张掖-民乐盆地地质构造特征与张掖市地热资源开发可行性分析

张掖—民乐盆地是受南北两侧右行走滑逆冲断裂控制形成的拉分盆地。在以往石油勘探中已发现在地下1 600～1 900m间有热储层存在,温度可达56℃～59℃。通过以往石油勘探和水文地质调查成果分析,祁连山北缘断裂和盆地内NNW向断裂构造较为发育,十分有利于热流的聚集与运移,认为张掖市所在的张掖—民乐盆地具备地热资源形成的储、盖、通、源条件,属中低温盆地传导型地热资源,具有经济开发价值。     

The Late-Quaternary deposits of the middle Dyfi Valley,Wales

The surficial deposits and landforms of the middle Dyfi Valley, Wales, are examined and a sequence of glacial, glacio-fluvial and glacio-lacustrine sediments is identified. This is considered to relate to a late stage in the wastage of the Late-Devensian Merioneth ice-cap. A sequence of terrace gravels overlying the giacigenic succession represents dissection during early Flandrian times.     

中国石油精细油藏描述进展与展望

结合研究实践,将中国石油精细油藏描述研究进展总结为基于开发地震技术的复杂构造精细研究、潜山复杂岩性识别技术、井震结合储层精细预测技术、特低渗透储层裂缝表征技术、砾岩储层微观孔隙结构分类研究、基于密井网资料隔夹层刻画技术、砾岩油藏水淹层解释技术、油田开发过程中储层变化规律研究、砾岩储层水流优势通道识别技术、低渗透储层定量...     

水分子结构模式及液态固态水若干特征成因探讨

水是包括海洋大气在内的地球生态系统中极重要又有很多特殊性的物质。其特性的成因尚远非清晰。本文提出一种水分子(H_2O)结构及其固态液态水体的结构模式,探讨和模拟计算了其若干特征的成因,结果能较好符合实测值。(1)从氢(H)氧(O)原子结构和电子绕各原子核及相互绕行规律的等概率随机轨道中实现符合库伦力和开普勒运动规律的优势轨道耦合成平均状态稳定的准刚性的水分子结构。其核心是O原子与等距离分立其两侧的2个H原子构成的等腰三角形,其间距平方之比(H-H)_2/(H-O)_2=2.5;电子云活动空间为1个由4个等边三角形为面构成具有6个等长稜的正四面锥体结构水分子模式(可简称"水分子正锥体模式");该模式具有很大电偶极矩。(2)水分子的端点间在约0.27 nm距离内可以按"+""-"电荷吸引原则耦合。6个水分子将按正、负电荷对接耦合,连接成六边环形"壁"的"笼式隧道空间",可容纳其他物质,无电荷显示,电导率极地。(3)在空气中0℃以下凝结冰晶时三维不对称,"薄片"的雪花形成概率更大,其形态也按自相似原则体现了水分子结构的六角六边六针形的特征。(4)液态水分子维持固态水冰的"冰/水笼"结构模式,但由于2个氢原子上的电子同时到达1个"-"电荷端的概率为1/11,当0℃以上部份水分子能摆脱框架水分子束缚后,可以再耦合一个从框架上"脱落"的"自由水分子"使其进入水笼,从而水容积缩小;固体冰和液态水的密度之比为11/12=0.916 667。自由水分子和水笼框架上的水分子可以随时互换(在10-5s时间尺度上),并适应固体壁的形态,既是不可压缩,又有柔软、可变形特点;水在0~100℃时的空/占比达2.28,模式可解译高温高压的水汽中检测到2.16 g·cm-3,水热传导系数很大,比热容量很大,有"异常"的U形特点,且液态水的比热容量略大于固态水冰的热容量的1/2等特征。(5)讨论了水对O_2、H_2S、NaCl、KCl等的溶解度随温度变化的若干特征的成因和计算模式。通过NaCl饱和溶液实验,证实了本文模式。(6)与液态水体表面特征有关的特点及本文实际应用将在随后续文中讨论。     

利用TRMM卫星资料对青藏高原地区强对流天气特征分析

利用热带测雨卫星TRMM(Tropical Rainfall Measure Mission)多种探测结果,结合NCEP再分析资料,研究了发生在青藏高原地区的一次强对流天气特征,综合分析了高原地区对流云特殊的水平、垂直结构特征。结果表明:(1)该强对流降水系统由几个孤立、零散的块状降水云团组成,以深厚弱对流降水为主,微波亮温的低值区也呈孤立、零散的块状分布,并且整个对流系统的云顶高度一致偏高,深厚强对流降水的雨谱主要集中在1～20mm.h-1的范围内,90%以上的深厚弱对流降水样本数和降水量都集中在0～5mm.h-1范围内,在垂直方向上呈被"挤压"状态。除云冰粒子集中在6～18km高度外,可降冰、可降水和云水粒子都集中在低层8km以下,冰雹天气表现为可降冰粒子在低层含量偏高。(2)高原地区强对流天气的特征与其他地方的不同,表现为雨强较小,比平原地区明显偏弱,且对流云降雨样本在不同降雨率范围内分布不均匀,降水云团雨顶高度也远低于平原地区的对流云,地表降水率大值区与微波辐射亮温低值区呈不完全对称分布,潜热释放呈单峰型。(3)高原地区强对流系统发生时,垂直上升运动在400hPa达到最大,水汽主要集中在400hPa高度以下的范围内。     

Impact of coherent eddies on airborne measurements of vertical turbulent fluxes

During the Hydrological-Atmospheric Pilot Experiment (HAPEX)-Sahel, which took place in Niger in the transitional period between the wet and dry seasons, two French aircraft probed the Sahelian boundary layer to measure sensible and latent heat fluxes. The measurements over the Niamey area often revealed organised structures of a few km scale that were associated with both thermals and dry intrusions. We study the impact of these coherent structures using a single day’s aircraft-measured fluxes and a numerical simulation of that day with a mesoscale model. The numerical simulation at high horizontal resolution (250 m) contains structures that evolve from streaks in the early morning to cells by noon. This simulation shows distribution, variance and skewness similar to the observations. In particular, the numerical simulation shows dry intrusions that can penetrate deeply into the atmospheric boundary layer (ABL), and even reach the surface in some cases, which is in accordance with the observed highly negatively skewed water vapour fluctuations. Dry intrusions and thermals organised at a few km scale give skewed flux statistics and can introduce large errors in measured fluxes. We use the numerical simulation to: (i) evaluate the contribution of the organised structures to the total flux, and (ii) estimate the impact of the organised structures on the systematic and random errors resulting from the 1D sampling of the aircraft as opposed to the 2D numerical simulation estimate. We find a significant contribution by the organised structures to the total resolved fluxes. When rolls occur, and for a leg length of about 30 times the ABL depth, the 1D sampled flux is shown to be sometimes 20% lower than the corresponding 2D flux when the 1D sampling direction is the same as the main axis of the rolls, whereas the systematic error is much lower when the direction of the leg is transverse to the rolls. In the case of cells, an underestimate of around 10% can still be observed with the 1D approach independent of direction, due to poor sampling of the energy-containing scales.     

Statistics of Air Temperature Spatial Variability in the Atmospheric Surface Layer

Surface-layer convection is investigated by analyzing multi-point measurements of temperature and velocity fluctuations at different sets of spatial points.The visual analysis of temperature and velocity fluctuations measured by sensors mounted on a mast of 36-m height clearly reveals the presence of large-scale convective cells (known as ramp structures) making large contributions to the heat transfer from the ground to lower atmosphere. The vertical temperature variability is described with the aid of empirical orthogonal functions derived from temperature covariance matrices for the heights of 1, 2, 5, 10, 18 and 36 m. Temporal-spatial correlation functions obtained allow estimates of a characteristic velocity scale, which may be interpreted as the downwind velocity of ramp structures.     

The Coherent Structure of Water Vapour Transfer in the Unstable Atmospheric Surface Layer

Observations of water vapour fluctuations over arice field show vapour ramps. Coherent structuresare first revealed by the frequently occurring ramp pattern in the vapourtrace. Wavelet and pseudo-wavelet analysis techniques were used inconditional sampling, and more than 100 hr of data have been analyzedto determine coherent structure characteristics. The most probablecoherent structure duration was in the range 2–12 sec andthe duration range of the most effective coherent structures shows somedifference between heat and water vapour transfers. Coherent structurescontribute to the major part of the total flux.     

Numerical Simulation of Macro- and Micro-structures of Intense Convective Clouds with a Spectral Bin Microphysics Model

By use of a three-dimensional compressible non-hydrostatic convective cloud model with detailed microphysics featuring spectral bins of cloud condensation nuclei (CCN), liquid droplets, ice crystals, snow and graupel particles, the spatial and temporal distributions of hydrometeors in a supercell observed by the (Severe Thunderstorm Electrification and Precipitation Study) STEPS triple-radar network are simulated and analyzed. The bin model is also employed to study the effect of CCN concentration on the evolution characteristics of the supercell. It is found that the CCN concentration not only affects the concentration and spectral distribution of water droplets, but also influences the characteristics of ice crystals and graupel particles. With a larger number of CCN, more water droplets and ice crystals are produced and the growth of graupel is restrained. With a small quantity of CCN the production of large size water droplets are promoted by initially small concentrations of water droplets and ice crystals, leading to earlier formation of small size graupel and restraining the recycling growth of graupel, and thus inhibiting the formation of large size graupel (or small size hail). It can be concluded that both the macroscopic airflow and microphysical processes influence the formation and growth of large size graupel (or small size hail). In regions with heavy pollution, a high concentration of CCN may restrain the formation of graupel and hail, and in extremely clean regions, excessively low concentrations of CCN may also limit the formation of large size graupel (hail).     

Vertical Structures of Convective and Stratiform Clouds in Boreal Summer over the Tibetan Plateau and Its Neighboring Regions

Cloud is essential in the atmosphere, condensing water vapor and generating strong convective or large-scale persistent precipitation. In this work, the relationships between cloud vertical macro- or microphysical properties, radiative heating rate, and precipitation for convective and stratiform clouds in boreal summer over the Tibetan Plateau (TP) are analyzed and compared with its neighboring land and tropical oceans based on CloudSat/CALIPSO satellite measurements and TRMM precipitation data. The precipitation intensity caused by convective clouds is twofold stronger than that by stratiform clouds. The vertical macrophysics of both cloud types show similar features over the TP, with the region weakening the precipitation intensity and compressing the cloud vertical expansion and variation in cloud top height, but having an uplift effect on the average cloud top height. The vertical microphysics of both cloud types under conditions of no rain over the TP are characterized by lower-level ice water, ice particles with a relatively larger range of sizes, and a relatively lower occurrence of denser ice particles. The features are similar to other regions when precipitation enhances, but convective clouds gather denser and larger ice particles than stratiform clouds over the TP. The atmospheric shortwave (longwave) heating (cooling) rate strengthens with increased precipitation for both cloud types. The longwave cooling layer is thicker when the rainfall rate is less than 100 mm d^?1, but the net heating layer is typically compressed for the profiles of both cloud types over the TP. This study provides insights into the associations between clouds and precipitation, and an observational basis for improving the simulation of convective and stratiform clouds over the TP in climate models.