伊拉克A油田白垩系孔隙型生屑灰岩高渗透层成因及分布特征

伊拉克A油田白垩系孔隙型碳酸盐岩高渗透储层具有分布普遍、类型复杂、成因多样等特征。岩石类型主要为泥晶生屑砂屑灰岩、亮晶生屑砂屑灰岩及泥晶生屑灰岩;生物扰动加剧了碳酸盐岩储层非均质性,导致高渗透储层在全油田广泛分布。通过岩心观察、常规薄片和铸体薄片的观察和测量,孔隙度、渗透率和毛管压力的测定,综合区域地质研究成果,发现高渗层的形成受层序演化、次级相对海平面变化、沉积环境、硬底形成、生物扰动及(准)同生期暴露淋滤等复杂多因素共同控制。高渗透储层形成模式表现为Khasib组沉积时期为晚高位域期,在Kh2-1-2L段上部沉积过程中,发生首次次级相对海平面下降,形成沉积间断。沉积间断期间硬底和区域规模性的生物扰动同时发育,在Kh2-1-2L段硬底尚未被胶结的相对疏松的基质中掘穴,形成厚几十厘米、迂曲状互相贯通的生物扰动通道。沉积间断结束后,在晚期高位域层序背景下,次级相对海平面上升,松散生屑砂屑充填扰动通道。由于沉积物堆积速率较快,限制了胶结作用的发生,使扰动通道内充填物能够发育连通性好的粒间孔,而后次级相对海平面再次下降,发生(准)同生期暴露淋滤。由于扰动部位连通性好,成为溶蚀流体优势通道,导致沿扰动部位发育溶孔及扩溶缝,形成了“粒间孔+溶孔+溶缝”高渗透网络。A油田高渗透储层物性表现出发育强烈生物扰动的部位具有明显高渗特征,其孔喉较粗,排驱压力低,孔喉配位数高、连通性好。高渗层全区稳定发育,由西至东厚度逐渐增大,高渗层的分布对油田单井产量、含水上升和油田采出程度影响较大。     

陡坡寺中微风化料的大型三轴试验研究

随着西部山区的基础设施建设进入迅速发展的阶段,越来越多的高填方工程正在或将要兴建,而对填料力学性质的认识也就成为决定这些高填方工程安全性的重要因素。通过一系列大型三轴试验,对分布于云南等地的陡坡寺中微风化料的剪切力学特性进行了研究。结果表明,陡坡寺中微风化料与典型堆石料的力学特性有很大不同,其强度较低,并且应力-应变关系、强度和刚度等特征都比较接近于细粒土。另外,水对陡坡寺中微风化料的力学特性有着显著的影响,其遇水后强度大为降低,因此,在设计和施工中必须予以充分考虑。对试验数据的拟合表明,邓肯-张模型能较好地模拟陡坡寺中微风化料在不同围压下的应力-应变关系。     

关于A型花岗岩判别过程中若干问题的讨论

自A型花岗岩提出(1979年)30年来,其内涵和外延相对于原始定义而言已发生了很大的变化.主要针对A型花岗岩的各种判别方法(尤其是判别图解)的有效性和局限性进行了讨论.这些判别方法对于A型花岗岩的判定并不总是奏效,所以在实践过程中不能过于依赖判别图解,否则就很容易得出错误的结论.实际上,A型花岗岩最本质的特征很可能在于它是一种高温花岗岩(相时于I型争S型花岗岩),因此较高地温梯度下的各种地球动力学背景均有利于这一类型花岗岩的发育.     

水杨酸对蛋白核小球藻(Chlorella pyrenoidosa) 生长及抗逆相关基因的影响

以蛋白核小球藻(Chlorella pyrenoidosa)为研究对象, 首先克隆了热激蛋白70(HSP70)和磷 酸甘油酸激酶(PGK)基因全长序列, 然后研究了0-20μg/mL 水杨酸对高温胁迫下HSP70 和PGK 基 因表达, 以及蛋白核小球藻生长、可溶性糖和蛋白含量的影响。结果获得了蛋白核小球藻HSP70 基 因的cDNA 序列2405 bp, 包括60 bp 的5'-非编码区(UTR)、1959 bp 的开放阅读框(ORF)和386 bp 的3'-UTR 和PGK 基因的cDNA 序列1664 bp, 包括35 bp 的5'-UTR, 1398 bp ORF 和231 bp 3'-UTR. 序列比较和分析表明该蛋白核小球藻HSP70 序列与其它绿藻的同源性高达83%-91%, PGK 为 70%-75%.荧光定量PCR 结果显示随着水杨酸浓度的增加, HSP70 和PGK 的表达量在12h 和24h 均有所增加, 而在10 μg/mL 水杨酸浓度下表达量最大, 12h 时分别为对照组的2.57 倍和1.56 倍, 24h 则为1.71 倍和1.79 倍。1-20μg/mL 水杨酸可促进该藻的比生长速率、可溶性糖和蛋白含量的升高。 本文结果表明一定浓度水杨酸对高温胁迫蛋白核小球藻有缓解作用, 且5 和10 μg/mL 水杨酸的效果 最显著。     

增强型AlGaN/GaN高电子迁移率晶体管高温退火研究

深入研究了两种增强型AlGaN/GaN高电子迁移率晶体管(HEMT)高温退火前后的直流特性变化.槽栅增强型AlGaN/GaN HEMT在500 ℃ N₂中退火5 min后,阈值电压由0.12 V正向移动到0.57 V,器件Schottky反向栅漏电流减小一个数量级.F注入增强型AlGaN/GaN HEMT在 400 ℃ N₂中退火2 min后,器件阈值电压由0.23 V负向移动到-0.69 V,栅泄漏电流明显增大.槽栅增强型器件退火过程中Schottky有效势垒     

基于一维综合孔径微波辐射计的海面温度反演研究

Due to the low spatial resolution of sea surface temperature(T_S) retrieval by real aperture microwave radiometers,in this study, an iterative retrieval method that minimizes the differences between brightness temperature(T_B)measured and modeled was used to retrieve sea surface temperature with a one-dimensional synthetic aperture microwave radiometer, temporarily named 1 D-SAMR. Regarding the configuration of the radiometer, an angular resolution of 0.43° was reached by theoretical calculation. Experiments on sea surface temperature retrieval were carried out with ideal parameters; the results show that the main factors affecting the retrieval accuracy of sea surface temperature are the accuracy of radiometer calibration and the precision of auxiliary geophysical parameters. In the case of no auxiliary parameter errors, the greatest error in retrieved sea surface temperature is obtained at low T_S scene(i.e., 0.710 6 K for the incidence angle of 35° under the radiometer calibration accuracy of0.5 K). While errors on auxiliary parameters are assumed to follow a Gaussian distribution, the greatest error on retrieved sea surface temperature was 1.330 5 K at an incidence angle of 65° in poorly known sea surface wind speed(W)(the error on W of 1.0 m/s) over high W scene, for the radiometer calibration accuracy of 0.5 K.     

An Explicit Symplectic Integrator for Cometary Orbits

A new symplectic algorithm is developed for cometary orbit integrations. The integrator can handle both high-eccentricity orbits and close encounters with planets. The method is based on time transformations for Hamiltonians separated into Keplerian and perturbation parts. The adaptive time-step of this algorithm depends on the distance from a centre and the magnitude of perturbations. The explicit leapfrog technique is simple and efficient.     

福州盆地及其周围地区地壳深部结构与构造的初步研究

1986—1988年,福建省地震局在福州盆地及其周围地区完成了五条地震测深剖面:宁德—永春剖面;洪懒—宁德剖面;莲峰—福州（尚干）剖面;南平—永泰—平潭非纵剖面;并在宁德—古田—嵩口首次试验扇形剖面观测系统,结果表明,扇形剖面对确定断裂是有效的. 根据对地震波走时的正、反演计算,用理论地震图和射线追踪方法进一步修改和完善,得到了福州盆地及其周围地区地壳深部为高、低速相间的速度分布特征.地壳介质速度为6.40km/s,在中地壳普遍发育一层速度为5.80—5.90 km/s、厚度约5.0 km的低速层.Moho面深度30—33 km,福州盆地为一Moho面隆起区,隆起幅度达3.0 km.北西向断裂发育,其中,闽江断裂在纵剖面和扇形剖面均有明显的反映,并切割到Moho面2.0—3.0 km. 反射波谱频方法计算得到福州盆地地壳Q值仅120—150,比邻近地区明显偏低,中地壳低速层Q值为40—80,是一典型的低速—高导—低Q（高衰减）结构层,此层上界面埋深14—15 km,与居里面埋深较一致.这些结果为福州地区的地热资源远景预测和开发提供了地壳深部结构和某些地球物理场背景.     

Unveiling the chemistry of hot protostellar cores with ALMA

High angular resolution mm-wave observations of the Orion-KL region, made with the IRAM Plateau de Bure interferometer (PdBI), reveal the presence of several cores of size 10³ AU, which have distinct spectral signatures. Complex molecules such as ethanol, vinyl cyanide and dimethyl ether show different distributions and their relative abundance varies from core to core by orders of magnitude. The molecular column densities derived in the cores also differ widely from the beam-averaged column densities observed with large single-dish telescopes. Obviously, the predictions of hot core chemistry models must be checked against high resolution observations. ALMA, which allies sensitivity and high angular resolution, will be a key instrument for this type of studies. The PdBI observations were part of a search for interstellar glycine, also carried out with the IRAM 30-m telescope and the Green Bank Telescope. We derive a 3σ upper limit on the column density of glycine of 1×10¹⁵ cm⁻² per 2″×3″ beam in the Orion Hot Core and Compact Ridge. Based on observations made with the IRAM PdB Interferometer, the IRAM 30-m telescope and the NRAO Green-Bank telescope. IRAM is supported by CNRS, MPG and IGN.