共查询到18条相似文献,搜索用时 51 毫秒
1.
2.
陈伯舫 《地震地磁观测与研究》1995,16(4):18-21
地面Sq磁场的分析在一定程度上可揭示场向电流的存在。本文将Sq资料按1/2(夏-冬)的方法定性地显示了空间等效电流的分布。结果表明:在夏、冬季清晨由夏季半球流向冬季半球的场向电流特别明显,可是黄昏时的场向电流似乎不存在,踵时由冬季半球流向夏季半球的场向电流强度反而比清晨场向电流弱一些。 相似文献
3.
根据IGY/IGC期间全球地磁台网以及中国地磁台站的资料,计算出每-UT小时的Sq外源和内源电流体系.对Sq电流体系UT变化和经度效应的分析研究表明,Sq外源电流体系的空间图案没有显著的UT变化,电流涡焦点的地理纬度与磁赤道有密切关系,其变化范围,北半球为25°-35°N,南半球为30°-42.5°S.外源电流总强度的平均值为229kA(北半球)和173kA(南半球),其变化范围为±50kA(北半球)和±40kA(南半球).Sq内源电流体系的图案和强度有显著的UT变化,电流体系焦点纬度有类似于外源电流系的变化.在大西洋、印度洋、北太平洋地区,内源电流体系的总强度明显小于大陆地区的内源电流强度,表明这些大洋地区上地幔电导率低于大陆地区. 相似文献
4.
5.
陈伯舫 《地震地磁观测与研究》1996,17(2):44-49
地面Sq磁场的分析在一定程度上揭示场向电流的存在,在赤道电射流区和低纬地区,某些日子的Y分量或D分量Sq变化可明显地显示午间场向电流的存在,1990年12月11日Baclieu,琼中,河内,Chapa,通海和成都等台的Sq(I)曲线清楚表明由冬季半球流向夏季半球的午间场向电流的影响,此外,本文还用(夏-冬)/2法分析了Sq(Z)的资料,从中也可观察到午间及清晨场向电流的踪迹。 相似文献
6.
本文分析了电离层风发电机理论中影响电流分布的几种主要因素,认为电离层电导率模型是最主要的影响因素。在计算太阴日变化(L)电流体系时,本文放弃了过去习惯采用的无限薄球壳的电导率模型,使用了分层电导率模型。考虑电导率随高度的变化以及电导率极大值的高度随纬度的变化,得到了与观测结果较为符合的理论L电流体系。本文的结果还指出,在处理某些全球性发电机理论问题时,不能简单地假定电离层为距地面等高度的无限薄球壳,而必须同时考虑大气潮汐振荡的特性及电导率随高度的变化。由此得出结论:发展三维电导率模型对于电离层风发电机理论是必要的。 相似文献
7.
利用地磁内外源场分离的方法,反演得到了1997年11月8日玛尼地震和1998年1月10日张北地震前地下和空间等效电流体系的演化图象,并分析研究了地磁低点位移出现前后等效电流体系变化特征.结果表明,内、外场等效电流体系的变化与地震ldquo;低点位移rdquo;异常现象有着内在的联系,等效电流体系变化可能是地磁低点位移异常现象产生的原因之一。随着我国地磁台站的加密建设,势必可以得到更为精确的地磁场等效电流体系的演化特征,更有利于地震预测的研究。 相似文献
8.
9.
在地理坐标系下推导出二维电离层发电机理论方程,采用逐线迭代法求解得到全球二维电离层发电机电流函数,进而得到电离层发电机电流和电场.模式中使用的电导率是根据外部经验模式给出的背景大气和电离层参数,采用理论公式计算得出;输入的中性风场和磁场分别由HWM93和IGRF2000模型给出,该电离层发电机理论模式很好地给出了全球Sq电流形态及电离层E层发电机电场的基本特征.利用该模式研究了外部模式风场以及地磁场随高度的变化对模拟结果的影响,发现在90~180 km高度上,风场随高度变化对电流影响较大,而地磁场影响较小;重点模拟研究了地磁平静时期,Sq电流涡旋中心位置和总电流强度的变化规律,初步研究发现,电流中心位置在地理纬度±30°附近,不同的地方时电流随地磁纬度线平行移动,且南北半球两个电流涡中心电流强度之和变化不大.分析发现这种规律与发电机高度上的磁场总强度及地磁倾角的全球分布有很好的相关性. 相似文献
10.
用中国地磁台站的资料,研究了S_q逐日变化的形态学特征,用理论模型计算了磁层环电流、部分环电流、场向电流、磁尾电流、Chapman-Ferraro电流的地磁效应.在消除了这些磁层电流体系的影响之后,得到了电离层潮汐风发电机电流产生的磁场S_q变化.对1973年的资料研究表明,S_q发电机电流的逐日变化主要表现在强度上,即使在磁扰期间,也可以分离出形态稳定的S_q变化.由此提出了一种新的地磁指数——S_q指数,用来描述S_q发电机电流强度的逐日变化. 相似文献
11.
12.
13.
John V. Shebalin 《地球物理与天体物理流体动力学》2013,107(3):353-375
We consider an unforced, incompressible, turbulent magnetofluid constrained by concentric inner and outer spherical surfaces. We define a model system in which normal components of the velocity, magnetic field, vorticity, and electric current are zero on the boundaries. This choice allows us to find a set of Galerkin expansion functions that are common to both velocity and magnetic field, as well as vorticity and current. The model dynamical system represents magnetohydrodynamic (MHD) turbulence in a spherical domain and is analyzed by the methods similar to those applied to homogeneous MHD turbulence. We find a statistical theory of ideal (i.e. no dissipation) MHD turbulence analogous to that found in the homogeneous case, including the prediction of coherent structure in the form of a large-scale quasistationary magnetic field. This MHD dynamo depends on broken ergodicity, an effect that is enhanced when total magnetic helicity is increased relative to total energy. When dissipation is added and large scales are only weakly damped, quasiequilibrium may occur for long periods of time, so that the ideal theory is still pertinent on a global scale. Over longer periods of time, the selective decay of energy over magnetic helicity further enhances the effects of broken ergodicity. Thus, broken ergodicity is an essential mechanism and relative magnetic helicity is a critical parameter in this model MHD dynamo theory. 相似文献
14.
The induction equation of magnetohydrodynamics (MHD) is mathematically equivalent to a system of integral equations for the magnetic field in the bulk of the fluid and for the electric potential at its boundary. We summarize the recent developments concerning the numerical implementation of this scheme and its applications to various forward and inverse problems in dynamo theory and applied MHD. 相似文献
15.
16.
17.
18.
Three-Dimensional Electromagnetic Modelling and Inversion from Theory to Application 总被引:12,自引:1,他引:11
The whole subject of three-dimensional (3-D) electromagnetic (EM) modelling and inversion has experienced a tremendous progress
in the last decade. Accordingly there is an increased need for reviewing the recent, and not so recent, achievements in the
field. In the first part of this review paper I consider the finite-difference, finite-element and integral equation approaches
that are presently applied for the rigorous numerical solution of fully 3-D EM forward problems. I mention the merits and
drawbacks of these approaches, and focus on the most essential aspects of numerical implementations, such as preconditioning
and solving the resulting systems of linear equations. I refer to some of the most advanced, state-of-the-art, solvers that
are today available for such important geophysical applications as induction logging, airborne and controlled-source EM, magnetotellurics,
and global induction studies. Then, in the second part of the paper, I review some of the methods that are commonly used to
solve 3-D EM inverse problems and analyse current implementations of the methods available. In particular, I also address
the important aspects of nonlinear Newton-type optimisation techniques and computation of gradients and sensitivities associated
with these problems. 相似文献