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Local recovery of sub-crustal stress due to mantle convection from satellite-to-satellite tracking data
University of West Bohemia, NTIS - New Technologies for the Information Society, Faculty of Applied Sciences, Plzeň, Czech Republic.
University West, Department of Engineering Science, Division of Computer, Electrical and Surveying Engineering.ORCID iD: 0000-0003-0067-8631
2016 (English)In: Acta Geophysica, ISSN 1895-6572, E-ISSN 1895-7455, Vol. 64, no 4, p. 904-929Article in journal (Refereed) Published
Abstract [en]

Two integral transformations between the stress function, differentiation of which gives the meridian and prime vertical components of the sub-crustal stress due to mantle convection, and the satellite-to-satellite tracking (SST) data are presented in this article. In the first one, the SST data are the disturbing potential differences between twin-satellites and in the second one the line-of-sight (LOS) gravity disturbances. It is shown that the corresponding integral kernels are well-behaving and therefore suitable for inversion and recovery of the stress function from the SST data. Recovery of the stress function and the stress components is also tested in numerical experiments using simulated SST data. Numerical studies over the Himalayas show that inverting the disturbing potential differences leads to a smoother stress function than from inverting LOS gravity disturbances. Application of the presented integral formulae allows for recovery of the stress from the satellite mission GRACE and its planned successor. © 2016 Šprlak and Eshagh.

Place, publisher, year, edition, pages
2016. Vol. 64, no 4, p. 904-929
Keywords [en]
GRACE satellite mission; integral equation; integral kernel; stress function; truncation error; upward/downward continuation
National Category
Geophysics
Research subject
ENGINEERING, Geodesy
Identifiers
URN: urn:nbn:se:hv:diva-8172DOI: 10.1515/acgeo-2016-0044ISI: 000382229800004Scopus ID: 2-s2.0-84984998996OAI: oai:DiVA.org:hv-8172DiVA, id: diva2:855202
Note

Funders: Czech Science Foundation, GA15-08045S.

Available from: 2015-09-19 Created: 2015-09-19 Last updated: 2019-12-03Bibliographically approved

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Eshagh, Mehdi

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