Effects of tillage management on infiltration and preferential flow in a black soil, Northeast China

The impacts of no-tillage (NT) and moldboard plough (MP) managements on infiltration rate and preferential flow were characterized using a combined technique of double-ring device and dye tracer on a black soil (Mollisols) in Northeast China. The objective of this study is to evaluate how tillage practices enhance soil water infiltration and preferential flow in favor of soil erosion control in the study area. The steady infiltration rates under NT management are 1.6 and 2.1 times as high as those under MP management in the 6th and 8th years of the tillage management in place, while the infiltrated water amounts under NT management are 1.4 and 2.0 times as high as those under MP management, respectively. The depth of methylene blue penetrated into NT soil increases from 43 cm in the 6th year to 57 cm in the 8th year, which are 16 cm and 19 cm deeper than those in MP soil, respectively. The results of morphologic image show that more biological macro-pores occur in NT soil than in MP soil. These macro-pores play a key role in enhancing preferential flow in NT soil, which in turn promotes water infiltration through preferential pathways in NT soil. The results are helpful to policy-making in popularizing NT and have the implications for tillage management in regard to soil erosion control in black soil region of China.     

页岩气藏清水压裂悬砂效果提升实验

针对页岩气藏压裂中清水压裂悬砂效果较差问题,分析压裂液和支撑剂性质,通过实验提出增强清水压裂悬砂效果方法:纤维复合清水压裂液技术和超低密度支撑剂技术.结果表明:纤维的加入不仅使清水压裂液的悬砂性能得到提高,同时还可以显著降低液体摩阻.低密度支撑剂可以降低沉降速度50%以上.综合采用纤维复合清水压裂液技术和超低密度支撑剂技术,支撑剂2h的沉降率为17%.不仅可以提高清水压裂的开发效果,还可以降低对地面泵车排量的要求,对于页岩气藏的开发具有指导意义.     

页岩气藏数值模拟及井底压力动态分析

为研究页岩气藏生产过程中井底压力动态及影响因素,基于质量守恒定律,考虑解吸和压力敏感系数,建立页岩气藏双孔双渗数学模型,对数学模型差分离散得到数值模型并求解;分析解吸、兰氏体积、兰氏压力、吸附时间、压力敏感系数等对井底压力双对数曲线的影响.结果表明:吸附气解吸使压降速率变缓且较晚触到边界;兰氏体积或兰氏压力越大,井底压力双对数曲线的下凹部分越明显;吸附时间常数越短,扩散效果越好,越容易达到整体径向流段;压力敏感系数越大,双对数曲线上翘越明显.该研究结果对页岩气藏开发具有指导意义.     

Design of database management system of oil shale resource evaluation based on GIS

Base on the oil shale data model,the authors analyz the four main data types and their mutual relations,grasped the focus on the oil shale data management,established UML visual demand model for oil shale resources in the field of evaluation,constructed three-tier system and developed oil shale resource evaluation database management system. The system can be used for managing oil shale data storage,enhancing the efficiency and quality of the oil shale resource evaluation.     

页岩气勘探目标层段优选

探讨了页岩气勘探目标层段优选中含气量、埋深及有机碳含量之间的互相补偿关系,并初步提出了相应的参考特征值。Ⅰ型、Ⅱ1型、Ⅱ2和Ⅲ型有机质热进入生气主峰的成熟度门限依次递降,Ro分别为1.2%、0.9%、0.7%和0.5%,相应的深度界限依次减小;对美国页岩气产层实际资料统计分析后认为,要形成工业价值的页岩气,在1 000 m、2 000 m、3 000 m深度页岩含气量至少应达到0.5 m3/t、1.0 m3/t、1.5 m3/t;根据渝东南地区下志留统龙马溪组Ⅰ型有机质页岩研究表明,要达到一定的含气量,有机碳含量与深度应互相补偿。若要含成熟有机质的页岩吸附气含量达到1.0 m3/t,则在500 m、1 000 m、2 000 m深度处TOC值需依次达到1.4%、1.1%和0.9%以上。     

骨架导电的混合泥质砂岩通用孔隙结合电阻率模型研究

在水介质中顺序添加分散粘土颗粒、油珠、导电骨架颗粒、层状泥质,并对每一种成分进行连续积分,建立了一种适用骨架导电及含有分散粘土和层状泥质的泥质砂岩通用电阻率模型.通过对该模型的影响因素分析,发现泥质分布形式对模型计算的含水饱和度有很大影响;对应两个不同粘土颗粒电阻率或骨架颗粒电阻率的地层电导率之差,几乎与总含水饱和度无关,而对应两个不同层状泥质电阻率的地层电导率之差,随总含水饱和度增大而增大;骨架胶结指数变化对地层电导率与总含水饱和度关系曲线的影响最大,而粘土胶结指数变化对地层电导率与总含水饱和度关系曲线的影响最小;饱和度指数对地层电导率与总含水饱和度关系曲线的影响随总含水饱和度的增大而减小.通过一组骨架导电的人造岩样的试验,表明当地层水电阻率.小于颗粒电阻率时,该模型可以用于不含粘土的骨架导电的岩石.通过两组分散泥质砂岩岩样实验测量数据和一组层状泥质砂岩测井资料及实际测井资料的计算,表明本文给出的电阻率模型既适用于分散泥质砂岩地层解释又适用于层状泥质砂岩地层解释,同时,还适用于含有分散粘土和层状泥质的混合泥质砂岩地层解释.     

白垩纪世界与大洋红层

白垩纪代表着地质历史中的一种极端的温室气候,已被国际地球科学界视为研究地球系统科学的典型范例。文中在评述白垩纪沉积作用、古气候、古海洋研究中取得的重要进展基础上,重点介绍推动白垩纪研究核心问题之一的黑色页岩和大洋缺氧事件以及由中国学者提出的白垩纪大洋红层和富氧作用。大洋缺氧事件与大洋红层的研究因其与碳氧循环、古气候和古海洋变化的紧密关系,已经成为国际白垩纪研究中的热点问题,并在今后一段时期内继续引领着白垩纪古海洋、古气候变化研究的不断深入。     

New Hubble Space Telescope imaging of the counterparts to six ultraluminous X-ray sources

We report the results of new Hubble Space Telescope imaging of the positions of six ultraluminous X-ray sources (ULXs). Using images in three Advanced Camera for Surveys (ACS) filters, we detect good candidate counterparts to four out of six ULXs, with one more possible detection, and observed magnitudes in the range   m ∼ 22–26  in the   F 606 W   filter. The extinction-corrected colours and absolute magnitudes vary from source to source, even after correcting for additional extinction in the host galaxy, and only one counterpart is readily explained as an OB star. Nevertheless, these counterparts are decent candidates for future follow-up in pursuit of dynamical mass constraints on the likely black holes powering these sources.