兰州市主城区房价分异及驱动因素研究

以2021年兰州市主城区678个居住小区房价数据为基础,引入地理场模型量化影响房价的外部因素,通过空间自相关分析、多尺度地理加权回归等模型对房价分异的空间格局及驱动因素的作用机理、带宽差异展开研究,以期为推动河谷型城市房产市场的公平发展提供参考。结果表明:(1)兰州市主城区平均房价为13739元·m^-2,空间上呈现“一主三副”的带状多中心组团式分布格局,房价由多中心向四周递减,价格相似的小区在地理空间上邻近分布,具有“小集中、大分散”的局部空间特征。(2)房价分异是多种驱动因素共同作用的结果,区位特征中的主商圈对房价的影响居于首位,建筑特征中的房龄、容积率和邻里特征中的中学数量、绿化率等对房价的影响较大,城市地理特征对房价具有显著影响,愈靠近黄河的小区、房价越高。(3)各驱动因素的带宽差异明显,主商圈、医院等小尺度变量存在高度空间异质性,而容积率、黄河等全局变量基本不存在空间异质性。     

地基SAR在滑坡形变监测中的应用

地基InSAR是近年发展起来的基于地基SAR(GB-SAR)获取地表形变的一种新的技术手段,分辨率高、可实时监测,实现毫米级形变监测精度,为近距离滑坡实时监测与预警提供了先进的技术手段。本文首先以澜沧江某滑坡体为研究对象,在滑坡体对岸设立固定站点,按固定频率进行GB-SAR数据采集;然后通过先后两景影像形成干涉对,利用相干阈值方法提取相干点目标;最后利用形变模型提取滑坡体形变结果。研究表明,地基SAR可获得整个滑体形变边界、形变大小空间分布及时间变化历程,对滑坡体灾害实时监测非常有效,可为滑坡灾害监测及预警提供参考。     

尼泊尔地震的NOAA卫星数据震前异常分析

发生地震时常伴随有地热辐射增强现象,这些异常信息隐藏于遥感卫星NOAA所捕获的地球射出长波辐射（OLR）数据中,目前多数研究还停留在对源数据的解读,缺乏有效的信息处理技术,致使大部分的OLR数据没有得到充分利用。因此,本文提出一种基于鞅理论的概率统计方法来识别异常特征算法,从有噪声的非结构化的源数据中提取出震前OLR数据异常变化特征序列,从时间序列和地域范围进行震前异常分析。本算法实验是以尼泊尔的在2014年9月至2015年7月期间（包括2015年4月25日Ms7.8大地震）发生的3次地震的OLR数据为例,实验结果显示震中区域的OLR数据在震前的2~3个月开始有显著的异常数据变化,通过分析发现数据显示数据异常在震前出现的时间长短与地震的大小相关,异常的发生区域与震区周围的地貌特征相关。这说明基于鞅理论的算法所提取的OLR数据异常点序列的确与地震发生的时间地点是有关系的。     

珠江口淇澳岛滨海湿地沉积环境演化及其对人类活动的响应

滨海湿地作为人类活动和全球变化反应最为敏感的区域,其沉积记录可以反映出周边地区环境变化及人类活动信息。珠江口淇澳岛滨海湿地钻孔分析结果表明,在中全新世期间淇澳岛附近海域为河口湾环境,在风化层以上开始出现淤积,但在4 200 a BP前后受极冷气候的影响,沉积物粗化;自2 500 a BP以来,沉积环境相对稳定,在小冰期期间略有变化。沉积速率计算结果显示:淇澳岛附近海域自中全新世高海面以来的平均沉积速率为0.29 cm/a,4 160~2 500 a BP、2 500 a BP-1488年、1488-1893年、1893-1986年、1990-2007年期间的平均沉积速率分别为:0.17 cm/a、0.23 cm/a、0.35 cm/a、1.37 cm/a和5.94 cm/a,沉积速率逐渐增大,反映了珠江三角洲演化过程中沉积相与沉积环境的变化;1986-1990年期间的海堤建造极大地扰动了该钻孔上部的沉积过程,在工程施工期间共沉积了厚度约112 cm的沉积层,而在海堤建成后,沉积速率也显著增大。沉积物总有机碳、总氮和C/N值的垂向分布表明,在4 160~2 500 a BP期间受海洋环境影响较大,沉积物中有机碳以海源为主,2 500 a BP以来沉积物中碳、氮含量明显增大,C/N也相应变大,有机碳主要来源于陆源输入,但在小冰期期间海源有机碳贡献略有所增大;近百年来由于受人类活动影响显著,陆源有机碳的贡献快速增加。     

基于地学信息图谱的河道、海岸线演变对黄河三角洲景观格局影响研究

本文利用1988、1998、2009和2016年四期遥感影像,运用GIS技术,将地学信息图谱的图形思维与景观生态学的定量思维相结合,以距今不同时期的亚三角洲和滨海湿地为研究区,从景观结构和景观演替两个方面探究黄河三角洲河道、海岸线演变对景观格局的影响。结果表明:(1)距今不同时间的河道对黄河三角洲景观结构的影响程度不同,距今时间越长的亚三角洲研究区内耕地占总面积的比例越大且耕地是亚三角洲研究区中的第一优势景观类型。在1855—1889亚三角洲研究区内,除耕地和建筑用地外,其他各类景观占总面积的比例都较小且随时间变化不明显;在1929—1934亚三角洲研究区内,盐田、养殖池占总面积的比例从2009年到2016年增加了近40%,涨幅明显;在1964—1976亚三角洲研究区内,各类景观占总面积的比例趋于平均;在2017至今的亚三角洲研究区内,耕地和光滩占总面积的比例较高,达到24%左右。(2)距今不同时间的海岸线对黄河三角洲景观结构的影响程度也不同,在1855滨海湿地研究区内,耕地占总面积比例为60%左右,而海域占总面积比例接近于0,极差较大;在1934和1974滨海湿地研究区内,光滩、柽柳、碱蓬群落、芦苇、白茅群落占总面积比例随时间变化几乎呈逐渐下降趋势,而建筑用地和盐田、养殖池则呈逐渐上升趋势;2009滨海湿地研究区,河流、人工水域占总面积比例在2009年和2016年均达到32%以上。(3)根据景观类型重心变化特征,分析河道、海岸线演变对景观演替的影响程度,将不同时期亚三角洲和滨海湿地研究区景观演替分为如下几类:亚三角洲人类活动主导型、废弃河道主导型、行水河道主导型、滨海湿地人类活动主导型、废弃海岸主导型、新海岸主导型。     

Bearing capacity of offshore umbrella suction anchor foundation in silty soil under varying loading modes

Considering the current disadvantages of present offshore wind turbine foundations, a novel anchor foundation with skirt and branches is proposed, called offshore umbrella suction anchor foundation (USAF). A series of experiments and numerical simulations were performed to explore the bearing capacity of the USAF under various kinds of loading modes. The bearing characteristics and the anchor–soil interactions are described in detail for horizontal static loading, horizontal cyclic loading, and an antidrawing (pullout) test in silty soil. In the static loading test, the load–deflection of the anchor under step loading was analyzed and the normalized curve of the load–deflection was obtained to determine the ultimate horizontal bearing capacity of the anchor under normal working conditions. Under horizontal cyclic loading, the relationship between the plastic cumulative deformation and cyclic number was determined. In addition, the responses of USAF were investigated for a low wave frequency and storm surges. In the drawing test, it was found that a “segmentation phenomenon” occurred during the test. Moreover, a method to identify the maximum antidrawing load of USAF was provided based on dynamic mechanics. The numerical results show that the use of anchor branches and skirt can enhance the bearing performance of USAF to a certain degree. However, the anchor branch has a slight positive influence on the bearing performance improvement. The USAF is not only similar to a stiff short pile, but a rotation occurs. The failure envelope under composite loading (V-M) was obtained and the changes associated with changes in the aspect ratio of the internal compartment were clarified.     

脐带缆螺旋滑移分析及力学性能研究

针对脐带缆内部螺旋层,应用Darboux标架建立螺旋结构空间坐标系,推导弯曲载荷下螺旋结构的局部变形和滑移。考虑螺旋构件间的接触和摩擦作用,建立螺旋结构的受力平衡偏微分方程,并研究螺旋角和摩擦系数对螺旋结构滑移的影响。基于同层螺旋结构本构关系相同假设,将所有螺旋结构力学性能线性叠加,拟合脐带缆整体弯曲刚度。运用建立的理论解析方法,对某双层铠装脐带缆的力学性能进行研究,并与数值模拟结果进行对比验证。对比结果表明,理论解析得到的螺旋滑移结果与数值模拟结果一致,理论解析得到的脐带缆弯曲刚度与数值模拟结果在全滑动阶段比较接近。     

An algorithm to resolve γ-rays from charged cosmic rays with DAMPE

The DArk Matter Particle Explorer(DAMPE),also known as Wukong in China,which was launched on 2015 December 17,is a new high energy cosmic ray and γ-ray satellite-borne observatory.One of the main scientific goals of DAMPE is to observe Ge V-Te V high energy γ-rays with accurate energy,angular and time resolution,to indirectly search for dark matter particles and for the study of high energy astrophysics. Due to the comparatively higher fluxes of charged cosmic rays with respect to γ-rays,it is challenging to identify γ-rays with sufficiently high efficiency,minimizing the amount of charged cosmic ray contamination. In this work we present a method to identify γ-rays in DAMPE data based on Monte Carlo simulations,using the powerful electromagnetic/hadronic shower discrimination provided by the calorimeter and the veto detection of charged particles provided by the plastic scintillation detector. Monte Carlo simulations show that after this selection the number of electrons and protons that contaminate the selected γ-ray events at～10 Ge V amounts to less than 1% of the selected sample.Finally,we use flight data to verify the effectiveness of the method by highlighting known γ-ray sources in the sky and by reconstructing preliminary light curves of the Geminga pulsar.     

Binary Star Fractions from the LAMOST DR4

Stellar systems composed of single, double, triple or higher-order systems are rightfully regarded as the fundamental building blocks of the Milky Way. Binary stars play an important role in formation and evolution of the Galaxy. Through comparing the radial velocity variations from multiepoch observations, we analyze the binary fraction of dwarf stars observed with LAMOST. Effects of different model assumptions, such as orbital period distributions on the estimate of binary fractions,are investigated. The results based on log-normal distribution of orbital periods reproduce the previous complete analyses better than the power-law distribution. We find that the binary fraction increases with Teff and decreases with [Fe/H]. We first investigate the relation between α-elements and binary fraction in such a large sample as provided by LAMOST. The old stars with high [α/Fe] dominate with a higher binary fraction than young stars with low [α/Fe]. At the same mass, earlier forming stars possess a higher binary fraction than newly forming ones, which may be related with evolution of the Galaxy.     

Seismogenic Structures of the 2006 ML4.0 Dangan Island Earthquake Offshore Hong Kong

The northern margin of the South China Sea, as a typical extensional continental margin, has relatively strong intraplate seismicity. Compared with the active zones of Nanao Island, Yangjiang, and Heyuan, seismicity in the Pearl River Estuary is relatively low. However, a ML4.0 earthquake in 2006 occurred near Dangan Island(DI) offshore Hong Kong, and this site was adjacent to the source of the historical M5.8 earthquake in 1874. To reveal the seismogenic mechanism of intraplate earthquakes in DI, we systematically analyzed the structural characteristics in the source area of the 2006 DI earthquake using integrated 24-channel seismic profiles, onshore–offshore wide-angle seismic tomography, and natural earthquake parameters. We ascertained the locations of NW-and NE-trending faults in the DI sea and found that the NE-trending DI fault mainly dipped southeast at a high angle and cut through the crust with an obvious low-velocity anomaly. The NW-trending fault dipped southwest with a similar high angle. The 2006 DI earthquake was adjacent to the intersection of the NE-and NW-trending faults, which suggested that the intersection of the two faults with different strikes could provide a favorable condition for the generation and triggering of intraplate earthquakes. Crustal velocity model showed that the high-velocity anomaly was imaged in the west of DI, but a distinct entity with low-velocity anomaly in the upper crust and high-velocity anomaly in the lower crust was found in the south of DI. Both the 1874 and 2006 DI earthquakes occurred along the edge of the distinct entity. Two vertical cross-sections nearly perpendicular to the strikes of the intersecting faults revealed good spatial correlations between the 2006 DI earthquake and the low to high speed transition in the distinct entity. This result indicated that the transitional zone might be a weakly structural body that can store strain energy and release it as a brittle failure, resulting in an earthquake-prone area.