高温交联酸用稠化剂合成及性能评价

利用丙烯酰胺(AM)与2-丙烯酰胺基-2-甲基丙磺酸(AMPS)作为原料,进行水溶液聚合,采用低温复合引发体系制备高温交联酸用稠化剂P(AM-co-AMPS),通过单因素分析法确定最佳反应条件;并对其纯化样品进行红外表征,室内性能评价。结果表明,该稠化剂酸溶性好,基液黏度随稠化剂加量增加而增大,配方:20%HCl+0.8%稠化剂+5%BZ酸化缓蚀剂+2%BZ措施用破乳助排剂+2%BZ酸化用铁离子稳定剂+0.3%BZ交联延迟剂。加入交联液(交联剂/交联延迟剂=1,交联比∶100∶0.8),90 s后能形成可挑挂冻胶,180℃,170 s~(-1)剪切速率下,剪切100 min,黏度保持在56 mPa·s左右。加入破胶剂后,在90℃加热1 h,破胶黏度为10 m Pa·s,利于酸液返排,可满足高温储层对交联酸的要求,具有较好的发展前景。     

条件价值评估法在森林生态旅游非使用价值评估中范围效应的研究

条件价值评估法(CVM)是目前最受欢迎的环境资源价值评估方法之一,但同时也是争议最多的方法,争议的焦点围绕该方法的有效性和可靠性。影响CVM结果有效性的因素很多,其中范围效应是最重要因素。笔者归纳了研究CVM范围效应有关理论,并通过1个实际案例来验证CVM评估环境资源非使用价值时范围效应是否存在。研究结果表明:范围效应不是CVM普遍现象,并非由CVM方法本身的缺陷造成。     

泥岩地基及嵌岩灌注桩的承载特性试验

红土崖组(KwH)泥岩是一种分布于青岛地区的白垩系王氏群泥岩,是一种非典型的黏土岩,其透水性弱,具有一定的膨胀特性。为研究泥岩的物理力学性质、变形特性及嵌入泥岩中灌注桩的承载特性,以红土崖组(KwH)泥岩为试验对象,在青岛某地区开展了泥岩常规物理力学试验、泥岩地基及泥岩地基中嵌岩灌注桩的静载荷试验。试验结果表明,红土崖组(KwH)泥岩含砂,吸水膨胀率较小,是一种非膨胀性岩;全风化及强风化泥岩地基的P-s曲线基本呈缓变型;而中风化泥岩地基在破坏时发生了压裂及隆起,P-s曲线呈陡降型,而且变异性较大。该场地泥岩地基中灌注桩分别加载至10800 kN、12960 kN,试桩均未发生破坏,嵌岩灌注桩的桩侧摩阻力和桩端阻力均未充分发挥;中风化泥岩的承载力较高,可作为桩基理想的持力层;泥岩具有初始损伤特性,且随着应力水平的提高其损伤逐渐加剧。研究成果对青岛地区泥岩地基中的工程建设具有参考价值。     

基于运动特征的人体异常行为识别

为了提高监控视频中人体异常行为识别的实时性和准确率,提出了基于运动特征的人体异常行为识别方法。利用分块更新的背景差法从图像中提取出完整的人体轮廓,通过区域关联结合颜色直方图实现人体目标跟踪,解决了非线性运动时漏跟和误跟的问题。通过人体运动轨迹、运动姿态及运动时间3个参数,对人的5种异常行为进行分析判断。实验结果表明,所提算法不仅能实时地对人体进行检测和跟踪,还能快速、准确地识别出异常行为,具有简单实用的特点。     

Triple Medium Physical Model of Post Fracturing High-Rank Coal Reservoir in Southern Qinshui Basin

In this paper, influences on the reservoir permeability, the reservoir architecture and the fluid flow pattern caused by hydraulic fracturing are analyzed. Based on the structure and production fluid f...     

Development of liquid-nitrogen-cooling friction stir spot welding for AZ31 magnesium alloy joints

A liquid-nitrogen-cooling friction stir spot welding (C-FSSW) technology was developed for welding AZ31 magnesium alloy sheets. The liquid-nitrogen cooling degraded the deformability of the welded materials such that the width of interfacial cracks increased with increasing cooling time. The grain size of the stirred zone (SZ) and the heat-affected zone (HAZ) of the C-FSSW-welded joints decreased, whereas that of the thermomechanically affected zone (TMAZ) increased with increasing cooling time. The maximum tensile shear load of the C-FSSW-welded joints welded with a cooling time of 5 or 7 s was larger than that of the friction stir spot welding (FSSW)-welded joint, and the tensile shear load decreased with increasing cooling time. The microhardness of the C-FSSW-welded joints was greater than that of the FSSW-welded joint. Moreover, the microhardness of the SZ and the HAZ of the C-FSSW-welded joints increased, whereas that of the TMAZ decreased, with increasing cooling time.     

Role of Ppt1 in multiple stress responses in Candida albicans

To study the function of CaPptl, we deleted PPT1 gene from the Candida albicans genome by sequentially replacing the entire coding region with the selectable markers ARG4 and HIS1. The results showed that the deletion of Pptl did not affect the hyphal formation of C. albicans under serum induction and caused enhanced sensitivity to DNA damage, Calcofluor white and salt- induced stress. We also found that Pptl was not required for the phenotypic response of cells treated with the genotoxins, methylmethane sulfonate and hydroxyurea. Flow cytometric analyses indicated that pptlA cells and wild-type cells showed similar G2/M arrest profiles when exposed to DNA damage stress. Pptl was not required for the activation of the DNA damage response pathway, as indicated by normal phosphorylation of Rad53 and Rfa2 in pptlA cells under DNA damage stress. We suggest that Pptl plays important roles in response to various stress conditions in C. albicans.     

初弯曲对钢框架的受力性能的影响分析

建立了考虑构件初弯曲的单层单跨钢框架计算模型,对不同初弯曲度下结构的位移、内力进行一阶和二阶分析,得出构件初弯曲对钢框架受力性能影响的一般性规律．     

The suppression of star formation by powerful active galactic nuclei

The old, red stars that constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at remarkable rates and active galactic nuclei (AGN) shone brightly as a result of accretion onto black holes. It is widely suspected, but unproved, that the tight correlation between the mass of the black hole and the mass of the stellar bulge results from the AGN quenching the surrounding star formation as it approaches its peak luminosity. X-rays trace emission from AGN unambiguously, whereas powerful star-forming galaxies are usually dust-obscured and are brightest at infrared and submillimetre wavelengths. Here we report submillimetre and X-ray observations that show that rapid star formation was common in the host galaxies of AGN when the Universe was 2-6 billion years old, but that the most vigorous star formation is not observed around black holes above an X-ray luminosity of 10(44) ergs per second. This suppression of star formation in the host galaxy of a powerful AGN is a key prediction of models in which the AGN drives an outflow, expelling the interstellar medium of its host and transforming the galaxy's properties in a brief period of cosmic time.