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高精度重力异常模型是研究地球内部结构的基础地球物理数据.本文依据中国大陆构造环境监测网络项目的 100个高精度绝对重力基准站数据,首先,分别与EGM2008模型和GGMplus模型进行对比,得到了模型之间的差异性特征统计参数;其次,我们对与绝对重力同点位测量的垂直梯度数据,进行统计分析,结果表明重力垂直梯度变化的标准差高达537.2E.通过提取Crust1.0地壳结构模型参数,计算得到了Moho界面起伏引起的垂直梯度变化,分析认为地表垂直梯度的变化主要与地形和浅部密度异常体相关.最后,基于重力场模型和观测数据的统计结果,针对经典重力异常计算公式中的一些流程提出了优化建议.本文结果对于使用区域重力异常模型,研究地壳结构和提高长剖面、小比例尺重力探查项目中的异常计算精度具有重要意义. 相似文献
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基于轨道扰动引力谱分析的方法确定低低观测重力卫星反演重力场的空间分辨率 总被引：1，自引：1，他引：0
基于低低卫-卫跟踪重力卫星的轨道特性,从垂直和水平两个方向计算了重力卫星高空扰动引力,并根据其谱特性及星载加速度的测量噪声水平分析了重力卫星能反演重力场的阶数.利用EGM96重力场模型分别计算了400 km、450 km和500 km 轨道高度处重力卫星受到的扰动引力谱及扰动引力谱的平均量级,分析其垂直特性表明:在三个轨道高度处能分别能反演150、140和130阶的重力场模型.利用两颗同轨重力卫星相距220 km的特性,计算了400 km、450 km和500 km 轨道高度处纬度相差2°的两颗卫星纬向扰动引力差,即扰动引力水平分量,分析其谱特性,表明:重力卫星能反演至117阶的地球重力场模型. 相似文献
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流动重力测量作为地震前兆监测手段之一, 所得到的区域重力场微变化信号反映地壳内部密度变化、 地壳变形、 流体运移等信息。 采用定量化和模型化方法研究与地震孕育相关的重力场变化信号时空特征, 对于构建地震预报定量化指标体系具有重要意义。 通过设定场源参数构建了数值模型, 正演得到了多组不同场源条件下的重力场变化模型; 通过模型对比, 分析了重力变化与重力梯度变化对不同类型场源参数的关系。 研究结果表明: 重力垂直梯度变化对异常体边界比较敏感, 特对浅部异常更为敏感, 适用于圈定异常体范围。 以此为基础提出了观测系统的优化测量方案, 以及对观测精度的需求。 研究结果对于构建地震预报指标参数, 优化流动重力观测系统具有一定参考意义。 相似文献
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本文基于绕月卫星跟踪技术的三种模式,即地面跟踪模式、高低跟踪模式和低低跟踪模式,将月球重力场的发展历程分为四个阶段.分别介绍了各阶段跟踪模式的主要原理、技术特点以及所获取的具有代表性的重力场模型,并对这些模型的精度特征进行了评述.进而,通过分析不同阶段重力场模型所获取的月球重力异常特征和精度、不同阶段重力场模型的定轨精度,阐明了:空间跟踪技术的进步,极大地提高了月球重力场模型的精度,并且,有效地促进了对月球物质结构特征的认识和绕月卫星定轨的可靠性.最后对月球重力场模型中尚存在的问题以及探测技术的发展前景进行了分析和展望. 相似文献
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建立高精度高分辨率区域地球重力场模型是大地测量学科的重要科学目标之一,可为固体地球物理、地球动力学、地震学以及资源勘探等领域提供基础信息,也是当前大地测量现代化发展实现GNSS测定海拔高程的重大需求.提出了一种基于矩谐分析的区域重力场建模方法,在局部直角坐标系中求解地球引力位的Laplace方程,推导了扰动位、重力异常、重力扰动、大地水准面差距和垂线偏差的矩谐展开式以及矩谐系数阶方差和阶误差的计算公式,给出了利用重力观测值进行矩谐分析求解矩谐系数的数学模型和算法,为抑制矩谐分析中存在的周期延拓边界效应,提出了扩展计算区域范围的策略.利用EGM2008重力位模型生成模拟地面重力和航空重力观测值,加入标准差为2 mGal的高斯白噪声,分别设计基于地面重力数据和基于航空重力数据的模拟数值试验,对矩谐分析建模方法进行了验证与分析.数值结果表明基于矩谐分析构建的区域重力场模型可靠且可达很高的精度,由地面和航空重力数据计算的2.5′×2.5′大地水准面精度分别达到1 cm和1.4 cm,4 km飞行高度处航空重力观测值的向下延拓误差仅为3.1mGal,矩谐分析可为区域重力场精细结构的逼近提供一种新的选择. 相似文献
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洋底板块运动是地球动力学和全球变化研究的重要内容.本文根据质量迁移与地球外部重力场变化的对应关系,利用不同时期测高资料推算的1995—2019全球海洋重力场变化结果,反演分析全球洋底板块运动特征.研究表明,板块汇聚边界、板块内无震海岭、海山群、断裂带等区域重力异常变化显著,而在板块离散边界无明显变化趋势;西南印度洋中脊、大西洋中脊、中印度洋中脊等地区重力异常垂直梯度变化显著,且在西太平洋俯冲带、部分海岭区域也存在明显变化,其空间分布与地形基本吻合.海洋重力场变化整体上准确反映了全球洋底板块构造运动.相较于重力异常变化反演结果,重力垂直梯度的变化能够更为准确地反映洋底板块运动特征,特别是在洋中脊区域,扩张速率越小,垂直重力梯度变化越显著.此外,详细讨论了测高海洋重力场不确定因素对洋底板块运动分析结果的影响,海面坡度改正是主要因素之一. 相似文献
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本文采用基于贝叶斯原理的重力平差方法对华北地区2009—2017年的16期陆地流动重力观测资料进行了统一处理,结合研究区内2009年以来4次M≥4.5 地震活动,分析区域重力场动态演化特征。基于华北地区均衡重力异常、布格重力异常、沉积层重力异常和莫霍面重力异常,研究华北地区三维密度结构特征,分析区域重力场变化与深部密度结构之间的关系。结果表明:研究区内近年来M≥4.5地震均位于区域差分重力场和累积重力场“零值”等值线附近、异常变化剧烈的梯度带及梯度带转弯部位,以及深部结构中理论均衡厚度与实际地壳厚度存在差异的非均衡区和三维密度结构的高低密度过渡带内。 相似文献
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本文介绍了"嫦娥一号"月球探测卫星轨道跟踪数据的特征,简要阐述了基于动力法精密定轨解算月球重力场模型的原理及策略.在"嫦娥一号"测控数据精度和覆盖均有限的条件下,独立使用"嫦娥一号"月球探测器6个月的在轨运行双程测距测速跟踪数据,成功得到了50阶次月球重力场模型CEGM-01.通过多种方式,如重力场模型频谱特性、实测数据定轨残差、月球重力异常特征、与地形的相关性及导纳值,对解算得到的CEGM-01月球重力场模型进行了精度评价,分析了相应的物理特性和效果.结果表明了CEGM-01解算过程的有效合理.在此基础上展望了我国月球重力场探测未来可能的发展方向. 相似文献
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陆地重力观测相较于航空和卫星重力观测,距离场源更近,观测精度相对较高,其静态异常和时变数据已广泛应用于研究多种地球动力学问题.21世纪以来,绝对重力观测技术发展迅速,陆地观测网络日益完善,高精度陆地重力观测数据产品逐渐丰富,基于这些产品的大地测量和地球物理研究不断取得新进展.本文总结了近十几年来高精度陆地重力观测数据在大地测量和地球物理领域的应用进展情况,包括基于重力异常数据构建重力场和大地水准面模型、建立地壳物性结构模型、反演Moho界面形态和估计岩石圈有效弹性厚度,以及利用时变重力数据构建时变重力场模型、探测微弱动力学信号、估计地壳构造变形速率和分析与火山、地震过程的可能关联,最后探讨分析了陆地重力测量的未来发展趋势,可为中国大陆重力观测系统建设与发展规划提供参考. 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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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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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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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 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
19.
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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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