松辽北部三肇地区泉四段高分辨率层序学研究

三肇凹陷扶余油层是松辽北部重点的油气勘探领域之一,主要为一套河流-浅水三角洲沉积,由于河道砂体单层厚度薄、侧向变化快,因此急需对该区开展精细的沉积微相研究,以指导后期地层-岩性油气藏勘探。以肇35区块为例,运用高分辨率层序地层学原理,结合岩心、录井、测井资料,识别层序界面特征,建立层序地层格架,并以短期基准面旋回为制图单元,编制高分辨率层序地层格架内的沉积微相展布图,阐明了其演化规律并建立沉积模式。研究表明：泉四段整体为一长期上升半旋回,内部分出7个短期基准面旋回(SSC1-SSC7),主要发育三角洲平原、前缘2种亚相,进一步分为(水下)分流河道、(水下)决口扇、天然堤等多种微相。7个短期旋回中,SSC1至SSC2基准面缓慢上升,发育上升为主的不完全对称旋回;SSC3至SSC4基准面迅速上升,发育对称旋回和上升为主的不完全对称旋回;SSC5至SSC7基准面上升至最高,发育上升为主的不完全对称旋回。沉积相展布受基准面升降变化控制明显,泉四段自下而上经历了三角洲平原-平原、前缘过渡-三角洲前缘,局部浅湖的演化过程,整体为一次水体由浅变深的湖侵过程。     

大庆宋芳屯油田肇35区块葡萄花油层非均质性研究

从储层宏观与微观非均质性入手,分别研究了肇35区块葡萄花油层的层内、层间、平面和微观非均质性特征及主控因素,研究区层内非均质性主要受到沉积构造、渗透率韵律以及夹层分布等的影响;从物性和隔层分布特征方面分析了层间非均质性特征,自下而上葡萄花油层非均质性呈现弱→强→弱的变化趋势;平面非均质性特征受砂体及沉积微相展布影响较大,沿河道延伸方向非均质性较好。研究区主要发育正常粒间孔、缩小粒间孔和粒内溶蚀孔,整体上储层微观孔隙结构发育良好。从不同方面分析了研究区非均质性对剩余油分布的影响,沉积微相类型和成岩作用是控制储层非均质性的主因素。最终对葡萄花油层主力小层进行储层评价,预测了有利储层的发育面积和分布范围,为下一步的勘探开发提供一定的依据。     

钻杆接头材料35CrMo硫氮复合处理层的干摩擦学性能研究

应用离子渗氮与离子渗硫技术,在钻杆接头材料35CrMo钢表面制备了硫氮复合处理层。采用M-200环块磨损试验机,对比研究了原始渗氮表面与硫氮复合表面在干摩擦条件下的抗磨损性能。结果表明,在干摩擦的条件下,由于摩擦副的接触表面缺乏润滑,硬度较高的渗氮层会加剧接触表面的磨损。而硫氮复合处理层由于在表面存在一层硫化亚铁固体润滑层,在磨损过程中可以起到一定的润滑作用,因此其在干摩擦条件下具备更好的抗磨损性能。     

正己烷/海水微乳液形成的相图研究

用相图方法研究正己烷／海水微乳液的形成。体系相图由水（或人工海水，盐度分别为０，１３．６９６，３０．０７０和４１．１１８）／油（正己烷）／表面活性剂（ＡＳ，ＣＴＡＢ及ＢＲＩＪ３５）／助表面活性剂（正丁醇）在４０℃时构成。分别研究表面活性剂类型，油及醇含量和海水盐度对微乳液形成的影响。结果表明：醇与表面活性剂的摩尔浓度比值大于１时，最适宜于形成微乳液；形成微乳液区的面积随正己烷含量增加而减少；含离子     

Equilibrium trading of climate and weather risk and numerical simulation in a Markovian framework

We consider financial markets with agents exposed to external sources of risk caused, for example, by short-term climate events such as the South Pacific sea surface temperature anomalies widely known by the name El Nino. Since such risks cannot be hedged through investments on the capital market alone, we face a typical example of an incomplete financial market. In order to make this risk tradable, we use a financial market model in which an additional insurance asset provides another possibility of investment besides the usual capital market. Given one of the many possible market prices of risk, each agent can maximize his individual exponential utility from his income obtained from trading in the capital market, the additional security, and his risk-exposure function. Under the equilibrium market-clearing condition for the insurance security the market price of risk is uniquely determined by a backward stochastic differential equation. We translate these stochastic equations via the Feynman–Kac formalism into semi-linear parabolic partial differential equations. Numerical schemes are available by which these semilinear pde can be simulated. We choose two simple qualitatively interesting models to describe sea surface temperature, and with an ENSO risk exposed fisher and farmer and a climate risk neutral bank three model agents with simple risk exposure functions. By simulating the expected appreciation price of risk trading, the optimal utility of the agents as a function of temperature, and their optimal investment into the risk trading security we obtain first insight into the dynamics of such a market in simple situations.

Identification of the diffusion coefficient for a semi-linear hyperbolic-parabolic problem with discontinuous nonlinear terms

Numerical computations concerning geochemical processes in porous media require a knowledge of the values of the macroscopic parameters. In the context of the interpretation of leaching tests one such parameter is the apparent macroscopic diffusivity. In this paper, a mathematical model for dissolution in the presence of diffusion is considered. It is shown that the constant diffusion coefficient can be identifiable when the time integral of the flux is known. Moreover, a practical algorithm for computing the diffusion coefficient is proposed. This revised version was published online in August 2006 with corrections to the Cover Date.     

The nature and structure of the emission line nebula K 3-35: a very young planetary nebula with precessing bipolar jet-like outflows?

We present Hα, [N  II ]6583 and 6-cm continuum images of the emission line nebula K 3-35. The optical images reveal an extended nebula (size ≃ 11 × 9 arcsec² in [N  II ]) in which most of the emission originates in a very narrow (width 0.7–1.3 arcsec) S-shaped region which extends almost all along the nebula (≃ 7 arcsec). The 6-cm continuum emission also arises in this narrow region, which is characterized by an exceedingly high point-symmetry and systematic and continuous changes of the orientation with respect to the nebular centre. The properties of the narrow region suggest that it represents a system of precessing bipolar jet-like components. Two low-excitation, compact bipolar knots near the tips of the jet-like components are observed in the deduced [N  II ]/Hα image ratio. These knots may be generated by the interaction of the collimated outflows with surrounding material. A comparison of the optical and radio images shows the existence of differential extinction within the nebula. Maximum extinction is observed in a disc-like region which traces the equator of the elliptical shell previously observed at 20-cm continuum. All available data strongly suggest that K 3-35 is a very young planetary nebula in which we could be observing the first stages of the formation of collimated outflows and point-symmetric structures typically observed in planetary nebulae. The properties of the jet-like components in K 3-35 are in good agreement with models of binary central stars in which highly collimated outflows originate either from a precessing accretion disc or via magnetic collimation in a precessing star.     

The separation of the stars in the binary nucleus of the planetary nebula Abell 35

Using the Planetary Camera on board the Hubble Space Telescope , we have measured the projected separation of the binary components in the nucleus of the planetary nebula Abell 35 to be larger than 0.08 arcsec but less than 0.14 arcsec. The system has been imaged in three filters centred at 2950, 3350 and 5785 Å. The white dwarf primary star responsible for ionizing the nebula is half as bright as its companion in the 2950-Å filter, causing the source to be visibly elongated. The 3350-Å setting, on the other hand, shows no elongation as a result of the more extreme flux ratio. The F300W data allow the determinination of the projected separation of the binary. At the minimum distance of 160 pc to the system, our result corresponds to 18 ± 5 au. This outcome is consistent with the wind accretion induced rapid rotation hypothesis, but cannot be reconciled with the binary having emerged from a common-envelope phase.     

Distribution of whitemouth croaker (Micropogonias furnieri, Desmarest 1823) larvae in the Río de la Plata estuarine front

Whitemouth croaker (Micropogonias furnieri) larvae obtained and hydrographic data collected in the Rio de la Plata estuary (35°S–56°W) between 1987 and 2000 were used to explore the early life stages spatial and temporal distribution patterns and their relation to oceanographic features. The spatial distribution, restricted to a band in the inner part of the estuary, coincided with the bottom salinity front and the maximum turbidity zone (MTZ, turbidity front). Larvae were present during the warmest months (October through May) within a range of 14–24.5 °C temperature and 0.9–33 salinity. A vertically stratified sampling performed in the region where the largest abundance was found (December 2005 and March 2006) was used to test the hypothesis that larvae retention occurs in the bottom salinity front.The vertically stratified sampling showed larvae throughout the water column with high predominance in the river–estuary transition zone. A positive correlation between abundance and the bottom salinity horizontal gradient was found. The size analysis showed that the largest individuals (>10 mm SL), probably undergoing the settlement process, inhabited near the bottom and that the smallest (<10 mm SL) were present in the whole water column. Length distribution along the front showed no trend.Results support the estuarine retention hypothesis of previous studies on whitemouth croaker gravid females, eggs distribution and outcomes from a numerical simulation model. Retention in the salinity front/MTZ would allow larvae to benefit from food accumulation in the region, the high turbidity level provide shelter against predators and retention in the estuary secure closeness to the main nursery ground.