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On the Comparison of Radial Base Functions and Single Layer Density Representations in Local Gravity Field Modelling from Simulated Satellite Observations

机译:基于模拟卫星观测的局部重力场建模中径向基函数与单层密度表示的比较

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摘要

The recovery of local (time-variable) gravity features from satellite-to-satellite tracking missions is one of the current challenges in Geodesy. Often, a global spherical harmonic analysis is used and the area of interest is selected later on. However, this approach has deficiencies since leakage and incomplete recovery of signal are common side effects. In order to make better use of the signal content, a gravity recovery using localizing base functions can be employed. In this paper, two different techniques are compared in a case study using simulated potential observations at satellite level – namely position-optimized radial base functions and a single layer representation using a piecewise continuous density. The first one is the more common approach. Several variants exist which mainly differ in the choice of the position of the base function and the regularization method. Here, the position of each base is subject to an adjustment process. On the other hand, the chosen radial base functions are developed as a series of Legendre functions which still have a global support although they decay rapidly. The more rigorous approach is to use base functions with a strictly finite support. One possible choice is a single layer representation whereas the density is discretized by basic shapes like triangles, rectangles, or higher order elements. Each type of shape has its own number of nodes. The higher the number of nodes of a particular element, the more complicated becomes the solution strategy but at the same time the regularity of the solution increases. Here, triangles are used for the comparison. As a result, the radial base functions in the employed variant allow a modeling with a minimum number of parameters but do not achieve the same level of approximation as the discretized single layer representation. The latter do so at the cost of a higher number of parameters and regularization. This case study offers an interesting comparison of a near localizing with a strictly localizing base function. However, results can currently not be generalized as other variants of the radial base functions might perform better. Also, the extension to a GRACE-type observable is desirable.
机译:从卫星到卫星的跟踪任务中恢复局部(随时间变化)重力特征是大地测量学当前的挑战之一。通常,使用全局球谐分析,然后选择感兴趣的区域。但是,这种方法有缺陷,因为泄漏和信号恢复不完全是常见的副作用。为了更好地利用信号内容,可以采用利用局部基本函数的重力恢复。本文在案例研究中使用卫星水平的模拟潜在观测结果对两种不同的技术进行了比较,即位置优化的径向基函数和使用分段连续密度的单层表示。第一个是更常见的方法。存在几种变体,它们的主要区别在于基本函数位置和正则化方法的选择。在此,每个基座的位置都要经过调整处理。另一方面,选定的径向基函数被开发为一系列的勒让德函数,尽管它们迅速衰减,但仍具有全局支持。更严格的方法是在严格有限的支持下使用基本函数。一种可能的选择是单层表示,而密度通过基本形状(例如三角形,矩形或更高阶元素)离散化。每种形状都有其自己的节点数。特定元素的节点数量越多,求解策略就越复杂,但同时解决方案的规则性也增加。这里,三角形用于比较。结果,所采用的变体中的径向基函数允许使用最少数量的参数进行建模,但无法达到与离散化单层表示相同的逼近度。后者这样做的代价是需要更多的参数和进行正则化。这个案例研究提供了一个有趣的比较,一个严格定位的基本功能的近定位。但是,由于径向基函数的其他变体可能会更好地执行,因此当前无法将结果进行概括。同样,希望扩展到GRACE类型的可观察对象。

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