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51.
渤南洼陷罗151块火成岩油藏特征及开发对策 总被引:2,自引:2,他引:2
罗151块火成岩油藏是近年在济阳坳陷发现的中型油藏,油藏埋深3150m;在研究罗151井区火成岩成因、侵入期次、岩相学及储层非均质性的基础上,建立了火成岩储层概念模型,划分出角岩微孔隙型油藏及辉绿岩溶蚀孔隙-裂缝型油藏两个类型,纵向上分为4个带,平面上分为3个区;预测了火成岩储层发育的有利部位;部署了合理的开发井网,钻探后,完钻新井14口,平均单井日产油27t,取得了显著效果;火成岩油藏初期产能高,产量递减快,弹性产率低,依靠天然能量开采,最终采收率只有14.1%,可以进行注水开发,注水效果较好。 相似文献
52.
通过遥感技术与地面测定相结合的方法,对北京城市热岛现状作观测研究,得到北京城市地面的温度分布特点。使用北京大学城市边界层模式从气象观点就“楔形绿地”规划对北京城市气候的影响进行研究和评价,模式通过对城市地表复杂性和多样性的特征进行细致描述,建立了一个细致模拟城市特点的城市边界层能量平衡模式,并用此能量平衡模式得到的地面温度作为下边界条件,中尺度气象模式MM5做初始场和侧边界条件,建立一个最小分辨率为500 m的城市边界层模式系统,来研究城市边界层在中尺度背景场作用下的精细结构。通过个例模拟,模式能够较准确地模拟城市边界层的风温场分布情况,可以用来对楔形绿地规划进行模拟试验。通过对规划后的气象场在特定的气象条件下进行模拟,结果显示,建造大型的楔形绿地后,绿地区域及绿地周围约1 km以内的地区温度有所降低,降低的程度由规划前后的地表类型改变的剧烈程度、风速大小及与绿地的距离决定,但是这种规划方案却会因城市的下风方向的风速减小而导致通风不畅。 相似文献
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一次冬季锋面暴风雪天气过程的斜压边界层特征的观测分析 总被引:4,自引:0,他引:4
对STORM-FESTIOP17一次冬季锋面暴风雪天气过程的斜压边界层结构演变及特征进行了分析。发现:暖湿空气沿锋面抬升凝结成云,产生降水过程中释放的大量潜热显著增加锋两侧的水平温度差异,产生锋生。与锋生相伴,在锋前产生低空急流和高空急流。当锋生至最强时,锋两侧温差可达20K,锋前低空急流开始减弱,锋后低空急流增强,锋后冷平流开始主导锋两侧的环流系统。该冷平流削弱锋两侧的温度水平梯度,产生锋消作用。对这次锋面斜压对流边界层的湍流特征分析表明:在边界层之上切应力wv明显增大;湍能收支分析表明在边界层之上的风切变产生项很强,即大尺度天气系统有利于斜压对流边界层的发展,边界层内各量充分混合。这次冬季锋面暴风雪天气过程,冷锋前的低空南风急流从墨西哥湾携带来的充足水汽及锋区边界层大气的强斜压性是其产生的关键因子:冷锋过后,大尺度高空急流的作用更有利于对流边界层的充分发展。 相似文献
56.
Ekman动量近似下中间边界层模式中的风场结构 总被引:2,自引:0,他引:2
发展了一个准三维的、中等复杂的边界层动力学模式,该模式包含了EKman动量近似下的惯性加速度和Blackadar的非线性湍流粘性系数,它进一步改进了Tan和Wu(1993)提出的边界层理论模型。该模型在数值计算复杂性上与经典Ekman模式相类似,但由于包含了Ekman动量近似下的惯性项,使得该模式比传统Ekman模式更近于实际过程。中详细地比较了该模式与其他简化边界层模式在动力学上的差异,结果表明:在经典的Ekman模式中,由于忽略了流动的惯性项作用,导致在气旋性切变气流(反气旋性切变气流)中风速和边界层顶部的垂直速度的高估(低估),而在半地转边界层模式中,由于高估了流动惯性项的作用,结果与经典Ekman模式相反。同样,该模式可以应用于斜压边界层,对于Ekman动量下的斜压边界层风场同时具有经典斜压边界层和Ekman动量近似边界层的特征。 相似文献
57.
改进的切线性模式对一个边界层模式变分资料同化的改善 总被引:7,自引:0,他引:7
大气、海洋中边界层物理过程的强非线性会对切线性模式近似(尤其是当积分时间长时)有较大的影响,从而给相应的4维变分资料同化问题的求解造成困难。本构造了Mellor-Yamada湍流封闭模式(level 2.5)的一个改进的切线性模式,相比通常的切线性模式和简化的切线性模式可以提高对非线性扰动的逼近。利用这个改进的切线性模式的伴随模式分别进行了1到7天的变分资料同化试验,得到了满意的结果。而用通常的伴随模式和简化的伴随模式都无法得到令人满意的结果。 相似文献
58.
The formation of cold air drainage flows in a shallow gully is studied during CASES-99 (Cooperative Atmosphere-Surface Exchange Study). Fast and slow response wind and temperature measurements were obtained on an instrumented 10-m tower located in the gully and from a network of thermistors and two-dimensional sonic anemometers, situated across the gully. Gully flow formed on clear nights even with significant synoptic flow. Large variations in surface temperature developed within an hour after sunset and in situ cooling was the dominant factor in wind sheltered locations. The depth of the drainage flow and the height of the down-gully wind speed maximum were found to be largest when the external wind speed above the gully flow is less than 2 m s-1. The shallow drainage current is restricted to a depth of a few metres, and is deepest when the stratification is stronger and the external flow is weaker. During the night the drainage flow breaks down, sometimes on several occasions, due to intermittent turbulence and downward fluxes of heat and momentum. The near surface temperature may increase by 6 ° C in less than 30 min due to the vertical convergence of downward heat flux. The mixing events are related to acceleration of the flow above the gully flow and decreased Richardson number. These warming events also lead to warming of the near surface soil and reduction of the upward soil heat flux. To examine the relative importance of different physical mechanisms that could contribute to the rapid warming, and to characterize the turbulence generated during the intermittent turbulent periods, the sensible heat budget is analyzed and the behaviour of different turbulent parameters is discussed. 相似文献
59.
Prakash M. Ramchandran Radhika Ramchandran K. Sen Gupta S. M. Patil P. N. Jadhav 《Boundary-Layer Meteorology》2002,104(3):445-461
The central path of the total solar eclipse (TSE) of 11 August 1999 mostly passedthrough a region of active monsoon in India, with the eclipse ending around localsunset. Measurements in the surface layer (SL) were carried out close to the eclipseaxis at Akola (20°42' N, 77°2' E) in central India. The globalradiation flux reaching the surface vanishes around totality at 1803:24 (LT), followedby a small recovery before again dipping to zero at sunset. The temperatures in the SL, and subsoil at 50-mm depth, show a local minimum with a lag of about 10 min after the second contact, whereas the lag appears to vanish when the temperature series is detrended. The SL exhibits near-neutral, though generally stable, conditions from about 1500 hr itself due to heavy cloud cover followed by the eclipse-induced cooling of the surface. The wind component across the eclipse axis vanishes at totality, the wind vector aligning with the azimuth of the traversing moon shadow. The deceleration of the mean flow can be due to the combined effect of the colder surface and downward heat flux, where the locally altered horizontal temperature gradients may cause, as in this instance, the cessation of the cross flow.The oscillations in temperature and wind that show significant peaks, around 90–100 min as well as the semi-period of the eclipse near 60 min, persist for several hours past the eclipse event. A fresh analysis of the published data on the TSE of 7 March 1970 shows spectral peaks in the temperature nearly coincident with those already reported from the surface pressure records. The oscillations in the SL fields during the two TSE events are very similar implying that the source mechanism is also likely to be the same in both the cases. 相似文献
60.
Methanol has been recognised as an important constituent of the background atmosphere, but little is known about its overall cycle in the biosphere/atmosphere system. A model is proposed for the production and emission to the atmosphere of methanol by flowering plants based on plant structure and metabolic properties, particularly the demethylation of pectin in the primary cell walls. This model provides a framework to extend seven sets of measurements of methanol emission rates to the global terrestrial biosphere. A global rate of release of methanol from plants to the atmosphere of 100 Tg y–1 is calculated. A separate model of the global cycle of methanol is constructed involving emissions from plant growth and decay, atmospheric and oceanic chemical production, biomass burning and industrial production. Removal processes occur through hydroxyl radical attack in the atmosphere, in clouds and oceans, and wet and dry deposition. The model successfully reproduces the methanol concentrations in the continental boundary-layer and the free atmosphere, including the inter-hemispheric gradient in the free atmosphere. The model demonstrates a new concept in global biogeochemistry, the coupling of plant cell growth with the global atmospheric concentration of methanol. The model indicates that the ocean provides a storage reservoir capable of holding at least 66 times more methanol than the atmosphere. The ocean surface layer reservoir essentially buffers the atmospheric concentration of methanol, providing a physically based smoothing mechanism with a time constant of the order of one year. 相似文献