Efficient 3D large-scale forward-modeling and inversion of gravitational fields in spherical coordinates with application to lunar mascons

Abstract

An efficient forward modeling algorithm for calculation of gravitational fields in spherical coordinates is developed for 3D large‐scale gravity inversion problems. 3D Gauss‐Legendre quadrature (GLQ) is used to calculate the gravitational fields of mass distributions discretized into tesseroids. Equivalence relations in the kernel matrix of the forward‐modeling are exploited to decrease storage and computation time. The numerical tests demonstrate that the computation time of the proposed algorithm is reduced by approximately two orders of magnitude, and the memory requirement is reduced by N'λ times compared with the traditional GLQ method, where N'λ is the number of the model elements in the longitudinal direction. These significant improvements in computational efficiency and storage make it possible to calculate and store the dense Jacobian matrix in 3D large‐scale gravity inversions. The equivalence relations can be applied to the Taylor series method or combined with the adaptive discretization to ensure high accuracy. To further illustrate the capability of the algorithm, we present a regional synthetic example. The inverted results show density distributions consistent with the actual model. The computation took about 6.3 hours and 0.88 GB of memory compared with about a dozen days and 245.86 GB for the traditional 3D GLQ method. Finally, the proposed algorithm is applied to the gravity field derived from the latest lunar gravity model GL1500E. 3D density distributions of the Imbrium and Serenitatis basins are obtained, and high‐density bodies are found at the depths 10‐60 km, likely indicating a significant uplift of the high‐density mantle beneath the two mascon basins.

Moho Beneath Tibet Based on a Joint Analysis of Gravity and Seismic Data

“…The EIGEN‐6C4 model (Förste et al, , http://icgem.gfz-potsdam.de/tom_longtime) to degree and order 720 is used to compute the free‐air gravity disturbances at the elevation 10 km refer to the GRS80 reference ellipsoid (Figure b). The gravity effects (Figure c) of the topography (Figure a) derived from ETOPO1 (Amante & Eakins, ) are calculated globally (Zhao et al, ) with the correction density of 2,670 kg/m 3 . The Bouguer gravity disturbances (Figure d) are obtained by removing the gravity effect of the topography from the free‐air gravity disturbances.…”