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Licensed Unlicensed Requires Authentication Published by De Gruyter September 14, 2017

Towards the Moho depth and Moho density contrast along with their uncertainties from seismic and satellite gravity observations

M. Abrehdary, L.E. Sjöberg, M. Bagherbandi and D. Sampietro

Abstract

We present a combined method for estimating a new global Moho model named KTH15C, containing Moho depth and Moho density contrast (or shortly Moho parameters), from a combination of global models of gravity (GOCO05S), topography (DTM2006) and seismic information (CRUST1.0 and MDN07) to a resolution of 1° × 1° based on a solution of Vening Meinesz-Moritz’ inverse problem of isostasy. This paper also aims modelling of the observation standard errors propagated from the Vening Meinesz-Moritz and CRUST1.0 models in estimating the uncertainty of the final Moho model. The numerical results yield Moho depths ranging from 6.5 to 70.3 km, and the estimated Moho density contrasts ranging from 21 to 650 kg/m3, respectively. Moreover, test computations display that in most areas estimated uncertainties in the parameters are less than 3 km and 50 kg/m3, respectively, but they reach to more significant values under Gulf of Mexico, Chile, Eastern Mediterranean, Timor sea and parts of polar regions. Comparing the Moho depths estimated by KTH15C and those derived by KTH11C, GEMMA2012C, CRUST1.0, KTH14C, CRUST14 and GEMMA1.0 models shows that KTH15C agree fairly well with CRUST1.0 but rather poor with other models. The Moho density contrasts estimated by KTH15C and those of the KTH11C, KTH14C and VMM model agree to 112, 31 and 61 kg/m3 in RMS. The regional numerical studies show that the RMS differences between KTH15C and Moho depths from seismic information yields fits of 2 to 4 km in South and North America, Africa, Europe, Asia, Australia and Antarctica, respectively.

Funding source: Swedish National Space Board

Award Identifier / Grant number: 116/12

Funding statement: This study was supported by projects no. 116/12 of the Swedish National Space Board (SNSB).

Acknowledgment

The authors would like to appreciate this organization for financial support. Mr. Alexey Baranov from Russian Academy of Sciences is acknowledged for providing some regional Moho depth models.

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Received: 2017-5-10
Accepted: 2017-7-24
Published Online: 2017-9-14
Published in Print: 2017-12-1

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