Determining the cosmological parameters from the linewidths of active galaxies

We have previously shown that the linewidth distribution in AGN can be accounted for by an axisymmetric broad-emission-line region. In this paper we show that the linewidth distribution changes with redshift and that these changes are dependent on H ₀ and q ₀. We show that relatively small samples of AGN at high redshift with measured linewidth at half maximum can be used to distinguish between values of H ₀ and q ₀. Furthermore, larger low-redshift samples can be used to distinguish between luminosity functions and hence different models of quasar evolution.     

海洋磁力测量测线布设间距的选取

基于海洋磁力测量特点,在对布设测线方向研究的基础上,对海洋磁力测量中布设测线间距的选取进行了研究,提出了选取布设测线间距的原则,给出了几种选取测线间距的方法,并对其可行性进行了验证。     

基于LiDAR点云数据的水体轮廓线提取方法研究

提出一种基于机载激光雷达点云数据提取水体轮廓线的方法。采用双层格网模式提取较窄的水体;以朝向水体的边界点作为拟合轮廓线的关键点提取更精确的轮廓线。实验表明,该方法可以较好地提取水体轮廓线。     

Ba II lines as luminosity indicators: s-Cepheids and non-variable supergiants

Ba II line equivalent widths appear to be well correlated with the absolute magnitudes for yellow supergiants. Two Ba II lines 5853.6 Å and 6141.7 Å were applied for investigation of the possible relation between their equivalent widths and M_v for small-amplitude Cepheids and non-variable supergiants.     

TIN中边侧向关系在三角形定位、Voronoi图和等值线生成等算法中的应用

使用一种含有边拓扑关系的TIN数据结构,从三角网的拓扑关系角度利用这种结构中的边拓扑关系设计了三角形定位、Voronoi图生成和等值线生成的算法.这些算法避免了在三角形中拓扑关系查询时的不必要的搜索.更重要的是,在算法的编写过程中,如果避免一些不必要的搜索,则意味着算法更加清晰,并减少了出错的机率.经过上机验证,三种算法都获得了正确、满意的结果.     

Populations of Rydberg levels of atoms in the interstellar medium

Populations of Rydberg levels of atoms are calculated including effects of lowering the atomic ionization potential. Due to these effects the boundary conditions in b_n problem is lim b_n = 0. The b_n factors were computed for T = 100 K. N_e = 0.1 cm⁻³ with b_n = 0 when n ≧ 3000. The result allows to interpret observational data of the carbon decametric lines without the use of the subthermal dielectronic recombination mechanism. The calculations predict high relative intensities of C_nβ and C_nγ lines.     

南海区域商船典型空间分布及贸易流向研究

随着中国对外开放的深入以及“一带一路”倡议的推进,南海战略地位更加显著。如何科学监管南海船舶,维护国家权益,促进地区之间贸易也成为摆在政府部门面前的难题。在本文中利用南海区域2015年的卫星AIS数据与船舶数据档案资料,通过计算南海水域船舶交通密度分析主要航路,与关键门线船舶流量计算相结合,明确船舶典型空间分布;同时基于4种类型船舶的主要航路的选择,明确南海货物贸易主要流向。研究成果表明：① 船舶空间分布在《世界大洋航路》的推荐航线上,南海的建设开发并未影响船舶的贸易运输;② 贸易运输以跨越南海的长距离运输为主,珠三角作为主要航路的重要端点表明中国在南海贸易的优势地位。     

循环荷载作用下合成纤维系缆粘弹塑性应力应变关系

在循环载荷作用下,合成纤维系缆的应力应变关系表现出明显的非线性特性,直接影响系泊缆绳的动力响应。如何针对其在循环载荷作用下的应力应变关系进行准确的定量描述是有关绷紧式系泊系统设计的关键问题。国内外研究者之前的研究不能反映缆绳的载荷历史、蠕变特性以及刚度变化过程,因此提出一个粘弹性粘塑性模型来描述合成纤维系缆的应力应变关系。本模型能够反映合成纤维缆绳的时间变化特性以及在整个加载—卸载过程中的刚度变化。此外,提出了明确的参数确定方法及步骤,基于简单的蠕变实验可以确定模型的各个参数。将两种载荷条件下聚酯缆绳的实验结果与模型结果进行对比,二者吻合较好,证明了模型的有效性和可靠性。本研究对于绷紧式系泊系统的研发和工程应用具有重要意义。     

Identification of D3 and Hα spicules

Basing on the analysis of observational material obtained with the 53-cm coronagraph in Abastumani, the author concludes that chromospheric spicules in hydrogen and helium lines are one and the same formation. Besides, it should be noted that, as a result of radial velocity measurements, it was found that hydrogen and helium D3 lines are emitted from different areas of the same spicule.