Understanding high-density matter through analysis of surface spectral lines and burst oscillations from accreting neutron stars

We discuss millisecond period brightness oscillations and surface atomic spectral lines observed during type I X-ray bursts from a neutron star in a low mass X-ray binary system. We show that modeling of these phenomena can constrain models of the dense cold matter at the cores of neutron stars. We demonstrate that, even for a broad and asymmetric spectral line, the stellar radius-to-mass ratio can be inferred to better than 5%. We also fit our theoretical models to the burst oscillation data of the low mass X-ray binary XTE J1814-338, and find that the 90% confidence lower limit of the neutron star’s dimensionless radius-to-mass ratio is 4.2.     

试论《工厂电气控制设备》课程设计

该文论述了《工厂电气控制设备》课程设计教学环节的重要性 ,并通过实例介绍了课程设计训练学生实际工作能力的过程 ,该方式使课程设计达到了提高学生动手能力的效果。     

Line blanketing by iron group elements in non-LTE model atmospheres of hot stars

We report on our recent progress in modeling non-LTE atmospheres of O-stars including blanketing by lines from the iron group elements. The numerical method to account for the huge number of atomic levels and line transitions is presented. Results of exploratory model calculations examining the effects on the temperature structure, the hydrogen and helium line profiles and UV/EUV fluxes are discussed.     

一种攻击大机动目标的组合导引律

在分析经典导引律和现代导引律内在联系的基础上,利用有限可获的制导信息,提出了一种新的组合导引律,由比例项和前置角项组成,力图综合经典导引律和现代导引律的优点,结构简单,易于工程实现,并在基于目标大机动规避的假设下给出了机理解释;通过仿真验证,此方法具有末段弹道平直的优点。     

Collisional profiles of ionized calcium perturbed by helium

The spectra of many cool DZ white dwarfs show extremely broad resonance lines of ionized calcium and magnesium in the optical and ultraviolet region. When the line center is strongly saturated, these wings may become a significant source of additional opacity in cool white dwarf atmospheres. The omission of this opacity results in systematic errors in the predicted flux distribution and hence in the effective temperatures and element abundances. In a continuation of Homeier et al. (2007) and Allard et al. (2012), where we presented absorption spectra of Na–He in cool white dwarfs, we extend this work to the Ca⁺–He system.     

LiHe spectra from brown dwarfs to helium clusters

The detection of Li I lines is the most decisive spectral indicator of substellarity for young brown dwarfs with masses below about 0.06 solar mass. Due to the weakness of the Li resonance lines, it is important to be able to model precisely both their core widths and their wing profiles. This allows an adequate prediction of the mass at which Li lines reappear in the spectra of brown dwarfs for a given age, or reversely an accurate determination of the age of a cluster. We report improved line profiles and the dependence of line width on temperature suitable for modeling substellar atmospheres that were determined from new LiHe molecular potential energies. Over a limited range of density and temperature, comparison with laboratory measurements was used to validate the potential energies which support the spectral line profile theory.     

Stark broadening data for spectral lines of rare-earth elements: Nb III

The electron-impact widths for 15 doubly charged Nb ion lines have been theoretically determined by using the modified semiempirical method. Using the obtained results, we considered the influence of the electron-impact mechanism on line shapes in spectra of chemically peculiar stars and white dwarfs.     

回转体线画图标记分析

线画图是人们之间以及人与计算机之间交换三维物体信息的主要来源之一。在计算机视觉研究领域中，线画图标记是对物体进行定性分析的一种有效方法，通过线画图的一致性标记，可排除许多不可能的物体结构，为线画图的定量分析减少工作量。曲面立休的线画图标记是一项非常困难的多作。回转体是一类特残的曲面立体，本文在前人线画图标记的研究成果基础上研究了回转体立体线画图的标记形式，得出了回转体线画图标记的新的节点型式。新的标记方法适用于由平面立体和回转体组合而成的复杂立体的线画图。     

空间失稳目标线阵成像畸变分析与三维重建

针对线阵扫描型激光雷达在非合作失稳航天器三维模型重建过程中，存在运动目标线扫数据畸变且目标因失稳导致运动特性难以准确估计问题，提出一种带畸变自修正式三维重建方法，并进行畸变容忍度临界值分析。该方法基于测量系统的角精度与测距精度设计畸变容忍度临界值判定条件，首先根据实际工况与判定条件进行比对，判定是否对线扫数据进行初始畸变恢复；其次，对相邻扫描带畸变点云依次进行配准获取目标运动增量、解算目标瞬时运动参数；然后对目标运动参数进行自修正式处理，去除特征突变点干扰；同时依次恢复点云到初始几何位置，完成初始目标三维重建；最后，通过系统进一步迭代，位姿增量自收敛直至最终满足重建精度要求。仿真结果表明，该方法在缺失非合作目标先验信息的情况下，能够有效避免因线扫描导致的畸变问题，并较为快速地实现满足精度要求的目标三维重建，有较强的鲁棒性。     

SBIRS-Low目标跟踪交接分析

对天基红外卫星系统低轨部分(SBIRS-Low)单星只测角的主动段跟踪交接进行了研究。提出了用插值和滤波两种方法计算目标视线(LOS)偏差的算法。仿真讨论了多项式阶数和时间窗长度对插值外推法的影响,以及插值外推法与滤波法性能的比较。结果表明:当预测时间小于30 s时,预测视线偏差小于0.4°,此时预测视线将以较大概率落入跟踪相机视场角1°×3°范围内,满足主动段跟踪交接条件,表明单星主动段跟踪交接具可行性。