneticamente (com jovens mais quentes do que adultos depois de removido o efeito do tamanho corpóreo). Houve relações entre a Tc e o CRC e entre a Tc e a massa corpórea, com lagartos maiores tendo Tc mais elevada (causada pela inércia térmica dos corpos). A variabilidade na Tc dos lagartos parece refletir a interação entre características ambientais locais, fatores intrínsecos e a filogenia da espécie. As aberturas dos abrigos foram localizadas principalmente próximas à linha de praia (possivelmente devido ao substrato menos compacto), predominantemente em terrenos inclinados e tiveram uma tendência de orientação influenciada pela inclinação do terreno. O comportamento de L. lutzae de orientar a entrada de seus abrigos para a direção descendente das inclinações pode ser vantajoso para torná-los menos vulneráveis a potenciais ameaças e distúrbios vindos da superfície.

Dynamic storage performance of two cyanine dye films and optimization design for a recordable compact disk

The optical constants of two cyanine dye films that we prepared were measured with a RAP-1-type (RAP is rotating analyzer and polarizer) spectroscopic ellipsometer. Toward making a simplified model for the wafers of a recordable compact disk (CD-R), we give their optimization designs developed with the cyanine dye films. in addition, the dynamic storage performances of two sample disks were tested by our dynamic storage testing system. Measurement results of the sample disks were obtained to test and verify our film designs. (C) 2000 Optical Society of America. OCIS codes: 160.4890, 160.4760, 210.4810.

Optical parameters and absorption of copper (II)-azo complexes thin films as optical recording media

Smooth thin films of three kinds of azo dyes of 2-(5'-tert-butyl-3'-azoxylisoxazole)-1, 3-diketones and their copper (II)-azo complexes were prepared by the spin-coating method. Absorption spectra of the thin films on a glass substrate in the 300-600 nm wavelength region were measured. Optical constants (complex refractive index N=n+ik) and thickness of the thin films prepared on single-crystal silicon substrate in the 300-600 nm wavelength region were investigated on rotating analyzer-polarizer type of scanning ellipsometer, and dielectric constants epsilon(epsilon=epsilon(1)+i epsilon(2)), absorption coefficients alpha as well as reflectance R of thin films were then calculated. In addition, one of the copper (II)-azo complex thin film prepared on glass substrate with an Ag reflective layer was also studied by atomic force microscopy (AFM) and static optical recording. AFM study shows that the copper (II)-azo complex thin film is very smooth and has a root mean square surface roughness of 1.89 nm. Static optical recording shows that the recording marks on the copper (II)-azo complex thin film are very clear and circular, and the size of the minimal recording marks can reach 200 nm. (c) 2004 Elsevier B.V. All rights reserved.

Determination and analysis of the optical constants of thin films of nickel(II) and copper(II) hydrazone complexes by spectroscopic ellipsometry

Thin films of four nickel(II) and copper(II) hydrazone complexes, which will hopefully be used as recording layers for the next-generation of high-density recordable disks, were prepared by using the spin-coating method. Absorption spectra of the thin films on K9 optical glass substrates in the 300-700 nm wavelength region were measured. Optical constants (complex refractive indices N) and thickness d of the thin films prepared on single-crystal silicon substrates in the 275-675 nm wavelength region were investigated on a rotating analyzer-polarizer scanning ellipsometer by fitting the measured ellipsometric angles (Psi(lambda) and Delta(lambda)) with a 3-layer model (Si/dye film/air). The dielectric functions epsilon and absorption coefficients alpha as a function of the wavelength were then calculated. Additionally, a design to achieve high reflectivity and optimum dye film thickness with an appropriate reflective layer was performed with the Film Wizard software using a multilayered model (PC substrate/reflective layer/dye film/air) at 405 nm wavelength.

Optical properties of nickel(II)-azo complexes thin films for potential application as high-density recordable optical recording media

Smooth thin films of three kinds of nickel(II)-azo complexes were prepared by the spin-coating method. Absorption spectra of the thin films on K9 glass substrate in the 300-600 nn wavelength region were measured. Optical constants (complex refractive index N = n + ik) and thickness of the thin films prepared on single-crystal silicon substrate in the 300-600 nm wavelength region were investigated on rotating analyzer-polarizer type of scanning ellipsometer, and dielectric constants epsilon (epsilon = epsilon(1) + i epsilon(2)), absorption coefficients a as well as reflectance R of thin films were then calculated at 405 nm. In addition, in order to examine the possible use of nickel(II)-azo complex thin film as an optical recording medium, one of the nickel(II)-azo complex thin film prepared on K9 glass substrate with an Ag reflective layer was also studied by atomic force microscopy and static optical recording. The results show that the nickel(II)-azo complex thin film is smooth and has a root mean square surface roughness of 2.25 nm, and the recording marks on the nickel(II)-azo complex thin film are very clear and circular, and their size can reach 200 nn or less. (c) 2006 Elsevier Ltd. All rights reserved.

2-氨基-6-乙氧基苯并噻唑类偶氮染料及其金属鏊合物的合成及光学热学性能研究

合成了2-（2-氨基-6-乙氧基苯并噻唑基偶氮）-5-（N,N-二乙基氨基）三氟甲基磺酰苯胺偶氮染料（EBTDATFS）及其与乙酸镍、乙酸钴、乙酸铜、乙酸锌等金属盐鏊合的金属鏊合物。通过红外光谱、紫外-可见吸收光谱和MALDI质谱等对染料及其金属鏊合物进行了结构表征;使用旋涂方法在K9玻璃和抛光的单晶硅基片上制备薄膜;研究了镍金属鏊合物的热学性能;使用椭偏仪研究了Ni和Zn鏊合物的光学常数。结果表明：4种金属鏊合物薄膜最大吸收光谱为621-629nm,且长波边吸收峰陡峭;TGA-DSC测试结果表明镍金属鏊

Low-Power Super-resolution Readout with Antimony Bismuth Alloy Film as Mask layer

Sb-Bi alloy films are proposed as a new kind of super-resolution mask layer with low readout threshold power. Using the Sb-Bi alloy film as a mask layer and SiN as a protective layer in a read-only memory disc, the super-resolution pits with diameters of 380 nm are read out by a dynamic setup, the laser wavelength is 780 nm and the numerical aperture of pickup lens is 0.45. The effects of the Sb-Bi thin film thickness, laser readout power and disc rotating velocity on the readout signal are investigated. The results show that the threshold laser power of super-resolution readout of the Sb-Bi mask layer is about 0.5 mW, and the corresponding carrier-to-noise ratio is about 20 dB at the film thickness of 50 nm. The super-resolution mechanism of the Sb-Bi alloy mask layer is discussed based on its temperature dependence of reflection.

Cr^3＋，Yb^3＋，Er^3＋共掺磷酸盐铒玻璃转镜调Q激光性质研究

研究了Cr^3＋，Yb^3＋，Er^3＋共掺磷酸盐铒玻璃转镜调Q激光性质．三种Er2O3掺杂浓度的激光实验结果表明，在Er2O3名义掺杂浓度为0．5wt％时，玻璃的综合激光性质最好，重复频率为0．1Hz时，它的激光阈值功率为14．5mJ，最大输出能量为9．6mJ，斜率效率为0．55％．在同种实验条件下，比较了Cr14和Kigre公司生产的QE-7S激光性质参数，实验表明，前者激光阈值功率稍低，而后者的斜率效率和最大输出功率略高．