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海底冷泉活动在全球大陆边缘海域广泛分布.与传统利用高频声学方法探测海底冷泉羽状流不同,本文利用常规多道反射地震(地震海洋学)方法对海底边界附近水体进行成像,结合盆地流体逸散结构特征,圈定活动冷泉流体活动发育位置,分析其地震反射特征和流体活动特征.研究表明,活动冷泉流体渗漏、逸散活动在多道反射地震剖面上一般呈羽状、扫帚状和不规则状几何形态,内部反射杂乱,反射振幅偏弱,但也有振幅增强的情况出现,这可能是由于含有较多泥质和细粒颗粒物悬浮.所造成的.冷泉活动一般与盆地内部泥底辟、流体管道、断层和裂隙、气烟囱、海底麻坑和泥火山等流体逸散结构相关,反映了地层内部流体自深部向浅部运移,在海底渗漏、逸散形成了活动冷泉.但分析结果仍需要进一步实地观测和理论模拟等相关研究确认. 相似文献
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海底冷泉羽状流是海底冷泉活动最直接的表现形式,与天然气水合物动态成藏和动态油气系统密切相关.近年来,因其对全球气候变化的影响和潜在的资源前景,冷泉流体活动受到越来越多重视.本文对全球重要海域海底冷泉羽状流的分布和通量相关研究进行总结分析,发现冷泉羽状流广泛分布在主动和被动大陆边缘,而在弧后地质背景和走滑大陆边缘发现较少,研究不够深入.在构造活动活跃、沉积速率和运移通道渗透率高的地质背景下,冷泉羽状流一般呈区域性聚集发育,规模与通量较大.目前研究发现,通常单个羽状流渗漏孔的通量一般介于3.5 mL/min～ 13.9 L/min之间,但受制于观测技术和成本,羽状流的通量估算具有不确定性,且易受到不同地质和海洋控制因素的影响.另外,冷泉羽状流发育区往往对应或指示重要海洋油气富集区,通过与海域天然气水合物试采结果和天然气水合物工业生产指标进行对比分析,认为大型单体冷泉羽状流以及与水合物赋存或深部油气藏相关的区域性羽状流群具有重大资源效应,主要体现在羽状流本身的气体通量资源效应、与天然气水合物的密切联系以及对于海洋深部动态油气藏的指示三个方面.建议重视对海底冷泉羽状流发育区的调查与探测,尤其针对大型单体冷泉羽状流,加强对其活动特征的长期观测,从而明确其时序渗漏特性、活动机制以及海洋与地质因素的控制作用.通过研究有效的通量测量技术和方法,建立冷泉羽状流资源评价技术标准,从而推进其进一步开发与利用. 相似文献
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近年来，活动冷泉的研究越来越受到关注.本文利用多波束数据、多道地震数据以及底质取样结果研究琼东南海域活动冷泉系统，分析活动冷泉的羽状流特征、海底地貌与底质特征以及流体活动构造特征.多波束水体数据上，观测到多个延伸高度超过750 m的气泡羽状流，海底流体活动非常强烈；多道地震上识别出麻坑、流体运移通道、气烟囱等流体渗漏相关的构造，与其他海域观测到的反射特征不同，羽状流的下方流体运移通道呈强振幅"串珠"反射；重力活塞取样在两个站位上获得浅表层块状天然气水合物.其中一个站位位于活动冷泉附近，天然气水合物赋存于海底以下8 m左右.基于以上三方面的数据，笔者提出了一个用于描述活动冷泉系统的形成模式，游离气通过气烟囱向上运移到达浅层，一部分在天然气水合物稳定带内形成天然气水合物，另一部分穿透天然气水合物稳定带到达海底，形成活动冷泉的羽状流. 相似文献
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海底冷泉羽状流与海底天然气水合物的分布密切相关,对水合物稳定带的边界具有指示作用,是未来能源勘探的重要领域.研究海底冷泉羽状流的地震响应特征,对确定天然气水合物的储集区域及成藏环境等均有重要意义.当前获得海底冷泉羽状流的地震响应主要通过数值模拟进行,然而该过程所依据的含气泡介质声速模型及随机介质理论不能完整描述海底冷泉的物理性质,采用的声波方程也不适用于高频地震波数值模拟.为了准确地实现海底冷泉羽状流地震波数值模拟,精确分析其地震响应特征,本文提出利用Keller-Miksis气泡振动模型来描述气泡在声波作用下的运动状态,同时考虑气泡间的相互作用,建立海底冷泉气泡模型.在此基础上,本文创新性地采用含气泡液体声波方程进行海底冷泉高频地震波数值模拟.数值模拟结果表明,本文提出的方法能够实现海底冷泉羽状流地震响应的高精度数值模拟. 相似文献
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《地球物理学报》2020,(9)
海底冷泉羽状流与海底天然气水合物的分布密切相关,对水合物稳定带的边界具有指示作用,是未来能源勘探的重要领域.研究海底冷泉羽状流的地震响应特征,对确定天然气水合物的储集区域及成藏环境等均有重要意义.当前获得海底冷泉羽状流的地震响应主要通过数值模拟进行,然而该过程所依据的含气泡介质声速模型及随机介质理论不能完整描述海底冷泉的物理性质,采用的声波方程也不适用于高频地震波数值模拟.为了准确地实现海底冷泉羽状流地震波数值模拟,精确分析其地震响应特征,本文提出利用Keller-Miksis气泡振动模型来描述气泡在声波作用下的运动状态,同时考虑气泡间的相互作用,建立海底冷泉气泡模型.在此基础上,本文创新性地采用含气泡液体声波方程进行海底冷泉高频地震波数值模拟.数值模拟结果表明,本文提出的方法能够实现海底冷泉羽状流地震响应的高精度数值模拟. 相似文献
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甲烷羽状流备受关注,因为它提供了海底气体泄漏的直接证据,并对天然气水合物的勘探识别起到了间接指示作用.为了深入研究冷泉活动区气泡羽状流的地震响应特征,根据已有研究成果——羽状流模型及其偏移剖面,通过小波变换分析单道地震信号及羽状流剖面的尺度特征.单道地震信号最佳尺度曲线表明不同气含量对应的最佳尺度也不同,而且不同深度的最佳尺度变化较大;羽状流最佳尺度剖面能够显示出羽状流区域的轮廓.羽状流气含量与最佳尺度呈较好的正相关,即随着气含量的增加,最佳尺度也随之增大. 相似文献
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海底冷泉渗漏是海洋环境中广泛分布的自然现象.本文主要介绍海底冷泉原住观测技术及全球几个典型冷来渗漏活动地区的原位观测结果.冷泉渗漏活动主要发育在海底裂隙和断层发育的地区,海底常有泥火山、麻坑、水合物、冷泉生物群落和冷泉碳酸盐岩的发育.冷泉渗漏主要包括液体和气体两种形式,流体流动包括上升流和下降流两种方式,流量变化大,主要与海底环境及构造作用有关.烃类渗漏是以气泡、油滴的形式沿断层向海底喷溢,释放量大,运移过程主要受涌浪、静水压力和裂隙压力等因素控制.冷泉渗漏活动是复杂的水文地质过程,受水合物形成和分解产生的气藏的充注和排空、深部常规油气藏的破坏及海底环境变化等多种作用的控制. 相似文献
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海底冷泉广泛分布于全球大陆边缘海域,是未来能源勘探的重要领域.本文根据海底冷泉羽流特征,设计多个典型2D冷泉气泡散射地球物理模型并观测其数值模拟的地震响应特征.冷泉正演模拟的关键是建立典型地震海底冷泉散射模型,本文首先构建了平稳随机散点模型,设计了符合实际的气泡半径和气泡体积分数的参数模型,通过参数填充和计算得到了等效速度模型.由此建立的模型在适应性和灵活度上凸显出很大优势,极大地提升了地震响应的可靠程度.单炮地震记录显示冷泉羽流区散射能量最强,地震波场散射清晰,散射波场沿冷泉延伸方向具有明显的方向性.复杂冷泉气泡散射模型的正演模拟结果表明地震响应能够准确描述海底冷泉羽流,对冷泉羽流的研究和寻找海洋天然气资源具有重要意义. 相似文献
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D. M. Pechersky A. A. Lyubushin Z. V. Sharonova 《Izvestiya Physics of the Solid Earth》2010,46(7):613-623
The data on geomagnetic reversals are compared with the changes in the organic world and with the lower-mantle plumes. The
times of the formation of plumes and the times of their appearance on the Earth’s surface relate to the intervals characterized
by the different frequencies of geomagnetic reversals, i.e., there is no interrelation between the formation of plumes and
the frequency of the changes in the geomagnetic field polarity. At the same time, a certain synchronism is observed between
the frequency of the geomagnetic reversals and the boundaries of the biostratigraphic ages, i.e., the changes in the organic
world in the long-period range. A hypothesis is proposed, which explains the change in the sign of the geomagnetic field by
the combined effect of the irregular rotation of the internal core relative to the mantle and the changes in the slope angle
of the axis of the Earth’s rotation, which, in turn, results in synchronous events on the Earth’s surface: the rates of changes
in the organic world. 相似文献
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Prof. Dr. W. A. Heiskanen 《Pure and Applied Geophysics》1958,41(1):1-18
Summary The author mentions the aims of the World-wide gravity project he established in the Ohio State University in Columbus, in 1950. He outlines the practical procedure of the gravimetric computations of the undulationsN and the vertical deflection components and and emphasizes that only by the global international cooperation and additional gravity observations at sea carried out during the last decade it has been possible to gather to Columbus the needed gravity material. Since there exist still large gravimetrically unsurveyed areas it is of vital significance to study what gravity anomalies are best to be used for these regions. The given figures concerning the accuracy of theN, and , estimated theoretically and obtained in practice, indicate that in the gravimetrically well surveyed parts of the world like in Europe and the United States we can get gravimetrically on basis of existing gravity material theN-values with accuracy of about 5–10 meters, and and with the accuracy of about 1. The geoid undulationsN are already computed in Columbus for more than 6000 points of the northern hemisphere. The sample maps show the interesting geoid of Europe and vicinity between the latitudes 60° and 30° and longitude 5° W and 30° E, drafted on basis of more than 1000N-values computed at the corners of 1°×1° squares. It is interesting to realize that the geoid undulations in all this area are positive, the extreme values being between 40 and 50 meters. The geophysical significance of the geoid maps of this kind is pointed out. 相似文献
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Summary The maintenance of the axisymmetric component of the flow in the atmosphere is investigated by means of a steady-state, quasi-geostrophic formulation of the meteorological equations. It is shown that the meridional variations in the time-averaged axisymmetric variables can be expressed as the sum of three contributions, one being due to the eddy heat transport, another to the eddy momentum transport, and a third to the convective-radiative equilibrium temperature which enters the problem through the specification of a Newtonian form of diabatic heating. The contributions by the large scale eddies are evaluated through the use of observed values for the eddy heat and momentum transports.The contributions from each of the three forcing mechanisms to the temperature and zonal wind fields are invstigated individually and found to be of about equal importance. The sum of the three contributions are also presented for the temperature, the zonal wind, the stream function associated with the mean meridional circulation and the corresponding vertical motion. Although the results fail to reproduce the main observed features of the lower stratosphere, they are found to be in good agreement with observations in the middle latitude troposphere. At any pressure level, for example, the computed mean zonal wind has a jet-like profile and the axis of the jet is found to slope to the south with height, as observed in the atmosphere.Based in part on a thesis submitted by the first author as partial fulfillment of the requirements for the Ph.D. degree at the University of Michigan. — Publication No. 194 from the Department of Meteorology and Oceanography, The University of Michigan. 相似文献
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综合APIA、HONOLULU、PAMATAI 3个地磁台三分量的11年周期变化的形态后，可定性地提出该变化源于内场。如内源为核幔边界的电涡流，则其中心点应位于3台之间。 相似文献
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V. E. Pavlov T. Yu. Tolmacheva R. V. Veselovskiy A. V. Latyshev A. M. Fetisova I. V. Bigun 《Izvestiya Physics of the Solid Earth》2017,53(5):702-713
Until recently, the existing data prevented the geophysicists from accurately dating the Bysy-Yuryakh stratum, which outcrops in the middle reach of the Kotuy River, constraining the time of its formation to a wide interval from the end of the Late Cambrian to the beginning of the Silurian. The obtained paleomagnetic data unambiguously correlate the Bysy-Yuryakh stratum to the Nyaian regional stage and constrain its formation, at least a considerable part of it, by the Tremadocian. This result perfectly agrees with the data on the Bysy-Yuryakh conodonts studied in this work and yields a spectacular example of the successful application of paleomagnetic studies in solving important tasks of stratigraphy and, correspondingly, petroleum geology. Within the Bysy-Yuryakh stratum, we revealed a large normal-polarity interval corresponding to the long (>1 Ma) period when the geomagnetic reversals were absent. This result, in combination with the data for the Tremadocian and Middle–Upper Cambrian sequences of the other regions, indicates that (1) the rate of occurrence of the geomagnetic reversals on the eve of the Ordovician Moyero superchron of reversed polarity was at most one reversal per Ma; (2) the superchron does not switch on instantaneously but is preceded by a certain gradual change in the operation conditions of the dynamo mechanism which, inter alia, manifests itself by the reduction of the frequency of geomagnetic reversals with the approach of the superchron. This finding supports the views according to which a process preparing the establishment of the superchrons takes place at the core–mantle boundary. 相似文献
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The nutations of the planets Mars andEarth are investigated and compared. Alarge number of interior structureparameters are involved in the nutationcomputations. The comparison between the observations and the computationsprovides several constraints on these parmeters andtherefore allows a better understanding of the physics of the interior of theplanet. For the Earth, the high precision of the observations of the nutationshas led to a very good determination of interior properties of the planet. ForMars, observations of nutations are not yet available, and we review how theamplitude of the Martian nutations depends on the hypotheses consideredfor its interior. Although Mars is very similar to the Earth, its interior is not well known;for example, we don't knowif its core is liquid or solid. Only if the core is liquid,the Free Core Nutation (FCN) normal mode exists and can alter the nutationswhich are close to the resonance. From the observed geoids, it is known thatboth planets are not in hydrostatic equilibrium. The departure is larger forMars than for the Earth, and consequently, the implication of considering a convective mantle instead of a mantle in hydrostatic equilibrium described byClairaut's equation for the initial equilibrium state of the planet is largeron the Martian nutations than on the Earth nutations. The consequences of theuncertainty in the core dimensions are also examined and shown to be of a veryhigh influence for Mars if the core is liquid, due to the potential changes inthe FCN resonance. The influence of the presence of an inner core, which isknown to exist for the Earth, could be more important for Mars than for theEarth if the inner core is large. Due to the presence of Tharsis on Mars, thetriaxiality of this planet has, additionally, larger effects than on Earth. 相似文献
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The global database on the paleointensity, containing determinations of the virtual dipole moment (VDM) for a stable (normal) regime of the geomagnetic field in a time interval of up to 3.5 Ga, is supplemented by new VDM determinations and analyzed. The field generation process started no later than 3–3.5 Ga (earlier data are absent) at the stage of the Earth’s core formation. Since that time, the dipole value has differed from its present value by no more than an order of magnitude, and the deviations that have already been detected tend toward smaller values. The distribution of VDM values in the time interval 0–400 Ma is bimodal, which apparently reflects the presence of two different generation levels of the geomagnetic field distinguished by a relatively large value (close to the present field value) and a relatively small value (approximately half as large as the present value). The total duration of decreased VDM values appreciably exceeds that of increased VDM values (179.1 and 28.6 Myr, respectively). On the whole, data on the paleointensity do not contradict the hypothesis about the dipole nature of the field over the last 400 Myr; however, the number of determinations at high paleolatitudes is too small to draw decisive conclusions on the validity (or invalidity) of the dipole field approximation based solely on paleointensity data. 相似文献
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Geomagnetism and Aeronomy - The evolution of the magnetic configuration in the solar corona is studied. The curvature of the K-corona helmets obtained from an analytical approximation of the... 相似文献