共查询到18条相似文献，搜索用时 140 毫秒
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IGRF（国际地磁参考场）资料在地磁学的基础研究中得到广泛的应用.利用IGRF国内外学者研究了高斯分析、地球磁场模型及其源场可能位置、重磁关系、核幔耦合、地磁场能量、地球非偶极子磁场以及长期变化场的西向漂移等,研究了IGRF在我国地区的误差以及产生的原因.在研制中国地磁等值图中也得到某些应用. 相似文献
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根据历史地磁场模型GUFM1、第10代国际参考地磁场（IGRF10）模型和日长资料,采用小波变换方法,分析了地磁场磁矩、能量、西向漂移等参数的长期变化和日长十年尺度变化的周期分量及其时变特征.结果表明,1800～2005年期间,偶极子磁场长期变化有82年和48年准周期分量,它们与日长变化的周期没有直接关系.非偶极子磁场参数的长期变化与日长变化有66年和32年准周期分量,66年准周期比32年准周期强.在66年准周期分量,西向漂移比日长变化超前8.8年,非偶极子磁场能量比日长变化滞后15.6年.日长十年尺度波动和地磁场长期变化的起源不存在因果关系. 相似文献
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王Tan文 《地震地磁观测与研究》1998,19(2):38-42
首次引用古地磁学中虚地磁极（ＶＧＰ）的计算方法来研究现代地磁场的变化规律。通过对中国地区６个台站资料的分析以及对全球３９个台站资料的分析结果可以得出结论：利用地磁场角度分量来研究长期变化是可行的;ＶＧＰ的漂移情况正好表明非偶极子磁场的存在与随时间的变化;ＶＧＰ漂移方向的全球分布与地磁长期变化场的有关分量等值图之间的一致性较好。 相似文献
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本文根据最新修正的国际地磁参考场模型，研究了１９４５－１９９５地磁场中心偶极矩变化，地磁总场及其分量Ｘ、Ｙ、Ｚ的空间功率谱，地磁场长期变化谱的经向漂移和纬向漂移的功率谱和西向漂移速度。研究中发现最近５０年偶极矩仍在继续衰减，空间功率谱的变化也呈减小趋势。在经向谱的漂移中观察到１９７０年出现最小值，而在纬向漂移变化中１９７０年出现最大值，西向漂移速度的变化也在１９７０年出现最大值，这种现象正是１９７０年发生的地磁长期变化的突变，称作地磁＂Ｊｅｒｋ＂。 相似文献
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本文根据最新修正的国际地磁参考场模型，研究了１９４５－１９９５地磁场中心偶极矩变化，地磁总场及其分量Ｘ，Ｙ，Ｚ的空间功率谱，地磁场长期变化谱的经向漂移和纬向漂移的功率谱和西向漂移速度。研究中发现最近５０年偶极矩仍在继续衰减，空间功率谱的变化也呈减小趋势。 相似文献
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国际地磁参考场资料在我国得到广泛应用。利用国际地磁参考场资料，我国学者研究了高斯分析、地球磁场模型及其源场可能位置、重磁关系、核幔耦合、地磁场能量、地球非偶极子磁场西向漂移等。在绘制中国地磁等值图中也利用了某些国际地磁参考场资料。 相似文献
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本文利用近三十年来的地面测量资料和东亚地区11个地磁台的资料,以及1965.0、1975.0国际地磁参考场等资料,对东亚大陆磁场的时、空变化特征进行了研究。内容包括:东亚大陆磁场的空间分布特征及场源深度的估算,东亚大陆磁场的中心位置及其磁场强度、磁场方向,近三十年来东亚大陆磁场的长期变化特征等。得到的主要结果是:1.东亚大陆磁场的中心位置近三十年来没有西向漂移的迹象,从而推断它的长期变化主要由场源强度的变化所引起,而不是主要由非偶场的西向漂移所引起;2.东亚大陆磁场的中心与它的长期变化的中心不相一致,同时,在青藏高原的东部还可能存在一弱中心。 相似文献
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对1950年以来中国及其邻近地区的地磁观测台和复测点地磁三分量数据进行了系统地分析,求得这期间每5年的共7组地磁长期变化的模型（SV模型）.利用这些SV模型将需要的地磁观测值归算到所需的年代,很好地建立了1950-1985年中国地区的主磁场模型.文中还表示了中国地区1950年以来地磁各分量地磁长期变化的时空变化趋势.这些SV模型系数和国际参考地磁场系数计算的SV值与相应观测的SV值比较,由中国SV模型系数得到的均方值比国际参考场的小. 相似文献
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西向漂移是地磁场长期变化最重要的特点之一,而西漂最显著的部分是非偶极子场部分．本文以１９００-２０００年国际参考地磁场（ＩＧＲＦ）为依据,运用无线电科学中的"移动变形图案相关分析"方法对近百年来东亚大陆磁异常的漂移运动进行了分析,得到磁异常各分量漂移矢量随时间的变化．结果表明,最能代表地磁场西漂特征的Ｚ分量异常近百年来平均西漂速度为０.０７°／ａ,明显小于全球磁场西漂的平均速度０．２°／ａ．Ｚ分量还显示出０.０２°／ａ的缓慢北向漂移．详细分析还表明,东亚大陆磁异常的漂移分为３个阶段：１９００-１９３０年为较快的西漂,平均速度为０.１０°／ａ;１９３０-１９８０年为西北向漂移,平均西漂速度分量０．０７°／ａ,北漂速度分量为０．０４°／ａ;１９８０年后漂移几乎停止,并有转为东漂的迹象． 相似文献
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1900~2000年的IGRF(国际地磁参考场)资料使研究20世纪中地磁场的变化规律成为可能,在20世纪中,即使从19世纪起,地球偶极子磁场发生了较大的变化,偶极矩一直保持衰减的势头,地心轴的所有3个分量都是减小的.地磁南极的位置变化在1930年左右发生大的转折,1960年起向西和向南快速移动,偶极子轴在纬度方面变化只有1°左右,经度变化在3°左右,离磁极倒转的条件差得远. 相似文献
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Takesi Yukutake 《Physics of the Earth and Planetary Interiors》1979,20(2-4):83-95
In view of the classification of the geomagnetic field into its axisymmetric and non-axisymmetric parts, studies of geomagnetic secular variations on the historical time-scale are reviewed. The westward drift of the geomagnetic field, which is one of the most conspicuous features of its secular variation, is examined first. The non-axisymmetric field during the past several hundred years can be well approximated by the superposition of two constant-magnitude fields, a standing and a drifting field, whose lifetimes are supposed to be longer than 1000 years. It is pointed out that the sectorial term of the non-dipole standing field is small compared with the drifting one. The lack of the n = M = 2 term of the standing field is particularly remarkable.
On the other hand, the equatorial dipole field is likely to consist of two components which are both drifting. One drifts westwards with a normal velocity and the other eastwards with a small velocity.
Besides the pronounced westward drift in an east-west direction, the poleward movements of particular foci of the secular variation are noted. This may, however, be related to the rapid growth of the axisymmetric quadrupole field.
The time variation of the dipole field is briefly examined. As far as the data on the historical time scale are concerned, an antiparallel relationship seems to exist between the variations in the dipole and the quadrupole field. As the dipole moment decreases, the magnitude of the quadrupole moment increases. Finally, characteristic oscillation periods of the dipole field are examined. Although the data are few, a 60–70-year period, a 400–600-year and a 8000-year period emerge as the dominant periods. 相似文献
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An analytical expression is derived for the cutoff rigidity of cosmic rays arriving at a point in an arbitrary direction, when the main geomagnetic field is approximated by that of an eccentric dipole. This expression is used to determine changes in geomagnetic cutoffs due to secular variation of the geomagnetic field since 1835. Effects of westward drift of the quadrupole field and decrease in the effective dipole moment are seen in the isorigidity contours. On account of the immense computer time required to determine the cutoff rigidities more accurately using the particle trajectory tracing technique, the present formulation may be useful in estimating the transmission factor of the geomagnetic field in cosmic ray studies, modulation of cosmogenic isotope production by geomagnetic secular variation, and the contribution of geomagnetic field variation to long term changes in climate through cosmic ray related modulation of the current flow in the global electric circuit. 相似文献
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R. Thompson 《Physics of the Earth and Planetary Interiors》1984,36(1):61-77
Spherical harmonic coefficients of the geomagnetic field, calculated from historical observations of declination, inclination and intensity, and from archaeomagnetic inclination results, have been used to produce a film of geomagnetic change since 1600 A.D. The non-dipole geomagnetic field is found to be constantly changing: no fixed or standing non-dipole features are observed. Non-dipole foci are seen to have lifetimes of a few hundred years. The westward drift, which was an important feature of the 18th and early 19th century geomagnetic field, was less pronounced in the 17th century. The growth, evolution, decay and replacement of non-dipole foci, but not their movement are found to have been the major features producing century-long secular directional magnetic variation. Most of the low degree and order spherical harmonic coefficients have changed significantly over the last few hundred years. In particular the change in sign of the axisymmetric quadrupole around 1837 A.D. is noted. Sustained, century-long, intensity changes, however, appear to have been dominated by variations in the intensity of the centred dipole, rather than by non-dipole field fluctuations. 相似文献
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地磁场的漂移运动和强度变化 总被引：4，自引：6，他引：4
在修正了Briggs提出的移动变形图案相关分析法基础上,对全球非偶极子磁场以及6个行星尺度磁异常区的漂移特性和强度变化进行了研究.结果表明,在1900-2000年期间,全球非偶极子磁场以0.15°/a的平均速度向西漂移,强度累计增长了29%;6个行星尺度异常区的西漂运动存在明显差异,其中漂移最快的是赤道附近的非洲异常,平均西漂速度为0.26°/a,其次是南半球的澳大利亚异常(0.23°/a),最慢的是欧亚异常(0.09°/a).除西漂外,大多数异常区还有较小的北向漂移.在1940-1955年期间北半球的欧亚、北美和北大西洋3个异常区以及赤道地区的非洲异常几乎同时由西漂或西南漂转为西北向漂移;紧接着,南半球的南大西洋和澳大利亚两个异常区的漂移特征也发生明显变化,主要是漂移明显减慢,而不是漂移方向的转折.在6个异常区中,澳大利亚、南大西洋、非洲和欧亚4个异常区的强度有明显增加,而北美和北大西洋两个异常区的强度则显示了减小的趋势. 相似文献
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Summary The direction of the geomagnetic field has changed substantially less in India than in Europe since the end of the 18th century.Whereas the European geomagnetic time series indicate a tendency of secular variation from which a remarkable westward drift of the non-axial field can be deduced, in India the field direction seems to have remained more or less fixed over the last two centuries. The drift of the non-axial field seems to be very small, or even eastward. 相似文献
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The dipole model of the main geomagnetic field sources has been developed by the authors for several years. At present, the model includes 13 sources that existed and continuously developed during the 20th century. It has been assumed that the main dipole motion can be related to the motion of the Earth’s axis of inertia. At the same time, the known sharp changes in the direction of this motion, the so-called “wanderings” of the axis of inertia coincide in time with a change in the coordinates of the exit point of the main dipole magnetic moment vector on the Earth’s surface, dependent mostly on changes in the vector inclination. The motion of the north magnetic pole has been studied based on the model. It has been obtained that the dynamics of the main dipole parameters and, mainly, a stable variation in the inclination of the magnetic moment vector are responsible for the westward pole motion. At the same time, the observed rapid northward motion of the pole is related to the time variations in the parameters of 12 sources approximating the so-called nondipole part of the main field. 相似文献