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A comparison of fixed- and free-positioned point mass methods for regional gravity field modeling

机译:区域重力场建模的固定和自由定位点谱系的比较

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Radial basis functions (RBFs) have been used widely for regional gravity field modeling. By using the RBFs with the point mass kernel, the RBF-based technique becomes the point mass method. The model setup of the point mass RBFs, consisting of the selection of the spectral bandwidths, depths and network, is crucial for the quality of recovered regional gravity field models. If the spectral bandwidths are defined, the point mass method can be classified into the fixed- and free-positioned methods. This study compares the two methods for modeling of regional gravity fields in a unified framework. The fixed-positioned method uses a Reuter grid to determine the RBF number and centers. The grid depth is chosen by experimenting several candidates to achieve the smallest root-mean-square (RMS) of the differences between predicted and observed values at a set of control points. The magnitudes of the RBFs are estimated by solving a linear equation system, where Tikhonov regularization is applied if the normal matrix is ill-conditioned. The free-positioned method starts with initially unknown positions of the RBFs, and also the number of RBFs is determined in the computation process. Here, we use a search process to select the RBFs automatically by means of solving a series of nonlinear problems with depth constraints on the RBFs to minimize the RMS difference between the predictions and observations. The magnitudes of all selected RBFs are later re-estimated in the least-squares sense while keeping their positions unchanged. EGM2008 coefficients are firstly used to simulate two harmonic fields to test the performance of the two methods on various Reuter grids, depth limits, and spectral bandwidths, in order to gain certain guidelines for a proper selection of the model parameters. The two methods are then applied to real gravity data sets in the Auvergne and White Sands test areas, respectively. The results reveal that the free-positioned method outperforms the fixed-positioned method in regions with rough gravity field features while using less RBFs. In regions with smooth gravity field features, both methods give similar results, where the fixed-positioned method needs more RBFs than the free-positioned method.
机译:径向基功能(RBFS)已被广泛用于区域重力场建模。通过使用具有点质量核的RBF,基于RBF的技术成为点质量方法。点质量RBFS的模型设置,包括选择光谱带宽,深度和网络,对恢复的区域重力场模型的质量至关重要。如果定义了光谱带宽,则点质量方法可以分为固定和自由定位的方法。本研究比较了统一框架中区域重力领域的两种方法。固定定位的方法使用REURER网格来确定RBF数量和中心。通过试验几个候选物来实现网格深度来实现在一组控制点处的预测和观察值之间的差异的最小根均线(RMS)。通过求解线性方程系统估计RBF的幅度,其中如果正常矩阵被释放,则施加Tikhonov正规。自由定位方法从最初的RBF的未知位置开始,并且在计算过程中确定RBF的数量。在这里,我们使用搜索过程通过求解RBF上的深度约束的一系列非线性问题来自动选择RBF,以最小化预测和观察之间的RMS差异。稍后将所有所选RBF的大小重新估计在最小方形的位置,同时保持其位置不变。 EGM2008 coefficients are firstly used to simulate two harmonic fields to test the performance of the two methods on various Reuter grids, depth limits, and spectral bandwidths, in order to gain certain guidelines for a proper selection of the model parameters.然后将这两种方法分别应用于Auvergne和白色沙子测试区域的实际重力数据集。结果表明,自由定位的方法在使用较少的RBF的同时优于具有粗糙重力场特征的区域中的固定定位方法。在具有平滑的重力场特征的区域中,两种方法提供类似的结果,其中固定定位的方法需要比自由定位方法更多的RBF。

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