基于年龄测试的黄庄—高丽营断裂活动性研究

黄庄—高丽营断裂是北京平原区一条重要的活动断裂,在庙城—高丽营段沿线发生地裂缝,造成大量房屋墙体开裂和道路破坏。在西王路村探槽揭示该断裂错断第四系地层,产生地表地裂缝。探糟断裂孢粉年龄测试,该断裂发生年龄大致在13～22ka,仍处于活动状态。     

全球变化背景下北方泥炭地释放溶解有机碳的驱动机制

泥炭地（peatland）是一类储碳效率很高的特殊陆地生态系统,其碳储量约占全球土壤碳库的近1／3,对全球碳循环有着举足轻重的作用。有证据表明在过去20余年,北半球大范围的天然水体中溶解有机碳的浓度呈显著增升趋势。普遍认为与全球变化背景下北方泥炭地大规模释放溶解有机碳有关,但其驱动机制尚不十分清楚。已经提出的具有代表性...     

储层砂岩声波速度预测

本文主要基于Ｇａｓｓｍａｎｎ方程和经验规律，提出了孔隙流体替代和孔隙度改变时对砂央地震波速度变化的估计，以及直接利用岩石矿物和孔隙流体的弹性性质计算砂岩地震波速度方法，利用已知的岩芯，测井或地震数据，运用这此方法，可合理地对储层砂岩地震波速度进行预测。     

巴林左旗-阿鲁科尔沁旗5.9级地震余震序列精确定位及分布特征

2003年8月16日内蒙古巴林左旗与阿鲁科尔沁旗间发生5．9级地震，使内蒙古东部地震活动再次进入活跃阶段。通过对巴林左旗-阿鲁科尔沁旗5．9级地震余震序列分析表明，序列的空间位置变化不太大，集中发生在较小的区域内，说明该震震源体较小。整个余震序列以NWW向条带分布为主，条带的走向与宏观烈度等值线长轴方向及震源机制B节面方向一致。ML≥3．0余震形成NW和NE两条相互垂直的条带，主震发生在NW条带的北西端。分析余震序列深度剖面图，说明NW向可能为此次地震的主破裂方向。     

Developing an Advanced Automated Method for Solar Filament Recognition and Its Scientific Application to a Solar Cycle of MLSO Hα Data

We developed a method to automatically detect and trace solar filaments in Hα full-disk images. The program is able not only to recognize filaments and determine their properties, such as the position, the area, the spine, and other relevant parameters, but also to trace the daily evolution of the filaments. The program consists of three steps: First, preprocessing is applied to correct the original images; second, the Canny edge-detection method is used to detect filaments; third, filament properties are recognized through morphological operators. To test the algorithm, we successfully applied it to observations from the Mauna Loa Solar Observatory (MLSO). We analyzed Hα images obtained by the MLSO from 1998 to 2009 and obtained a butterfly diagram of filaments. This shows that the latitudinal migration of solar filaments has three trends in Solar Cycle 23: The drift velocity was fast from 1998 to the solar maximum, after which it became relatively slow. After 2006, the migration became divergent, signifying the solar minimum. About 60 % of the filaments with latitudes higher than 50^° migrate toward the polar regions with relatively high velocities, and the latitudinal migrating speeds in the northern and the southern hemispheres do not differ significantly in Solar Cycle 23.     

Puzzling Origin of CEMP-r/s Stars: An Interpretation of Abundance and Enrichment of s- and r-Process Elements from Asymptotic Giant Branch Supernovae

CEMP-r/s stars at low metallicity are known as double-enhanced stars that show enhancements of both r-process and s-process elements. The chemical abundances of these very metal-poor stars provide us a lot of information for putting new restraints on models of neutron-capture processes. In this article, we put forward an accreted scenario in which the double enrichment of r-process and s-process elements is caused by a former intermediate-mass Asymptotic Giant Branch (AGB) companion in a detached binary system. As the AGB superwind is only present at the ultimate phase of AGB stars, there is thus a lot of potential that the degenerate-core mass of an intermediate-mass AGB star reaches the Chandrasekhar limit before the AGB superwind. In these circumstances, both s-process elements produced in the AGB shell and r-process elements synthesized in the subsequent explosion would be sprayed contemporaneously and accreted by its companion. Despite similarity to physical conditions of a core-collapse supernova, a major focus in this scenario is the degenerate C–O core surrounded by an envelope of a former intermediate-mass AGB donor that may collapse and explode. Due to the existence of an outer envelope, r-process nucleosynthesis is expected to occur. Hypothesizing the material-rich europium (Eu) accreted by the secondary via the wind from the supernova to be in proportion to the geometric fraction of the companion with respect to the exploding donor star, we find that the estimated yield of Eu (as representative of r-process elements) per AGB supernova event is about 1 × 10^?9 M _⊙ ～ 5 × 10^?9 M _⊙. Using the yields of Eu, the overabundance of r-process elements in CEMP-r/s stars can be accounted for. The calculated results show that the value of parameter f , standing for efficiency of wind pollution from the AGB supernova, will reach about 10⁴, which means that the enhanced factor is much larger than unity due to the impact of gravity of the donor and the result of the gravitational focusing effect of the companion.     

土壤生态质量地球化学综合评价初探——以“贵阳市地区多目标区域地球化学调查”成果为例

多目标区域地球化学调查,是针对第四纪覆盖区开展的以基础地质、资源潜力与生态环境等为主要内容的基础性、公益性调查与评价工作,其成果可广泛服务于资源、农业、生态及城市规划等多领域.本文在介绍多目标区域地球化学调查产生的时代背景、工作方法及全国多目标调查取得的主要成果基础上,提出了土壤生态地球化学评价的评价方法和思路,该评价结果可以为贵阳市地区土地资源宏观分等定级提供充分依据.     

虎头崖铅锌多金属矿床矿体三维空间变化结构及分布规律

文章利用Vulcan和Datamine三维可视化软件建立了虎头崖铅锌多金属矿床矿体的三维实体模型、块体模型及地层三维实体模型;运用地质统计学方法分析了虎头崖矿区67线以东和117线以西矿体的Pb,Zn品位空间变化结构,得出搜索椭球体,实现了虎头崖铅锌多金属矿床矿体、地层形态和铅锌品位变化形态的空间分布展示;结合三维建模结果和铅锌矿体空间变化结构,总结出矿体空间分布规律,并用三维可视化软件对矿体分布规律进行显示,指导隐伏矿体的预测,寻找有利的找矿部位。