The optical emission lines of type 1 X-ray bright Active Galactic Nuclei

A strong X-ray emission is one of the defining signatures of nuclear activity in galaxies. According to the Unified Model for Active Galactic Nuclei (AGN), both the X-ray radiation and the prominent broad emission lines, characterizing the optical and UV spectra of Type 1 AGNs, are originated in the innermost regions of the sources, close to the Super Massive Black Holes (SMBH), which power the central engine. Since the emission is concentrated in a very compact region (with typical size r?0.1$r?0.1$ pc) and it is not possible to obtain resolved images of the source, spectroscopic studies of this radiation represent the only valuable key to constrain the physical properties of matter and its structure in the center of active galaxies. Based on previous studies on the physics of the Broad Line Region (BLR) and on the X-ray spectra of broad (FWHM_Hβ ? 2000 km s⁻¹) and narrow line (1000 km s⁻¹ ?FWHM_Hβ ? 2000 km s⁻¹) emitting objects, it has been observed that the kinematic and ionization properties of matter close to the SMBHs are related together, and, in particular, that ionization is higher in narrow line sources. Here we report on the study of the optical and X-ray spectra of a sample of Type 1 AGNs, selected from the Sloan Digital Sky Survey (SDSS) database, within an upper redshift limit of z=0.35$z=0.35$, and detected at X-ray energies. We present analysis of the broad emission line fluxes and profiles, as well as the properties of the X-ray continuum and Fe Kα emission and we use these parameters to assess the consistency of our current AGN understanding.     

A model for the Balmer pseudocontinuum in spectra of type 1 AGNs

Here we present a new method for subtracting the Balmer pseudocontinuum in the UV part of type 1 AGN spectra. We calculate the intensity of the Balmer pseudocontinuum using the prominent Balmer lines in AGN spectra. We apply the model on a sample of 293 type 1 AGNs from SDSS database, and found that our model of Balmer pseudocontinuum + power law continuum very well fits the majority of AGN spectra from the sample, while in ∼$\sim$15% of AGNs, the model fits reasonable the UV continuum, but a discrepancy between the observed and fitted spectra is noted. Some of the possible reasons for the discrepancy may be a different value for the optical depth in these spectra than used in our model or the influence of the intrinsic reddening.     

Determination of visible coordinates of the low-orbit space objects and their photometry by the CCD camera with the analogue output. Initial image processing

The number of artificial space objects in the low Earth orbit has been continuously increasing. That raises the requirements for the accuracy of measurement of their coordinates and for the precision of the prediction of their motion. The accuracy of the prediction can be improved if the actual current orientation of the non-spherical satellite is taken into account. In so doing, it becomes possible to directly determine the atmospheric density along the orbit. The problem solution is to regularly conduct the photometric surveillances of a large number of satellites and monitor the parameters of their rotation around the centre of mass. To do that, it is necessary to get and promptly process large video arrays, containing pictures of a satellite against the background stars.     

基于图形法的仿生拓扑优化方法

针对图形系统自动生成图形拓扑形式的优势,提出了一种以隐式方式表征结构拓扑形式的分步拓扑优化设计方法。该分步优化方法首先以基结构法（ground structure method）的计算结果为基础,并通过均匀化方法得到设计区域内的离散拓扑信息,利用第一步所得的拓扑数据指导分形系统中每一级新增拓扑结构的生长方向,以类似细胞分裂生长的形式完成整体结构拓扑形式生成。最后以参数化建模方式完成模型的结构有限元的批量计算,并结合进化算法,完成对设计模型的优化。其中第一个案例通过本文仿生方法在多目标优化方法下得到了近似Michell结构的最优拓扑结构,第二个方案中机翼蒙皮的屈曲载荷系数提升了10.61%,并且质量降低了10.85%,验证了本文方法在类平面结构拓扑优化方面的可行性。      

基于热力学的HTPB/AP复合底排药损伤本构模型及损伤差异分析

为研究HTPB/AP复合底排药（CBBG）单轴拉伸力学性能,进行了准静态（233~301 K,8.3×10^-5~8.3×10^-1 s^-1）和冲击（233~323 K,1 200~8 000 s^-1）加载实验。实验结果表明,各工况下的真应力应变曲线均有明显的屈服点,初始模量、屈服应力及后屈服阶段形态均呈现显著的温度和应变率相关性。在不可逆热力学框架内,推导了热力学力表达式和内变量演化法则,结合初始模量和屈服应力模型,建立了黏弹-黏塑-损伤本构模型。根据HTPB/AP CBBG宽泛温度和应变率实验数据,利用一维形式的本构模型进行了参数辨识和模型验证。结果表明,该模型能较准确描述黏弹性阶段和后屈服阶段。不同工况下的损伤演化律表明,冲击加载和低温均有利于损伤扩展。     

面向映射单调性的TC4初生α相晶粒尺寸超声评价方法

随着被检对象微观组织结构复杂信息的增加,以误差最小为目标来建立有效的评价曲线越来越难,针对这一问题提出了一种以单调性为目标的TC4钛合金初生α相晶粒尺寸超声评价方法。依据相关性度量从多个超声参数中选取有效参数,经映射函数降成单维参数并归一化处理后与晶粒尺寸进行一次项拟合,构建以单调性（特征参数样本点依次序列差值同时为正或为负）最大为目标的优化问题并结合自适应差分进化（SADE）算法进行求解,寻找最佳的映射函数和拟合函数系数,最终建立映射单调性的多参数超声评价模型。实验结果表明,因考虑了单调性的重要性且与误差为目标的评价模型相比,所建模型的评价效应更显优势。与单一参数的声速模型、衰减系数模型和非线性系数模型对比分析,所建模型误差小、单调性好、性能稳定且有着评价结果精度高等特点。     

光船对气液两相介质激光支持爆轰波影响的数值模拟

建立了气液两相介质单脉冲激光支持爆轰波的数值模型,结合光船边界条件,数值模拟爆轰波及其周围流场的演化过程,分析温度、压力、速度场在爆轰波发生时的变化特性和演化形态。研究表明:有无光船边界在30μs前爆轰波发展趋势基本一致。激光作用结束后,焦点范围处温度压力均达到最大,速度继续上升达到最大后逐渐衰减。温度最大值一直在焦点附近,压力最大值则是在激光作用时出现在中心处,激光作用结束后,转移到波阵面上,而速度最大值发生在冲击波波阵面上。光船模型中,冲击波会与壁面发生耦合作用,冲击波的反射与叠加作用使最大温度中心会向外偏移,压力和速度会在壁面与冲击波边沿接触面的两侧处达到最大值,向内侧逐渐减小。      

Computations of unsteady transonic flow over airfoil at low Reynolds number

Transonic flow over a thin airfoil at low Reynolds number was studied numerically by directly solving two-dimensional full Navier-Stokes equations through 5th order weighted essentially non-oscillatory(WENO) scheme without using any turbulence model.A series of distinguished unsteady phenomena for a thin 2-D transonic airfoil flow were presented.Due to continuous adverse pressure gradient in the subsonic flow downstream of the sonic line, the unsteady separated boundary layer with main vortex and secondary vortex was developed at the rear of the airfoil.At the trailing edge,the vortex-shedding was characterized by periodical connection of the main vortex and secondary vortex on the other side of the airfoil.The unsteady separation and vortex-shedding occurred with the same period.On the airfoil surface,the average pulse pressure related to the unsteady supersonic region was obviously smaller than that related to the vortex-shedding at the trailing edge.With the attack angle increasing from 0° to 2°, the frequency of vortex-shedding decreases about 4.2%.At last, the turbulence intensity and many second-order statistics in the wake region were investigated.      

基于自适应差分进化和BP网络的罗盘误差补偿

To improve the acuuracy of heading angle measured by electronic compass, a new error compensation method is proposed based on adaptive differential evolution algorithm and BP neural network. In the method, the 3 layer BP neural network is used to model heading angle error, and adaptive differential evolution algorithm is adopted to train the weights of network, thus obtaining a more exact error model, and compensating the heading angle error measured by electronic compass. Compared with other compensation methods such as 8 position least squares, BP neural network, differential evolution algorithm for optimizing BP neural network, and so on, its error compensation accuracy is significantly improved, the method has strong global optimization ability, great convergence rate, good stability, and so on. The experimental results show that after compensation, the error range of heading angle is decreased from -16°~30.7° to -0.22° ~0.2°, which satisfies the needs of higher accuracy navigation systems.