Abstract

We investigate the gravity gradient components corrected for major known anomalous density structures within the Earth's crust. Heterogeneous mantle density structures are disregarded. The gravimetric forward modeling technique is utilized to compute the gravity gradients based on methods for a spherical harmonic analysis and synthesis of a gravity field. The Earth's gravity gradient components are generated using the global geopotential model GOCO-03s. The topographic and stripping gravity corrections due to the density contrasts of the ocean and ice are computed from the global topographic/bathymetric model DTM2006.0 (which also includes the ice-thickness dataset). The discrete data of sediments and crust layers taken from the CRUST2.0 global crustal model are then used to apply the additional stripping corrections for sediments and remaining anomalous crustal density structures. All computations are realized globally on a one arc-deg geographical grid at a mean satellite elevation of 255 km. The global map of the consolidated crust-stripped gravity gradients reveals distinctive features which are attributed to global tectonics, lithospheric plate configuration, lithosphere structure and mantle dynamics (e.g., glacial isostatic adjustment, mantle convection). The Moho signature, which is the most pronounced signal in these refined gravity gradients, is superimposed over a weaker gravity signal of the lithospheric mantle. An interpretational quality of the computed (refined) gravity gradient components is mainly limited by a low accuracy and resolution of the CRUST2.0 sediment and crustal layer data and unmodeled mantle structures.

Highlights

  • When studying the Moho density interface based on gravity field analysis and inversion, the topographic, bathymetric and additional corrections which account for anomalous mass density structures within the Earth’s crust are applied to observed gravity data

  • Robert Tenzer & Pavel Novák improved their application in various scientific fields: the CHAllenging Mini-satellite Payload (CHAMP) launched in 2000, the GRavity field and Climate Experiment (GRACE) launched in 2002, and the Gravity field and steady-state Ocean Circulation Explorer (GOCE) launched in 2009

  • The GOCE gravity gradiometry significantly improved the gravity field at medium wavelengths from about 100 to 250 of spherical harmonics, but it is relatively inaccurate at long wavelengths

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Summary

Introduction

When studying the Moho density interface based on gravity field analysis and inversion, the topographic, bathymetric and additional corrections which account for anomalous mass density structures within the Earth’s crust are applied to observed gravity data (see e.g., Sjöberg and Bagherbandi 2011; Sampietro et al 2013). In geophysics, this step is known as gravity stripping (e.g., Hammer 1963). Robert Tenzer & Pavel Novák improved their application in various scientific fields: the CHAllenging Mini-satellite Payload (CHAMP) launched in 2000, the GRavity field and Climate Experiment (GRACE) launched in 2002, and the Gravity field and steady-state Ocean Circulation Explorer (GOCE) launched in 2009 The combined CHAMP/GRACE/GOCE gravity field solutions have the ability to extend current knowledge concerning the Earth’s inner density structures especially beneath oceanic and continental areas where seismic data are not yet available or their accuracy and spatial coverage is inadequate

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