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31.
- The variation of the amplitude of waves with varying incident angles when waves propagate through a typical approach channel is discussed by a numerical calculation method, the result of which shows that the influence of the channel on wave propagation is obvious. When the wave propagation direction is in coincidence with the channel axis, the wave amplitude ratio will decrease with the increase of propagation distance. When the incident angle is 15 - 30 , there appears an area of larger wave amplitude ratio on the side slope facing the waves, but at the another side, the wave amplitude ratio is generally small, indicating that the channel has a shielding effect. When waves propagate across the channel perpendicularly, the wave amplitude ratio can be calculated with the shallow water coefficient.  相似文献   
32.
为了监视北京地区的地壳稳定性,北京测绘院对10多个基岩点和北京市区进行了多次沉降观测,结果表明香山点近10多年来高程变化只有几毫米,其重力效应可略而不计,但测点东北和东南方有两个较大的下沉区。用线积分法计算了两个局部沉降的重力效应,在沉降区中心其影响可达0.38μms^-2,但对香山点的重力效应非常小,完全可以忽略。因此得出如下结论:香山点观测到的重力变化不是地壳变形引起的。  相似文献   
33.
水平层状介质中侧向电阻率测井快速迭代反演与应用   总被引:10,自引:3,他引:10  
侧向电阻率测井由于具有较好的探测深度和较高的纵向分辨率而成为油储地球物理测井中的一种重要方法,是确定储层中油气含量的最方要手段。然而,当地层的厚度小于基纵向分辨率时,由于受井眼泥浆和上下围岩等的影响,实测的视电阻率以已无法反映地层电阻率的起初变化,给油气层的划分及油储层的定量评价带有极大的困难,因此,研究侧向电阻率测井反演不论在理论上还是实际应用上均有非常重要的意义。  相似文献   
34.
Sedimentary response to an orogenic process is important for determining whether South China had compressional or extensional orogeny during the period from the Late Permian to the Middle Triassic besides the tectonic and magmatologic evidence. An intracontinental collision event took place between the Yangtze and Cathaysia blocks in the Late Permian. Beginning at the Late Triassic, the tectonic movement was completely changed in nature and entered a post-collisional extensional orogenic and basin-making process. This paper presents sedimentological evidence from the Late Permian to the Middle Triassic in the Shiwandashan basin at the southwestern end of the junction zone between the Yangtze and Cathaysia blocks.  相似文献   
35.
黄河下游壶穴的研究   总被引:10,自引:0,他引:10       下载免费PDF全文
黄河下游(泺口以下)发育了大量的壶穴(Pothole),按成因可以分为6种:流水侵蚀、风蚀、圆砾铸模、冰压刻、冰融水滴蚀及泄气侵蚀。流水侵蚀形成的圆形Pothole规模不一,小者直径在十余厘米,深数厘米,大者直径达数米,深1 m余;风蚀形成的圆形Pothole规模一般比较小,直径多在二、三十厘米以下,深10 cm以下,大部分穴壁缓斜,状如盘碟;圆砾铸模形成的Pothole规模一般较小,直径多在一、二十厘米以下、穴壁陡倾,状如锅穴;冰融水滴蚀形成的Pothole形态复杂,规模不一,既有穴壁缓斜的盘碟状者,也有穴壁陡倾近乎直立的近圆柱状者,直径从不足1cm到三、四十厘米,其穴缘、穴壁和穴底常有次级构造;泄气侵蚀形成的Pothole更是十分复杂,平面形态可以圆形到近圆形甚至其他复杂形态,穴壁可以非常平缓,也可以陡倾,直径从数厘米到数十厘米,深数毫米到二、三十厘米,穴缘和穴壁也常有次级伴生构造,既可单独产出,也可成群产出,同时还可以多个密集产出,状如蜂巢,这一类Pothole的成因极为独特,主要与黄河断流河床捕获的空气泄漏有关。  相似文献   
36.
北天山巴音沟蛇绿岩中堆晶辉长岩的LA-ICPMS锆石U-Pb测年结果确定:巴音沟蛇绿岩中辉长岩形成的同位素地质年代为344.0±3.4Ma。表明巴音沟蛇绿岩所代表的洋盆形成于早石炭世。综合前人天山石炭纪蛇绿岩及构造演化的研究成果,笔者认为巴音沟蛇绿岩是大陆板内强烈拉张的产物。  相似文献   
37.
The wave forces on 1, 2 and 4 vertical circular piles under the action of several wave trains of the same wave parameters, such as Hs,Tp and Mo, but different wave group factor GF are measured in the laboratory. After comparing these forces, it may be concluded that the mean and significant wave forces are almost of no difference for the wave trains with different GF. When GF is larger, the one-tenth of the wave froce extreme is slightly increased and the maximum wave force is much larger than the ones with smaller GF, to which attention must be paid in engineering practice.  相似文献   
38.
Arps递减开发模型   总被引:14,自引:8,他引:14  
本文在Arps递减产能预测模型的基础上提出了Arps递减开发模型,提出了开发速度,采出程度等开发指标的数学关系式,分析了参数Arps递减开发模型的影响,提出了开发初期Arps递减开发模型的确定方法,便于开发初期决策,制作了Arps递减开发模型的logVd-logRp图版,logVd-log(Dt)图版,logRp-log(Dt)图版,提出了开发中晚期Arps递减开发模型的判断方法,三点抛物线法和三  相似文献   
39.
The physics behind the spectral energy distribution (SED) of blazars remains open. We assembled 36 blazars to tackle the factors that control their SED. Now, many blazar spec- tra have the "double hump" feature in the radio and far-IR frequencies. For these a parameter, , is created to characterize the behavior of the SED. We found a significant correlation be- tween the broad-line luminosity (LBLR) and . Because LBLR is an indicator of the accreting power of the source in blazars, we derived a linear correlation, ∝ M˙1/3.18, which suggests that the SED of blazars may depend on the accretion rate, like that of BL Lac objects. We also found a significant correlation between ■ and for a sample of 11 blazars (out of one of 36) with available black hole masses. This implies the Eddington accretion ratio may influence the shape of the SED of blazars.  相似文献   
40.
Following the paper entitled A Preliminary Proposal on Crustobody Geotectonics presented by the first author to the 30th IGC in 1996, this paper further extends and elucidates the concept of crustobody in order to make a unifying study of the evolution and motion of crustal structures and to understand the law governing the formation and development of the earth' crust. In this paper the characteristics of crustobody evolution-motion are given. The authors lay emphasis on the relationship between crustobody evolution-motion and tectonic metallogeny. In the end, a multiple dynamic system of the crustobody evolution-motion is discussed from internal and external dynamic forces, and the mantle creep in internal dynamic factors is paid special attention to.  相似文献   
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