A tomographic crustal velocity model of the central Fennoscandian Shield

International audience In this paper, local seismic tomographic method is used to find the terrane distribution within the central parts of the accretionary Svecofennian Orogen. This study presents a crustal P-wave velocity model, and for the first time the S-wave velocity and Vp/Vs ratio model of S...

Full description

Bibliographic Details
Published in:Geophysical Journal International
Main Authors: Hyvonen, T., Tiira, T., Korja, A., Heikkinen, P., Rautioaho, E.
Other Authors: Institute of Seismology
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2007
Subjects:
Online Access:https://hal-insu.archives-ouvertes.fr/insu-00346260
https://hal-insu.archives-ouvertes.fr/insu-00346260/document
https://hal-insu.archives-ouvertes.fr/insu-00346260/file/168-3-1210.pdf
https://doi.org/10.1111/j.1365-246X.2006.03242.x
Description
Summary:International audience In this paper, local seismic tomographic method is used to find the terrane distribution within the central parts of the accretionary Svecofennian Orogen. This study presents a crustal P-wave velocity model, and for the first time the S-wave velocity and Vp/Vs ratio model of SVEKALAPKO area that is 700 × 800 km2 in southern and central Finland. The 3-D model is presented as P- and S-wave velocity as well as Vp/Vs ratio depth slices and vertical sections. The data set comprised of several subsets of crustal Pg- and Sg-wave traveltime data: from local events recorded by the SVEKALAPKO seismic tomography array in 1998–1999, from older controlled source shots recorded at portable stations as well as at permanent stations, and from non-controlled chemical explosions recorded at permanent seismic stations. From 300 local explosions a total of 10 404 Pg-wave and 9361 Sg-wave arrival times were inverted to create independent 3-D Vp and Vs tomographic models, from which the Vp/Vs ratio was calculated. According to sensitivity tests, the optimal horizontal resolution of recognizable velocity structures in the central study area is at least 60 km down to depths of 40 km. In the final model, the seismic velocities vary smoothly. The lateral variations are larger for Vp (5.9–6.6 km s−1) than for Vs (3.5–3.8 km s−1) in the upper 20 km of the crust. At depths of 20–40 km, Vp varies from 6.5 to 7.2 km s−1 and Vs from 3.7 to 4.1 km s−1. The Vp/Vs ratio varies spatially more distinct than P- and S-wave velocities, usually from 1.70 to 1.74 in the upper crust and from 1.72 to 1.78 in the lower crust. Schist belts and their continuations at depth are associated with lower velocities and lower Vp/Vs ratios ( Vp < 6.2–6.8 km s−1 Vs < 3.6–3.9 km s−1 Vp/Vs= 1.68–1.73) than the granitoid areas (Vp= 6.3–7.4 km s−1; Vs= 3.6–4.2 km s−1; Vp/Vs= 1.72–1.78). The Svecofennian Orogen was accreted from crustal blocks ranging in size from 100 × 100 km2 to 200 × 200 km2 in cross-sectional area. The intervening ...