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1.
东亚地磁场模型的计算与分析   总被引:4,自引:0,他引:4       下载免费PDF全文
根据中国、前苏联和蒙古等地区的地磁复测点和地磁台站资料,使用泰勒多项式方法和冠谐分析方法,计算东亚地磁场(X,Y,Z)的泰勒多项式模型和冠谐模型,以及东亚剩余磁场(ΔX,ΔY,ΔZ)的冠谐模型和泰勒多项式模型,并绘制了相应的理论地磁图. 泰勒多项式模型的展开原点位于45°N和100°E,截断阶数为7.地磁场泰勒多项式模型的均方偏差为:X分量是133.0nT,Y分量是107.4nT,Z分量是14.0nT. 球冠极点位于45°N和100°E,球冠半角为42°,冠谐模型的截断阶数为10. 剩余磁场冠谐模型的均方偏差分别为131.2nT(ΔX),112.6nT(ΔY)和13.7nT(ΔZ). 对比分析了上述两种模型. 提出了确定区域模型截断阶数的判据.  相似文献   

2.
青藏高原地磁场模型的研究   总被引:9,自引:6,他引:3       下载免费PDF全文
根据青藏高原地磁三分量绝对测量资料,使用泰勒多项式方法和冠谐分析方法,计 算了青藏高原地磁场(X, Y,Z )的泰勒多项式模型和青藏高原地磁剩余场(△X,△Y,△Z)的冠谐 模型,并绘制了相应的理论地磁图.分析了磁异常点对地磁场模型的影响,对比分析了地磁 场的多项式模型和冠谐模型,讨论了地磁场模型的边界效应问题.  相似文献   

3.
地磁正常场的选取与地磁异常场的计算   总被引:34,自引:8,他引:26       下载免费PDF全文
根据2003年中国地磁观测数据(包括135年地磁测点和35个地磁台)以及我国邻近地区38个IGRF计算点的地磁数据,计算中国地磁异常场的分布。选取两种地磁场模型作为地磁正常场,一是国际参考地磁场的球谐模型,二是中国地磁场泰勒多项式模型。根据各个测点的地磁异常值(观测值减去模型计算值),用球冠谐分析方法计算地磁异常场的球冠谐模型,并绘制2003年中国地磁异常(△D,△I,△F,△X,△Y,△Z)。分析和讨论了中国地磁异常场。  相似文献   

4.
We used data from 1960.0, 1970.0, 1980.0, 1990.0, and 2000.0 to study the geomagnetic anomaly field over the Chinese mainland by using the three-dimensional Taylor polynomial (3DTP) and the surface spline (SS) models. To obtain the pure anomaly field, the main field and the induced field of the ionospheric and magnetospheric fields were removed from measured data. We also compared the SS model anomalies and the data obtained with Kriging interpolation (KI). The geomagnetic anomaly distribution over the mainland was analyzed based on the SS and 3DTP models by transferring all points from 1960.0–1990.0 to 2000.0. The results suggest that the total intensity F anomalies estimated based on the SS and KI for each year are basically consistent in distribution and intensity. The anomalous distributions in the X-, Y-, and Z-direction and F are mainly negative. The 3DTP model anomalies suggest that the intensity in the X-direction increases from ?100 nT to 0 nT with longitude, whereas the intensity in the Y-direction decreases from 400 nT to 20 nT with longitude and over the eastern mainland is almost negative. The intensity in the Z-direction and F are very similar and in most areas it is about ?50nT and higher in western Tibet. The SS model anomalies overall reflect the actual distribution of the magnetic field anomalies; however, because of the uneven distribution of measurements, it yields several big anomalies. Owing to the added altitude term, the 3DTP model offers higher precision and is consistent with KI.  相似文献   

5.
Following a new train of thinking, this paper has explored first the potential information in the ground resistivity data observed by the existing geoelectric observation system, investigated and proposed a new dimensionless geoelectric precursor factor, the degree of ground resistivity anisotropy, S, and studied the characteristics of dynamic evolution pattern of S during the seismogenic process. The results show that, during the seismogenic process, the degree of ground resistivity anisotropy (S) displays a process of 'normal' →'abnormal strengthening (amplitude, range)' →abnormal weakening' → 'earthquake occurrence'→ 'normal'. The earthquake would occur at the time when the S value has entered the late stage of strengthening and turns to weaken and in the gradient belt on the margin of S anomaly region. The dynamic evolution pattern of S reflects the changes of the tectonic stress field during the seismogenic process. Therefore, it would be possible to trace the process of earthquake generation and occurrence from the dynamic evolution pattern of S so as to service earthquake prediction.  相似文献   

6.
1950~1990年中国地磁剩余场冠谐分析   总被引:2,自引:0,他引:2       下载免费PDF全文
根据中国1950、1960、1970、1980年和1990年地磁三分量绝对测量资料,使用球冠谐和分析方法,分别计算1950~1990年各个年代中国地磁剩余场冠谐模型. 球冠极点位于36°N和104°E,球冠半角为30°,冠谐模型的截断阶数为8. 地磁剩余场冠谐模型的均方偏差分别为:对于X分量,1950年为93.1 nT,1960年为128.9 nT,1970年为107.2 nT,1980年为107.6 nT,1990年为95.2 nT;对于Y分量,1950~1990年依次为74.8 nT,98.1 nT,89.2 nT,89.9 nT和84.0 nT;对于Z分量,分别为122.2 nT(1950年),135.0 nT(1960年),137.7 nT(1970年),110.1 nT(1980年)和107.5 nT(1990年). 根据中国地磁剩余场冠谐模型和全球地磁场DGRF模型,得到中国地磁场的冠谐模型,并对冠谐模型的边界效应进行了分析和讨论.  相似文献   

7.
Studyonthepatternandmodeofverticalcrustaldeformationduringtheseismogenicprocessofintraplatestrongearthquakes杨国华,桂昆长,巩曰沐,杨春花,韩...  相似文献   

8.
In the work 2D and 3D fields of stresses of several scale levels close to the off of the main fault (vertical strike-slip fault) in conditions of compression are mathematically calculated and investigated. The solution is found for the elastic task for a 2D “horizontal” field; a 3D field of stresses is obtained by the imposition of a “vertical” unaxis compression. It is shown that the surroundings of the fault are subdivided into three (not two, as is usually considered) regions of types of predictable secondary fractures: “extension,” “strike-slip fault,” and “compression.” In regions close to the off of the main fault, three different microregions occur. The type of destruction in these microregions depends on the parameters of the outer load. Natural and model data of second order fractures that are compared with the calculated data are examined and generalized. The performed investigation is important for the determination of the genesis of secondary fractures, located close to the main fault. The calculated parageneses of secondary fractures may be used for the estimation of the stress tensor type of the regional field.  相似文献   

9.
冯彦  蒋勇  孙涵  安振昌  黄娅 《地球物理学报》2018,61(4):1352-1365
利用149个地面实测数据以及12个子午工程测点数据,50个CHAMP卫星高度实测数据,并结合高空180 km处的50个IGRF12数据点,基于这三个高度的数据首次建立了中国地区地磁场三维曲面Spline(3D Spline)模型.在境外添加了39个测点以控制边界效应.通过CM4模型将所有测点的场源进行分离,统一通过主磁场值建模分析.通过将模拟结果与实测值、曲面Spline(2D Spline)以及Taylor(2D Taylor)、三维Taylor(3D Taylor)模型及IGRF12模型相比较,结果显示3D Spline模型的空间分布与其他模型整体趋势一致,但更为曲折,随着高度上升,3D Spline模型的要素Y的强度逐渐减弱.通过比较3D Spline、2D和3D Taylor模型对于不同高度6个缺测点的模拟值,残差和均方根偏差(RMSE),3D Spline模型的模拟效果最好,要素Y、Z和总强度F的RMSE值要比其他模型低50%以上.3D Spline模型在不同高度处的模拟效果主要取决于该高度附近的实测值数量和精度.  相似文献   

10.
中国地区地磁场水平梯度的计算与分析   总被引:4,自引:4,他引:0       下载免费PDF全文
冯彦  潘剑君  安振昌  孙涵  毛飞 《地球物理学报》2010,53(12):2899-2906
根据2000年中国地区156个地磁台站和复测点的实测数据以及国境外的6个地磁台站实测数据,加上国境外36个IGRF点,分别利用Taylor多项式模型和曲面Spline模型,建立了中国地区地磁场总强度(F)、磁偏角(D)和磁倾角(I)的地磁模型,通过对两种模型中各分量的φ(纬度)和λ(经度)进行微分,计算得到F、D、I的水平梯度值,并绘制相应分量沿南北方向和东西方向的水平梯度图,将其与2000年IGRF10的水平梯度图作比较,最后对水平梯度的空间分布以及三种梯度图进行了分析比较.结果表明:F和I的水平梯度主要随纬度变化,F随纬度增加,变幅约为7.0~6.0 nT/min,在中部地区(25°~35°N,90°~120°E)强度达到最大;I随纬度的增加,变幅约为2'/min~1'/min;D的水平梯度随纬度和经度而变化,随着经度和纬度的增加,变幅分别约为0.4'/min~-0.3'/min和-0.1'/min~-0.4'/min.  相似文献   

11.
12.
Detailed gravity and aeromagnetic data over maars in the Auckland volcanic field reveal contrasting anomalies, even where surface geology is similar. Pukaki and Pukekiwiriki, almost identical maars marked by sediment-filled craters and tuff rings, have gravity and magnetic anomalies of − 6 g.u. and 20 nT, and 8 g.u. and 160 nT, respectively. The Domain and Waitomokia maars, with similar tuff rings but each with a small central scoria cone, have gravity and magnetic anomalies of 32 g.u. and 300 nT, and 21 g.u. and 310 nT, respectively. These differences in geophysical expression are attributed to varying volumes of dense, magnetic basalt in the form of shallow bowl-shaped bodies up to several hundreds of metres in diameter and up to 140 m thick beneath the maar centres. These bodies are interpreted as solidified magma that ponded into early-formed phreatomagmatic explosion craters. Where magma supply was limited relative to groundwater availability, no residual subsurface basalt occurs (as at Pukaki); continued magma supply, but limited groundwater, resulted in ponding (e.g. at Pukekiwiriki) and eventually the building of a scoria cone (as at Domain and Waitomokia). There is no evidence in these geophysical data for diatreme structures below the maars or for shallow and/or extensive feeder dykes associated with these maars. If diatreme structures do occur, their lack of geophysical signature must be a consequence of either their small geophysical contrast with host Miocene sediments and/or masking by the stronger anomalies associated with the subsurface basalt. In addition, any magma conduits appear to be confined centrally beneath the maars, at least to shallow depths (upper 100 m).  相似文献   

13.
计算震磁背景场的数学方法   总被引:2,自引:2,他引:0  
如何计算地磁场 (或地磁剩余场 )及其长期变化的趋势变化 ,是提取震磁异常的关键。文章简要介绍了计算震磁背景场的数学方法 :多项式方法、球冠谐和分析方法、矩谐分析方法和曲面样条函数方法  相似文献   

14.
2000年中国地区地磁场长期变化的区域特征   总被引:10,自引:2,他引:8       下载免费PDF全文
本文用中国地磁场复测点和地磁台站资料,建立了2000年代中国参考地磁场长期变化模型CGRF-SV2000.模型显示,中国地区地磁场变化比较平缓,X、Y、Z、H、D、I、F七个地磁要素的“无符号平均年变率”分别为122 nT/a、82 nT/a、438 nT/a、118 nT/a、096(′)/a、299(′)/a、224 nT/a,比国际参考地磁场IGRF给出的全球年变率约小1/3到1/2.各地磁要素的变化显示,地磁北极正在向中国移近,或者说,中国正在向高地磁纬度方向移动,平均移动速度约为3(′)/a.磁偏角变化还显示,中国地区东西部偏角差异继续扩大.作为检验和对比研究,本文利用第8代国际参考地磁场(IGRF)模型,分析了全球地磁场长期变化的时空特征,讨论了全球长期变模型IGRF_SV与中国长期变模型CGRF_SV的异同点.对比分析表明,中国地区地磁场的长期变化与全球长期变化总趋势基本符合,但是,CGRF_SV也表现出一些特有的局部异常特征.  相似文献   

15.
重力异常分离的小波域优化位变滤波方法   总被引:1,自引:1,他引:0       下载免费PDF全文
在重力异常分离中,频率域滤波分离方法是以全局数据频谱特征设计针对性的滤波器实现的.滤波器参数与空间位置无关,因此无法针对局部数据频谱特征动态调整滤波器参数.针对该局限性,在小波域滤波理论和优化滤波方法的基础上,本文研究提出了小波域优化位变滤波法,该方法具有空间变化滤波能力,在不同空间位置实现不同的滤波器特性,从而能实现局部数据频谱与全局数据频谱存在较大差异的重力异常分离问题.理论模型数据分离实验结果表明,在局部数据频谱与全局数据频谱差异较大的情况下,该方法相对于Butterworth滤波和优化滤波等方法具有优势.最后,用一个实例进行检验计算,体现了所提方法技术的效果和应用前景.  相似文献   

16.
利用CHAMP卫星矢量和标量地磁测量数据,通过三维Taylor多项式模型建立了2010.0年中国及邻近地区在300km高度附近的X、Y、Z和F分量的三维磁场模型.为了比较验证所建模型,分析了其与Taylor多项式模型(二维模型)不同截断阶数所对应的均方偏差(RMSE)、残差及分布等.结果表明,三维模型每一阶的RMSE和残差绝对值的平均值均要比二维模型的小约45%.由于采用了系数完全展开的建模方式,三维模型的系数数量约为二维模型的2倍,三维模型较低的截断阶数可以反映更多的地磁信息.本研究中的5阶三维Taylor模型基本可达到8阶Taylor模型的精度.两种模型绘制的地磁场及残差分布有较好的一致性.  相似文献   

17.
菲律宾及其邻近地区的地磁场模型研究   总被引:2,自引:1,他引:1       下载免费PDF全文
根据2001~2007年期间在菲律宾境内测量的74个点的地磁场数据,利用球冠谐和、泰勒多项式两种方法建立了2005.0菲律宾及周边地区地磁基本场模型,得到了菲律宾地区X、y、Z、D、I、H、F七个分量的分布.两种模型反映的同一地区的地磁场分布形态基本类似,只在拐点的舒缓度、等值线平滑度等方面存在区别.在8°N左右,X、...  相似文献   

18.
The performances of least-squares orthogonal polynomial and relaxation techniques in the separation of regional and residual anomalies have been evaluated with a view to minimizing personal biasing. The advantage of orthogonal over nonorthogonal polynomials is their ability to estimate an optimum order of polynomial to represent the predominant regional trend in the data using an approximate 2D difference table, the Z-matrix. The correlation coefficients between residuals of two consecutive orders also give the same result. In the relaxation technique, a linear trend is assumed within each cell of the mesh of a square grid. A set of such linear segments can approximate any complicated regional trend. The performances of these two techniques have been evaluated using simulated gravity anomalies produced by 2D and 3D complex regional structures superimposed on residual fields due to cylinders and prismatic bodies, as well as three field examples taken from the published literature. The analyses have revealed that the relaxation technique produces excellent results when an optimum polynomial order rather than an arbitrary fixed one is used for computing the boundary conditions along the periphery of the map. Analyses have revealed that such boundary conditions provide minimum distortion near the two ends of the profile.  相似文献   

19.
Current horizontal strain field in Chinese mainland derived from GPS data   总被引:3,自引:0,他引:3  
Introduction In the years when the reliable data could not be obtained and in the analysis of strain property and magnitude in history, the intensity, property and activity pattern of strain field were mainly inferred on the bases of geometric characters of surface traces and behaviors (especially the faults) as well as the characteristics of petrology (XIE, et al, 1993; Molnar, Tapponnier, 1975, 1977; Tapponnier, Molnar, 1977; FU, et al, 2000). However, they are the averaged results accumu…  相似文献   

20.
The parameter of cosmic ray fluctuations, which indicates the degree of IMF inhomogeneity, was introduced in order to quantitatively describe the dynamics of the galactic cosmic ray (GCR) intensity fluctuations during the geoeffective phases of the 11-year cycle. The 5-min data of the high-latitude neutron monitor at Oulu station (Finland) during cycles 20–23 was used in the calculations. The nonrandom non-Gaussian character of the GCR fluctuation parameter is caused by the nonstationary semiannual variation reflecting the transient nonstationary oscillatory process of sign reversal of the general solar magnetic field. This transient oscillatory process is responsible for the maximal geoeffectiveness and duration of the phase of polarity reversal, which manifests itself in a sharp and deep GCR intensity minimum during the final stage of the field sign reversal. The invariant of the 11-year “amplitude-duration” cycle was confirmed on a new basis: the LF drift of the “low” cycle period was detected, which was observed in an increase in the duration of cycle 23 we anticipated.  相似文献   

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