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|Title:||Comparing gravity-based to seismic-derived lithosphere densities: a case study of the British Isles and surrounding areas|
|Authors:||Root, B. C.|
van der Wal, W.
England, R. W.
Vermeersen, L. L. A.
|Publisher:||Oxford University Press (OUP), Royal Astronomical Society|
|Citation:||Geophysical Journal International, 2017, 208(3), pp. 1796-1810.|
|Abstract:||Lithospheric density structure can be constructed from seismic tomography, gravity modelling, or studies using both data sets. The different approaches have their own uncertainties and limitations. This study aims to characterise and quantify the uncertainties in gravity modelling of lithosphere densities. To evaluate the gravity modelling we compare between the gravity-based and lithosphere densities based on seismic velocities. This study proposes a new gravity modelling approach to estimate lithosphere densities,using a crustal model, lithospheric isostasy, and gravity field observations. To quantify the effect of uncertainty in the crustal model, three models are implemented in this study: CRUST1.0, EuCrust-07, and a high resolution P-wave velocity model of the British Isles and surrounding areas. Different P-wave velocity-to-density conversions are used to study the uncertainty in these conversion methods. The crustal density models are forward modelled into gravity field quantities using a method that is able to produce spherical har1monic coefficients. Deep mantle signal is assumed to be removed by removing spherical harmonic coefficients of degree 0-10 in the observed gravity field. The uncertainty in the resulting lithosphere densities due to the different crustal models is ±110 kg/m3, which is the largest uncertainty in gravity modelling. Other sources of uncertainty, such as the VP to density conversion (±10 kg/m3), long-wavelength truncation (±5 kg/m3), choice of reference model (< ±20 kg/m3), and Lithosphere Asthenosphere Boundary uncertainty (±30 kg/m3), proved to be of lesser importance. The resulting lithosphere density solutions are compared to density models based on a shear wave velocity model [Schaeffer and Lebedev(2013)]. The comparison shows that the gravity-based models have an increased lateral resolution compared to the tomographic solutions. However, the density anomalies of the gravity-based models are threetimes higher. This is mainly due to the high resolution in the gravity field. To account for this, the gravity-based density models are filtered with a spatial Gaussian filter with 200 km halfwidth, which results in similar density estimates (±35 kg/m3) with the tomographic approach. Lastly, the gravity-based density is used to estimate laterally varying conversion factors, which show to correlate with major tectonic regions. The independent gravity-based solutions could help in identifying different compositional domains in the lithosphere, when compared to the tomographic solutions.|
|Rights:||Copyright © 2016, Oxford University Press (OUP), Royal Astronomical Society. Deposited with reference to the publisher’s open access archiving policy.|
|Appears in Collections:||Published Articles, Dept. of Geology|
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