Pseudo-beam method for compressive buckling characteristics analysis of space inflatable load-carrying structures

This paper extends Le van＇s work to the case of nonlinear problem and the complicated configuration. The wrinkling stress distribution and the pressure effects are also included in our analysis. Pseudo-beam method is presented based on the inflatable beam theory to model the inflatable structures as a set of inflatable beam elements with a prestressed state. In this method, the discretized nonlinear equations are given based upon the virtual work principle with a 3-node Timoshenko＇s beam model. Finite element simulation is performed by using a 3-node BEAM189 element incorporating ANSYS nonlinear program. The pressure effect is equivalent included in our method by modifying beam element cross-section parameters related to pressure. A benchmark example, the bending case of an inflatable cantilever beam, is performed to verify the accuracy of our proposed method. The comparisons reveal that the numerical results obtained with our method are close to open published analytical and membrane finite element results. The method is then used to evaluate the whole buckling and the loadcarrying characteristics of an inflatable support frame subjected to a compression force. The wrinkling stress and region characteristics are also shown in the end. This method gives better convergence characteristics, and requires much less computation time. It is very effective to deal with the whole load-carrying ability analytical problems for large scale inflatable structures with complex configuration.

Synthesis,Crystal Structure and Spectroscopic Properties of 1,2-Benzothiazine Derivatives:An Experimental and DFT Study

1,2-Benzothiazine derivatives methyl 3-methoxy-4-oxo-3,4-dihydro-2H-benzo[e] [1,2]thiazine-3-carboxylate 1,1-dioxide（1） and methyl 2-ethyl-3-hydroxy-4-oxo-3,4-dihydro-2Hbenzo[e][1,2]thiazine-3-carboxylate 1,1-dioxide（2） were synthesized, and characterized by spectroscopic techniques; 1H-NMR and infrared（IR） spectroscopy. Crystals of 1 and 2 were grown by slow evaporation of methanol and ethyl acetate, respectively and their crystal structures were investigated by single-crystal X-ray diffraction analysis. Geometric properties were calculated by the B3 LYP method of density functional theory（DFT） at the 6-31G＋（d） basis set to compare with the experimental data. Simulated properties were found in strong agreement with the experimental ones. Intermolecular forces have also been modeled in order to investigate the strength of packing and strong hydrogen bonding was observed in both compounds 1 and 2. Electronic properties such as Ionization Potential（IP）, Electron Affinities（EA） and coefficients of the highest occupied molecular orbital（HOMO） and the lowest unoccupied molecular orbital（LUMO） of com- pounds 1 and 2 were simulated for the first time.

Observational Features of Large-Scale Structures as Revealed by the Catastrophe Model of Solar Eruptions

Large-scale magnetic structures are the main carrier of major eruptions in the solar atmosphere. These structures are rooted in the photosphere and are driven by the unceasing motion of the photospheric material through a series of equilibrium configurations. The motion brings energy into the coronal magnetic field until the system ceases to be in equilibrium. The catastrophe theory for solar eruptions indicates that loss of mechanical equilibrium constitutes the main trigger mechanism of major eruptions, usually shown up as solar flares, eruptive prominences, and coronal mass ejections （CMEs）. Magnetic reconnection which takes place at the very beginning of the eruption as a result of plasma instabilities/turbulence inside the current sheet, converts magnetic energy into heating and kinetic energy that are responsible for solar flares, and for accelerating both plasma ejecta （flows and CMEs） and energetic particles. Various manifestations are thus related to one another, and the physics behind these relationships is catastrophe and magnetic reconnection. This work reports on recent progress in both theoretical research and observations on eruptive phenomena showing the above manifestations. We start by displaying the properties of large-scale structures in the corona and the related magnetic fields prior to an eruption, and show various morphological features of the disrupting magnetic fields. Then, in the framework of the catastrophe theory, we look into the physics behind those features investigated in a succession of previous works, and discuss the approaches they used.

Structural, mechanical, and electronic properties of 25 kinds of Ⅲ–Ⅴbinary monolayers: A computational study with first-principles calculation

Using first-principle calculations, we investigate the mechanical, structural, and electronic properties and formation energy of 25 kinds of Ⅲ–V binary monolayers in detail. A relative radius of the binary compound according to the atomic number in the periodic table is defined, and based on the definition, the 25 kinds of Ⅲ–V binary compounds are exactly located at a symmetric position in a symmetric matrix. The mechanical properties and band gaps are found to be very dependent on relative radius, while the effective mass of holes and electrons are found to be less dependent. A linear function between Young’s modulus and formation energy is fitted with a linear relation in this paper. The change regularity of physical properties of B–V(V = P, As, Sb, Bi) and Ⅲ–N(Ⅲ = Al, Ga, In, Tl) are found to be very different from those of other Ⅲ–V binary compounds.

Quantum Chemical Study of Geometric Structures and Properties for Ag_nH_2S(n = 1～10) Clusters

The stable structures and stabilities of AgnH2S（n = 1-10） clusters have been calculated using the B3P86-DFT method. The results predicate that the stable geometries of AgnH2 S clusters can be got by directly adding the H2 S molecule on different sites of Agn clusters. Agn clusters would like to bond with sulfur atom and the H2 S molecules are partial to adsorb at the top site in the clusters. After adsorption, the structures of Agn clusters and H2 S molecule keep the original structures except Ag9. The binding energy of AgnH2 S is distinctly larger than that of pure Agn clusters. The second difference in energy and the HOMO and LUMO gaps of Agn and AgnH2 S exhibit an obvious odd-even oscillation, which demonstrate that the stabilities of even-numbered silver clusters are relatively more stable than the neighboring odd-numbered silver clusters. Mulliken population analysis shows that charges always transfer from the H2 S molecule to Agn clusters in all clusters.

First-principles study of the co-effect of carbon doping and oxygen vacancies in ZnO photocatalyst

Although tuning band structure of optoelectronic semiconductor-based materials by means of doping single defect is an important approach for potential photocatalysis application,C-doping or oxygen vacancy(Vo)as a single defect in ZnO still has limitations for photocatalytic activity.Meanwhile,the influence of co-existence of various defects in ZnO still lacks sufficient studies.Therefore,we investigate the photocatalytic properties of ZnOx C0.0625(x=0.9375,0.875,0.8125),confirming that the co-effect of various defects has a greater enhancement for photocatalytic activity driven by visible-light than the single defect in ZnO.To clarify the underlying mechanism of co-existence of various defects in ZnO,we perform systematically the electronic properties calculations using density functional theory.It is found that the coeffect of C-doping and Vo in ZnO can achieve a more controllable band gap than doping solely in ZnO.Moreover,the impact of the effective masses of ZnO_(x)C_(0.0625)(x=0.9375,0.875,0.8125)is also taken into account.In comparison with heavy Vo concentrations,the light Vo concentration(x=0.875)as the optimal component together with C-doping in ZnO,can significantly improve the visible-light absorption and benefit photocatalytic activity.

h-P Finite Element Approximation for Full-Potential Electronic Structure Calculations

The(continuous) finite element approximations of different orders for the computation of the solution to electronic structures were proposed in some papers and the performance of these approaches is becoming appreciable and is now well understood.In this publication,the author proposes to extend this discretization for full-potential electronic structure calculations by combining the refinement of the finite element mesh,where the solution is most singular with the increase of the degree of the polynomial approximations in the regions where the solution is mostly regular.This combination of increase of approximation properties,done in an a priori or a posteriori manner,is well-known to generally produce an optimal exponential type convergence rate with respect to the number of degrees of freedom even when the solution is singular.The analysis performed here sustains this property in the case of Hartree-Fock and Kohn-Sham problems.

基于电动伺服系统的转向试验台阻力加载策略的研究

以电动伺服缸为核心的转向台架加载系统在加载过程中受减速丝杠内部摩擦、阻尼和惯量等非线性因素影响,电机电磁转矩与缸体端部实际加载阻力并非简单的减速比关系,同时被测转向系统的位移扰动产生的多余力也对阻力加载精度产生较大影响。针对这些问题,本文中首先建立转向台架的传递函数,采用PID力闭环控制和串联校正方法来提高阻力加载系统的稳定裕度和加载精度,在此基础上利用结构不变性原理和速度补偿控制对多余力进行抑制。仿真和台架试验结果表明,提出的阻力加载控制策略可有效提高加载精度和减小扰动下多余力的影响。

完全图上结构异常的搜索算法——融入量子计算思维的经典算法探讨

采用量子计算思维探索新的图结构搜索方法,提出了一种基于散射量子行走的完全图上结构异常的搜索算法.在N个顶点的完全图上外接一个悬挂点,既破坏了完全图的对称性,也预示着图的拓扑结构将发生变化.首先给出完全图上散射量子行走酉算子U的解析刻画,将行走的Hilbert空间投影到低维不变子空间S,并给出酉算子U在空间S中的作用US的形式;然后将完全图中所有状态的均匀叠加态选择为行走的初态,借用微扰理论求出酉算子US的本征值和特征向量,通过数学解析计算出行走的终态(悬挂点);最后分析算法的时间复杂度和成功概率.算法分析及Matlab仿真结果表明,利用散射量子行走可以在O(N^(1/2))步内以接近于1的概率找到异常位置,而经典算法中使用邻接矩阵查找该异常点的时间复杂度为O(N),因此相对特定问题和特定的经典算法,使用散射量子行走搜索算法可以实现二次加速.

直升机加载抑制多余力控制研究

针对直升机旋翼加载多余力问题,对耦合模型进行了分析,基于结构不变性原理,讨论了解耦通道的设计,给出了不同的结构和参数配置情况及其多余力消除效果,其结论用于实际系统调试参考。

应用前馈控制提高起落架加载系统性能的方法研究

在理论上分析了起落架加载系统多余力的产生机制及特性,并建立了相应的数学模型。利用结构不变性原理,提出了可行的前馈补偿以消除多余力的方法,并将该方法应用到某型飞机的起落架加载试验中,取得了很好的效果,满足了系统的精度要求。

系列伺服作动器动态加载系统及其控制策略

针对系列多型号伺服作动器系统的动态加载试验需求,设计了一种由直线电机与液压增力模块构成的新型加载系统,并基于AMESim/MATLAB联合仿真模型研究了系统的加载控制策略:采用多闭环与前馈复合控制提高加载系统力控制精度并改善相位滞后;基于结构不变性理论对伺服作动器的位移输出信号进行前馈补偿并抑制多余力.仿真结果表明,该加载系统方案能够有效抑制多余力,减小系统相位滞后,提高力加载精度,保证加载系统具有良好的整体性能,并可灵活地满足不同载荷、不同频率的加载测试需求.

阀控非对称缸被动加载系统中多余力的抑制

从系统的力传递函数出发,分析了阀控非对称缸被动加载系统中多余力的存在对系统加载性能的影响,此多余力经结构不变性原理补偿后在低频段可以很好地被消除,但由于在高频段滞后现象加重,多余力对加载系统的影响仍然存在。针对这一问题提出了采用最优二次型抑制多余力的控制方法,将系统的力传递函数经最优二次型控制理论优化设计并仿真后发现,在结构不变性原理的基础上采用最优二次型的控制方法可以使阀控非对称缸被动加载系统中的多余力在高频段得到较好的抑制,提高了系统的加载性能。

某旋翼加载系统分析

在进行某旋翼加载系统试验时,核心是减小多余力影响问题。文中分析了两种方法,前馈补偿和基于结构不变性原理补偿方法。前馈控制通过测量位置系统的伺服阀位移,该位移是位置干扰的函数,补偿多余力影响包括补偿伺服阀死去非线性影响。基于不变性原理补偿是实际应用中通过测量位置系统的速度,在位置系统输出和加载系统输入之间加入的补偿通道。该文研究某旋翼加载系统的多余力动态补偿及其有效性,仿真显示了补偿效果和两种方法的对比。仿真结果表明, 两种方法都有很好的多余力消除效果,可根据实际情况进行选择。

被动式电液伺服加载系统的多余力抑制

针对电液伺服加载系统中多余力较大且结构不变性原理对多余流量难以完全补偿的问题,首先要求配置合适的蓄能器,使系统有适当的体积弹性模量,从而使活塞运动所产生的多余力在可控制的范围之内;其次通过结构不变性原理对多余流量进行精确补偿,但由于伺服阀的流量增益与负载压力是非线性的,采用状态观测器获得内部压力,以实现对流量的精确控制。以AMESim-Simulink为基础建立联合仿真模型,仿真结果表明,采用上述方法对多余力的抑制效果有明显提高。

液压提升机负载适应性研究

在某型导弹液压提升机研制过程中,由于提升机受负载变化、摩擦力变化以及液压系统本身受环境因素等影响,为保证导弹装填过程的高可靠、高安全性,必须解决各种工况变化引起的输出一致性差和稳定性差等问题。通过机理建模分析方法,将液压提升机等效为一个双输入单输出的控制系统数学模型,通过对系统时域和频域仿真分析,提出了一种采用结构不变性原理和自适应变参数的速度闭环控制方法,同时根据阀的流量非线性特性,引入变步长的线性速度规划方法来减小动载荷冲击。最后通过试验验证了该控制策略的有效性。试验结果与仿真结果保持一致,满足速度控制精度要求,能够保证负载运行的安全性和可靠性。

电液伺服加载系统控制方法的改进研究

电液伺服加载系统用于仿真飞行器在空中飞行所受到的气动力状况,有效的消除由舵机的主动运动所引起的多余力是电液伺服加载中的核心问题。针对此问题采用经典的结构不变性原理设计消扰控制器进行消扰时所存在的消扰器微分阶数较高,信号的品质不好,实现起来比较困难等缺陷,选取了不同的反馈输出信号进行改进设计,降低消扰器阶数,并通过测量内部反馈信号来补偿伺服阀的流量变化。建立了电液伺服加载系统数学模型,并利用该模型对改进设计进行仿真验证。试验结果表明:改进设计系统满足预期指标要求,较好地消除了加载系统跟踪的滞后,有效减少多余力,效果令人满意。

Effect of Zn doping on electronic structure and optical properties zincblende GaN(A DFT+U insight)

The development of new materials,having exceptional properties in comparison to existing materials is highly required for bringing advancement in electronic and optoelectronic technologies.Keeping this fact,we investigated structural,electronic,and optical properties of zincblende GaN doped with selected Zn concentrations(6.25%,12.50%,and 18.70%),using the first-principle calculations based on density functional theory with GGA+U.We conducted the entire study using the WIEN2K code.In this study,we calculated various significant parametric quantities such as cohesive energies,formation energies,bulk moduli,and lattice constants along with the study of optical and electronic properties by substituting Ga atoms with Zn atoms in 1×2×2 supercell.The structural stability is confirmed by studying the phonon dispersion curves which suggest that Zn:GaN material is stable against the 6.25%and 18.70%Zn concentrations while for 12.50%,it shows instability.The Hubbard values U=0,2,4,6 eV were added to GGA and the electronic properties were improved with the U=6 eV.Optical absorption was blue shifted while the refractive index and dielectric constant were increased with increasing the Zn concentrations.Electronic properties are enhanced due to the prime contribution of cations(Zn)3ri states.The optical and electronic properties are further discussed in detail in the entire study.

On the complex structure of symplectic quotients

Let K be a compact group.For a symplectic quotient M_(λ) of a compact Hamiltonian Kahler K-manifold,we show that the induced complex structure on M_(λ) is locally invariant when the parameter λ varies in Lie(K)^(*).To prove such a result,we take two di erent approaches:(i)use the complex geometry properties of the symplectic implosion construction;(ii)investigate the variation of geometric invariant theory(GIT)quotients.

Pairwise Velocity Statistics of Dark Halos

We have accurately evaluated the halo pairwise velocity dispersion and the halo mean streaming velocity in the LCDM model (the fiat ω0 = 0.3 model) using a set of high-resolution N-body simulations. Based on the simulation results, we have developed a model for the pairwise velocity dispersion of halos. Our model agrees with the simulation results over all scales we studied. We have also tested the model of Sheth et al. for the mean streaming motion of halos derived from the pair-conservation equation. We found that their model reproduces the simulation data very well on large scale, but under-predicts the streaming motion on scales r < 10 h-1 Mpc. We have introduced an empirical relation to improve their model. These improved models are useful for predicting the redshift correlation functions and the redshift power spectrum of galaxies if the halo occupation number model, e.g. the cluster weighted model, is given for the galaxies.