Optical polarimetric study of open clusters: distribution of interstellar matter towards NGC 654

We present new B ,  V and R linear polarimetric observations for 61 stars towards the region of the young open cluster NGC 654. In this study we found evidence for the presence of at least two layers of dust along the line of sight to the cluster. The distances to the two dust layers are estimated to be ∼200 pc and ∼1 kpc which are located much closer to the Sun than the cluster (∼2.4 kpc). Both the dust layers have their local magnetic field orientation nearly parallel to the direction of the Galactic plane. The foreground dust layer is found to have a ring morphology with the central hole coinciding with the centre of the cluster. The foreground dust grains are suggested to be mainly responsible for both the observed differential reddening and the polarization towards the cluster.     

黄河三角洲海岸剖面类型与演变规律

根据1976-2002年黄河三角洲滨海区36个断面的地形实测资料以及利津水文站的水沙资料,运用动力地貌学的方法,对黄河三角洲海岸剖面形态及冲淤演变进行了研究。结果表明,黄河三角洲海岸剖面可分为建设型、破坏型和稳定型三种基本类型。建设型海岸分布于行水河口,等深线向海推进的距离取决于入海泥沙的堆积过程与海洋动力对泥沙的侵蚀过程两者之间的对比;破坏型海岸主要分布于停止行河不久的废弃河口附近,剖面侵蚀深度与海洋动力条件尤其是潮流流速大小密切相关;而稳定型海岸主要分布于长时间不行河的湾湾沟口附近和广利河以南岸段,前者受河海动力因素影响较小,而后者主要与莱州湾潮流流场有关。     

Sand wave deposition in the Taiwan Shoal of China

The Taiwan Shoal is the convex terrain in the southern Taiwan Strait, the largest strait in China. In 2006 and 2007, 21 samples and more than 200-km sub-bottom data as well as 80-km near shore side-scan sonar data were gotten, which gave an initial image of the boundaries of the Taiwan Shoal and revealed the internal structure of the sand waves in this area. The results showed that the major component of the sediment samples was sand, and sand waves occurred everywhere in this area, which closely followed the range of the Taiwan Shoal as we know. The western boundary of the Taiwan Shoal thus reaches the 30 m isobaths near the shore, and as a result, its area potentially covers approximately 12 800-14 770 km². The sand waves have different shapes under the complex ocean dynamics, and the height of sand waves in the near shore is usually smaller than that in the Taiwan Shoal. The number of sand waves ranged from 1-5 per kilometer, with more waves in the isobath-intensive area, suggesting the importance of topography for the formation of sand waves. The stratigraphic structure under the seabed has parallel bedding or cross bedding, and large dipping groove bedding can be seen locally in different parts, which may be the result of terrestrial deposition since the Late Pleistocene.     

K-band imaging of strong Ca ii-absorber host galaxies at z∼1

We present K -band imaging of fields around 30 strong Ca  ii absorption-line systems, at  0.7 < z < 1.2  , three of which are confirmed damped Lyman α systems. A significant excess of galaxies is found within 6.0 arcsec (≃50 kpc) from the absorber line of sight. The excess galaxies are preferentially luminous compared to the population of field galaxies. A model in which field galaxies possess a luminosity-dependent cross-section for Ca  ii absorption of the form  ( L / L *)^0.7  reproduces the observations well. The luminosity-dependent cross-section for the Ca  ii absorbers appears to be significantly stronger than the established  ( L / L *)^0.4  dependence for Mg  ii absorbers. The associated galaxies lie at large physical distances from the Ca  ii -absorbing gas; we find a mean impact parameter of 24 kpc  ( H ₀= 70 km s⁻¹ Mpc⁻¹)  . Combined with the observed number density of Ca  ii absorbers the large physical separations result in an inferred filling factor of only ∼10 per cent. The physical origin of the strong Ca  ii absorption remains unclear, possible explanations vary from very extended discs of the luminous galaxies to associated dwarf galaxy neighbours, remnants of outflows from the luminous galaxies, or tidal debris from cannibalism of smaller galaxies.     

Geostatistical evaluation of magnetic indicators of forest soil contamination with heavy metals

The goal of the study was the geostatistical evaluation of quantitative magnetic measures, which can be used for effective delineation of the extent of the area polluted with heavy metals. Several parameters of magnetic susceptibility, measured in the soil profile, were proposed as magnetic indicators of soil pollution and analyzed in detail. The following parameters were calculated: maximum magnetic susceptibility, magnetic susceptibility at the depth of 3 cm and 5 cm, and the area under the curve of magnetic susceptibility. Measurements were performed at two forested study areas, located in Upper Silesian Industrial Area (Poland). Analyses were performed using geostatistical methods, and the results were verified using dense chemical measurements. The results showed that the area under curve of magnetic susceptibility was the most effective magnetic indicator of soil contamination with heavy metals. It was possible to detect the entire polluted area, and only about 16% of the study area was assumed to be contaminated while being unpolluted. The results obtained with maximum magnetic susceptibility and magnetic susceptibility at the depth of 3 cm and 5 cm were less effective in comparison with the area under curve of magnetic susceptibility.     

青岛大沽河断裂活动性初步研究

大沽河断裂是青岛地区规模较大的一条隐伏断裂,前人对该断裂没有进行过详细的研究。由于缺乏足够的证据,无法确定该断裂的展布和产状,更加无法确定其活动性。本文首先基于地质图布设几条地球物理勘探测线,根据物探结果,选取三处异常点分别布设若干钻孔进行钻探验证。根据钻孔地层结构绘制三个联合地质剖面,剖面揭示有断裂通过,从而在土层中选取四个土样进行年代学测试。研究表明,大沽河断裂通过了地球物理勘探的三处异常点,基本确定了断裂走向;年代学测试结果表明该断裂为早更新世或中更新世早中期断裂,不属于活动断裂;根据统计规律,该断裂不会发生破坏性地震,也不会造成地表破裂,重大建设工程不需要避让该断裂。本研究具有十分重要的意义。     

陕西省榆林市秋冬季黑碳观测研究

利用2011年秋冬季榆林大气成分站黑碳浓度、颗粒物质量浓度、大气能见度、地面气象资料,计算边界层高度、气溶胶吸收系数、大气消光系数,导出单次散射反照率,并对其进行分析讨论。结果表明：（1） 榆林秋冬季平均黑碳浓度为2.6 μg·m^-3。（2）黑碳占颗粒物质量浓度PM_1.0比值为10.6%,黑碳与颗粒物质量浓度PM_1.0、PM_2.5、PM₁₀相关系数分别为0.91、0.91、0.72。（3）黑碳浓度受边界层高度影响,沙漠风场对黑碳的堆积输送起主导作用。（4） 榆林地区气溶胶吸收系数与大气消光系数比值为16.8%。（5）单次散射反照率平均值为0.72。     

二维沙丘迎风坡沙粒跃移运动的数值模拟

为了研究沙丘迎风坡面上沙粒的跃移运动,本文根据风工程和空气动力学的最新理论,给出了沙丘迎风坡面上风场的空间分布规律,在此基础上对沙粒跃移运动进行了数值计算。由于沙丘周围流场情况较为复杂,各处的风速廓线也不同,故选取不同的坡面位置进行跃移计算,其中各处的起沙率由已有的实验结果或拟合公式给出。计算结果表明：从坡脚到坡顶,平均风速加速比和摩阻风速逐渐增加,到沙丘顶部达到最大值;同时沿坡面向上,各截面处单宽输沙率和距离当地地面相同高度处输沙浓度逐渐加强,这与已有文献报道的结果吻合良好。     

Profile and Character of Atmospheric Structure Constant of Refractive Index Cn2

Random fluctuations of turbulence bring random fluctuations of the refractive index, making the atmosphere a random fluctuation medium that destroys the coherence of light-waves. Research in atmospheric turbulence is actually the investigation of the atmospheric refractive index. The atmospheric structure constant of refractive index, Cn2, is an important parameter denoting atmospheric turbulence. In this paper, Cn2 is measured during the day and at night and in all four seasons using a high sensitivity micro-thermal meter QHTP-2. The vertical profile of Cn2 in Hefei (0–30 km) is investigated by the analysis of experimental data. The average profile of Cn2 in Hefei exhibits conspicuous day and night differences with increased altitude. The distribution of log(Cn2) is nearly normal and has conspicuous seasonal differences.     

1/2000数字地面模型在高速公路勘测中的精度验证及应用

对1/2000数字地面模型DTM的高程精度进行了阐述,结合高速公路施工勘测对其进行了精度验证,并成功地应用于福建浦南高速公路施工图定测纵横断面的可靠性检查。