Open Session - SWISS GEOSCIENCE MEETINGs
Open Session - SWISS GEOSCIENCE MEETINGs
Open Session - SWISS GEOSCIENCE MEETINGs
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Symposium 1: Structural Geology, Tectonics and Geodynamics<br />
1.<br />
Transitions in tectonic mode based on calculations of self-consistent<br />
plate tectonics in a 3D spherical shell<br />
van Heck Hein* & Tackley Paul*<br />
*Institute of Geophysics, Schafmattstrasse 30, CH-8093 Zuerich (hvanheck@erdw.ethz.ch)<br />
In the past decade, several studies have documented the effectiveness of plastic yielding in causing a basic approximation of<br />
plate tectonic behavior in mantle convection models with strongly temperature dependent viscosity, strong enough to form<br />
a rigid lid in the absence of yielding. The vast majority of such research to date has been in either two-dimensional, or threedimensional<br />
cartesian geometry. Also, scalings for mixed internally and bottom heated convection are not well established.<br />
In the present study, mantle convection calculations are done to investigate the planforms of self consistent tectonic plates<br />
in three-dimensional spherical geometry. Several diagnostics are used to analyze how successful each model is in producing<br />
tectonic plates. We study the proposed transitions in tectonic mode (e.g. changes in plate size, rigid lid convection to tectonic<br />
plates, smoothly evolving plates to more episodic, time dependent, tectonics) as a function of yield stress envelope,<br />
Rayleigh number and heating mode.<br />
Cases with zero bottom heat flux are compared to cases which have both internal heating and bottom heating. This enables<br />
us to investigate which tectonic mode prevails as function of lithospheric yield stress, Ra and heating mode. The results are<br />
compared to analytical scalings for boundary regimes as well as scalings for heat flux. This allows us to scale to different<br />
planets of different sizes and can be applied to the evolution of Earth, Mars and Venus as well as terrestrial extra-solar planets.<br />
1. 8<br />
Late Quaternary slip rates of active faults adjacent lake Qinghai,<br />
northeastern margin of the Tibetan Plateau<br />
Yuan Dao-Yang*, Champagnac Jean-Daniel**, Ge Wei-Peng*, Molnar Peter***, Zhang Pei-Zhen****, Zheng Wen-Jun****, Zhang<br />
Hui-Ping****, Liang Ming-Jian*<br />
* Lanzhou Institute of Seismology, China Earthquake Administration, Lanzhou 730000, China<br />
** Institute of Mineralogy, University of Hannover, Callinstrasse 3, Hannover D-30167, Germany<br />
*** Department of Geological Sciences, and CIRES, University of Colorado, Boulder, Colorado, 80309, USA<br />
**** State Key Laboratory of Earthquake Dynamics, Institute of Geology, China Earthquake Administration, Beijing 100029, China<br />
Combining the terrace riser offsets with terrace ages dated by 14 C, OSL and 10 Be techniques, we determine average strike slip<br />
rates of Elashan and Riyueshan faults, two north-northwest-trending strike-slip faults along the western and eastern sides of<br />
the lake Qinghai, northeastern margin of the Tibetan plateau, to be about 1.0 ± 0.2 mm/yr and 1.2 ± 0.2 mm/yr, respectively.<br />
Between them, the Qinghainanshan fault consists of three secondary thrust faults, whose total vertical slip rate and shortening<br />
rate are ≈0.4-1.0 mm/yr and ≈0.2-1.2 mm/yr, respectively.<br />
The relatively low slip rates in this region reflect distributed deformation. The total right-lateral offsets of the geological<br />
contacts, which were interpreted from 1:200,000-scale Qinghai regional geological maps of the region, are about 8.8-11.9 km<br />
along the Elashan fault and 10.9-11.6 km for the northern segment of Riyueshan fault. If long–term slip rates were constant<br />
during late Cenozoic time, initiation of dextral movement would be 10.3 ± 3.6 Ma and 9.4±2.3 Ma for the two strike-slip faults,<br />
consistent with records of tectonic deformation in Cenozoic basins nearby.<br />
Our study highlights a stage of tectonic deformation in the northeastern margin the Tibetan plateau beginning near ≈10 Ma,<br />
long after the collision between India and Eurasia began.