Land use and land cover change in Liaocheng Prefecture of China

1 Introduction1.1 Introduction to Liaocheng PrefectureLiaocheng Prefecture lies in northwest of Shandong Province and slightly north to the center of the Huang-Huai-Hai Plain with latitudes between 35(47'N and 37(02'N and longitudes between 115(16'E and 116(32'E. Administratively, it consists of two cities (Liaocheng and Linqing) and six counties (Yanggu, Shenxian, Chiping, Dong'e, Guanxian and Gaotang). It covers a total area of 8590 km2 with a maximum distance of 114 km from eas…     

长江中下游岸线资源的特征及其开发利用

运用大比例尺水下地形图，在岸线资源总量勘查的基础上，评价了长江中下游干流岸线的水深条件、岸线稳定性条件和建港自然条件，分析了本区域岸线资源的基本特征，提出了长江岸线资源开发的基本原则和中下游干流岸线利用建议。     

南太行——中条山植物区系地理研究

南太行—中条山地区是中国种子植物区系研究薄弱地区之一。本区约有种子植物1627种,隶属618属142科。通过该区种子植物各类地理成分分析及与相关地区的比较,得出:本地区植物区系具有温带区系特点,又具有温带向亚热带区系过渡性质,是华北植物区系分区南部亚区的一条重要界线。该地区存在许多古老及残遗植物,表明该区系起源古老,同时也是产生新分化的中心之一。     

2010—2015年中东北非政局变动中的“政治性民意势力”及其影响

援引批判地缘政治学话语权和地缘政治想象分析方法,在对“民意”“政治性民意”“政治性民意势力”内涵界定的基础上,分析了2010—2015年中东北非地区相关国家政局变动中“政治性民意势力”的形成背景、过程及其影响。结果表明：中东北非国家“政治性民意势力”的形成有着深厚的国内背景和复杂的国际背景;“政治性民意势力”的形成经历了从民意事件客体的呈现,到民众聚集并上升为政治性议题,再到国内外势力借力博弈形成挑动抗议、推动政变的政治力量的过程;“政治性民意势力”形成以后,多行为体借力博弈下,在国别、区域上呈现不同的扩散轨迹和规律;“政治性民意势力”一方面造成了中东北非相关国家的政局变换,另一方面则推动区域地缘政治格局的变迁。这是对民意事件的地缘政治理论解读和分析,是一次较为有意义的尝试。     

义县组时代及解体

辽西中生界义县组时代归属问题 ,争论已久 ,归纳起来主要有三种划分方案 :第一 ,隶属于侏罗纪 ;第二 ,隶属于白垩纪 ;第三 ,归属于为侏罗 -白垩纪 ,属跨纪地层。结合多年来各科研院所及生产单位采集的众多同位素年龄资料的分析及野外所见接触关系研究认为 :原义县组中下部层位岩性组合 ,根据其特征 ,需另建立组级岩石单位 ,应归属到上侏罗统 ,广义义县组上部层位一套岩性组合 ,需重新定义 ,时代应归属到下白垩统。     

地理信息系统技术在区域城镇发展用地评价中的应用——以海南省为例

区域城镇发展用地评价是区域经济开发的先行步骤。作者利用地理信息系统的技术,建立地形评价模型、基础设施辐射范围扩散模型、分区多幅图覆盖分析模型等一整套模型,使评价工作较以往更为科学、系统,且省时省力。本文研究了海南省城镇发展用地条件。     

A search for the 53-MHz OH line near G48.4−1.4 using the National MST Radar Facility

We present the results of a search for the ground-state hyperfine transition of the OH radical near 53 MHz using the National Mesosphere–Stratosphere–Troposphere (MST) Radar Facility at Gadanki, India. The observed position was G48.4−1.4 near the Galactic plane. The OH line is not detected. We place a 3σ upper limit for the line flux density at 39 Jy from our observations. We also did not detect recombination lines (RLs) of carbon, which were within the frequency range of our observations. The 3σ upper limit of 20 Jy obtained for the flux density of carbon RLs, along with observations at 34.5 and 327 MHz, are used to constrain the physical properties of the line-forming region. Our upper limit is consistent with the line emission expected from a partially ionized region with electron temperature, density and path lengths in the range 20–300 K, 0.03–0.3 cm⁻³ and 0.1–170 pc, respectively.     

Red companions to a z=2.15 radio-loud quasar

We have conducted observations of the environment around the z =2.15 radio-loud quasar 1550–269 in search of distant galaxies associated either with it or the z =2.09 C  iv absorber along its line of sight. Such objects will be distinguished by their red colours, R − K >4.5. We find five such objects in a 1.5 arcmin² field around the quasar, with typical K ' magnitudes of ∼20.4 and no detected R -band emission. We also find a sixth object with K =19.6±0.3, and undetected at R , just two arcsec from the quasar. The nature of all these objects is currently unclear, and will remain so until we have determined their redshifts. We suggest that it is likely that they are associated with either the quasar or the C  iv absorber, in which case their properties might be similar to those of the z =2.38 red Ly α emitting galaxies discovered by Francis et al. The small separation between the quasar and the brightest of our objects suggests that it may be the galaxy responsible for the C  iv metal line absorption system. The closeness to the quasar and the red colour might have precluded similar objects from being uncovered in previous searches for emission from C  iv and damped absorbers.     

枣庄南部岩溶塌陷风险预测及评估

枣庄南部岩溶塌陷发育,严重制约着当地经济的发展,并对居民生产、生活构成威胁。通过对影响岩溶塌陷的各要素进行系统的调查,结合当地社会经济发展资料,采用信息预测的方法,对枣庄南部岩溶塌陷进行风险预测及评估,并对不同地段的岩溶塌陷风险等级进行划分,从而为枣庄市地下水资源合理开发利用、环境治理、保护与规划提供了决策依据。     

Linear polarization of precataclysmic variables

The optical linear polarization of three precataclysmic variables was measured in B and R. A noticeable polarization was detected only in BD +50°2869. In the other two cases, the polarization is probably interstellar in origin.