GEODYNAMICS

IF 1 Q3 GEOCHEMISTRY & GEOPHYSICS
M. Fys, A. Brydun, A. Vovk
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引用次数: 0

Abstract

The conventional approach to constructing a three-dimensional distribution of the Earth's masses involves using Stokes constants incrementally up to a certain order. However, this study proposes an algorithm that simultaneously considers all of these constants, which could potentially provide a more efficient method. The basis for this is a system of equations obtained by differentiating the Lagrange function, which takes into account the minimum deviation of the three-dimensional mass distribution of the planet's subsoil from one-dimensional referential one. An additional condition, apart from taking into account the Stokes constants, for an unambiguous solution to the problem is to specify the value of the function on the surface of the ellipsoidal planet. It is possible to simplify the calculation process by connecting the indices of summation values in a series of expansions to their one-dimensional analogues in the system of linear equations. The study presents a control example illustrating the application of the given algorithm. In its implementation, a simplified variant of setting the density on the surface of the ocean is taken. The preliminary results of calculations confirm the expediency of this approach and the need to expand such a technique with other conditions for unambiguously solving the inverse problem of potential theory. Objectives. To create and implement the algorithm that takes into account the density of the planet’s subsoil on its surface. Method. The mass distribution function of the planet's subsoil is represented by a decomposition into biorthogonal series, the coefficients of decomposition which are determined from a system of linear equations. The system of equations is obtained from the condition of minimizing the deviation function of the desired mass distribution from the initially determined two-dimensional density distribution (PREM reference model). Results. On the basis of the described algorithm, a three-dimensional model of the density distribution of subsoil masses in the middle of the Earth is obtained, which takes into account Stokes constants up to the eighth order inclusively and corresponds to the surface distribution of masses of the oceanic model of the Earth. Its concise interpretation is also presented.
运动学
构建地球质量三维分布的传统方法涉及使用斯托克斯常数递增到一定阶次。然而,本研究提出了一种同时考虑所有这些常数的算法,这有可能提供一种更有效的方法。其基础是通过微分拉格朗日函数得到的方程组,该方程组考虑了行星底土三维质量分布与一维参考质量分布的最小偏差。除了考虑斯托克斯常数外,要明确地解决这个问题,还有一个条件,那就是指定椭圆形行星表面的函数值。通过将一系列展开式中的求和值指数与其线性方程组中的一维类似值联系起来,可以简化计算过程。本研究提供了一个控制实例,说明了给定算法的应用。在实施过程中,对海洋表面密度的设置进行了简化。计算的初步结果证实了这一方法的便捷性,并证明有必要将这一技术扩展到其他条件,以明确解决势理论的逆问题。目标。建立并实施考虑到行星表面底土密度的算法。方法。行星底土的质量分布函数通过分解为双正交序列来表示,分解系数由线性方程组确定。该方程组的条件是使所需质量分布与最初确定的二维密度分布(PREM 参考模型)的偏差函数最小化。结果在所述算法的基础上,获得了地球中部底土质量密度分布的三维模型,该模型考虑了斯托克斯常数(含八阶),并与地球海洋模型的表面质量分布相对应。同时还给出了简明的解释。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Geodynamics
Geodynamics GEOCHEMISTRY & GEOPHYSICS-
自引率
33.30%
发文量
11
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