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The spherical Slepian basis as a means to obtain spectral consistency between mean sea level and the geoid

机译:球形斯列普基作为获得平均海平面与大地水准面之间光谱一致性的一种手段

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摘要

The mean dynamic topography (MDT) can be computed as the difference between the mean sea level (MSL) and a gravimetric geoid. This requires that both data sets are spectrally consistent. In practice, it is quite common that the resolution of the geoid data is less than the resolution of the MSL data, hence, the latter need to be low-pass filtered before the MDT is computed. For this purpose conventional low-pass filters are inadequate, failing in coastal regions where they run into the undefined MSL signal on the continents. In this paper, we consider the use of a bandlimited, spatially concentrated Slepian basis to obtain a low-resolution approximation of the MSL signal. We compute Slepian functions for the oceans and parts of the oceans and compare the performance of calculating the MDT via this approach with other methods, in particular the iterative spherical harmonic approach in combination with Gaussian low-pass filtering, and various modifications. Based on the numerical experiments, we conclude that none of these methods provide a low-resolution MSL approximation at the sub-decimetre level. In particular, we show that Slepian functions are not appropriate basis functions for this problem, and a Slepian representation of the low-resolution MSL signal suffers from broadband leakage. We also show that a meaningful definition of a low-resolution MSL over incomplete spherical domains involves orthogonal basis functions with additional properties that Slepian functions do not possess. A low-resolution MSL signal, spectrally consistent with a given geoid model, is obtained by a suitable truncation of the expansions of the MSL signal in terms of these orthogonal basis functions. We compute one of these sets of orthogonal basis functions using the Gram–Schmidt orthogonalization for spherical harmonics. For the oceans, we could construct an orthogonal basis only for resolutions equivalent to a spherical harmonic degree 36. The computation of a basis with a higher resolution fails due to inherent instabilities. Regularization reduces the instabilities but destroys the orthogonality and, therefore, provides unrealistic low-resolution MSL approximations. More research is needed to solve the instability problem, perhaps by finding a different orthogonal basis that avoids it altogether
机译:可以将平均动态地形(MDT)计算为平均海平面(MSL)与重力大地水准面之间的差。这要求两个数据集在光谱上保持一致。在实践中,大地水准面数据的分辨率小于MSL数据的分辨率是很常见的,因此,在计算MDT之前,需要对后者进行低通滤波。为此目的,常规的低通滤波器是不够的,在沿海地区遇到大陆上未定义的MSL信号时会失效。在本文中,我们考虑使用带限,空间集中的Sleepian基来获得MSL信号的低分辨率近似值。我们计算海洋和部分海洋的Slepian函数,并将通过此方法与其他方法(特别是迭代球谐方法与高斯低通滤波相结合)和各种修改方法计算MDT的性能进行比较。根据数值实验,我们得出的结论是,这些方法均未提供亚分米级的低分辨率MSL近似值。尤其是,我们表明,Slepian函数不适用于该问题,并且低分辨率MSL信号的Slepian表示会遭受宽带泄漏。我们还表明,对不完整球形域的低分辨率MSL的有意义定义涉及正交基函数以及具有Slepian函数不具备的其他属性。通过根据这些正交基函数对MSL信号的展开进行适当的截断,可以获得与给定的大地水准面模型在频谱上一致的低分辨率MSL信号。我们使用针对球谐函数的Gram–Schmidt正交化来计算其中一组正交基函数。对于海洋,我们只能为与球谐度36等效的分辨率构建正交基础。由于固有的不稳定性,因此无法以更高的分辨率计算基础。正则化减少了不稳定性,但破坏了正交性,因此提供了不切实际的低分辨率MSL近似值。需要进行更多的研究来解决不稳定性问题,可能是找到一个完全避免这种不稳定性的正交基础。

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