TY - JOUR A1 - Astudillo-Sotomayor, Luis A1 - Jara Muñoz, Julius A1 - Melnick, Daniel A1 - Cortés‐Aranda, Joaquín A1 - Tassara, Andrés A1 - Strecker, Manfred T1 - Fast Holocene slip and localized strain along the Liquiñe-Ofqui strike-slip fault system, Chile JF - Scientific reports N2 - In active tectonic settings dominated by strike-slip kinematics, slip partitioning across subparallel faults is a common feature; therefore, assessing the degree of partitioning and strain localization is paramount for seismic hazard assessments. Here, we estimate a slip rate of 18.8 +/- 2.0 mm/year over the past 9.0 +/- 0.1 ka for a single strand of the Liquirie-Ofqui Fault System, which straddles the Main Cordillera in Southern Chile. This Holocene rate accounts for similar to 82% of the trench-parallel component of oblique plate convergence and is similar to million-year estimates integrated over the entire fault system. Our results imply that strain localizes on a single fault at millennial time scale but over longer time scales strain localization is not sustained. The fast millennial slip rate in the absence of historical Mw> 6.5 earthquakes along the Liquine-Ofqui Fault System implies either a component of aseismic slip or Mw similar to 7 earthquakes involving multi-trace ruptures and > 150-year repeat times. Our results have implications for the understanding of strike-slip fault system dynamics within volcanic arcs and seismic hazard assessments. KW - Geodynamics KW - Geomorphology KW - Tectonics Y1 - 2021 U6 - https://doi.org/10.1038/s41598-021-85036-5 SN - 2045-2322 VL - 11 IS - 1 PB - Macmillan Publishers Limited, part of Springer Nature CY - London ER - TY - JOUR A1 - Smith, Adam G. G. A1 - Fox, Matthew A1 - Schwanghart, Wolfgang A1 - Carter, Andrew T1 - Comparing methods for calculating channel steepness index JF - Earth science reviews : the international geological journal bridging the gap between research articles and textbooks N2 - Channel steepness index, k(s), is a metric derived from the stream power model that, under certain conditions, scales with relative rock uplift rate. Channel steepness index is a property of rivers, which can be relatively easily extracted from digital elevation models (DEMs). As DEM data sets are widely available for Earth and are becoming more readily available for other planetary bodies, channel steepness index represents a powerful tool for interpreting tectonic processes. However, multiple approaches to calculate channel steepness index exist. From this several important questions arise; does choice of approach change the values of channel steepness index, can values be so different that choice of approach can influence the findings of a study, and are certain approaches better than others? With the aid of a synthetic river profile and a case study from the Sierra Nevada, California, we show that values of channel steepness index vary over orders of magnitude according to the methodology used in the calculation. We explore the limitations, advantages and disadvantages of the key approaches to calculating channel steepness index, and find that choosing an appropriate approach relies on the context of a study. Given these observations, it is important that authors acknowledge the methodology used to calculate channel steepness index, to ensure that results can be contextualised and reproduced. KW - Channel steepness index KW - Fluvial geomorphology KW - Rivers KW - Tectonics KW - Geomorphology KW - Digital elevation models KW - Sierra nevada Y1 - 2022 U6 - https://doi.org/10.1016/j.earscirev.2022.103970 SN - 0012-8252 SN - 1872-6828 VL - 227 PB - Elsevier CY - Amsterdam ER - TY - JOUR A1 - Yang, Wei A1 - Dupont-Nivet, Guillaume A1 - Jolivet, Marc A1 - Guo, Zhaojie A1 - Bougeois, Laurie A1 - Bosboom, Roderic A1 - Zhang, Ziya A1 - Zhu, Bei A1 - Heilbronn, Gloria T1 - Magnetostratigraphic record of the early evolution of the southwestern Tian Shan foreland basin (Ulugqat area), interactions with Pamir indentation and India-Asia collision JF - Tectonophysics : international journal of geotectonics and the geology and physics of the interior of the earth N2 - The Tian Shan range is an inherited intracontinental structure reactivated by the far-field effects of the India-Asia collision. A growing body of thermochronology and magnetostratigraphy datasets shows that the range grew through several tectonic pulses since similar to 25 Ma, however the early Cenozoic history remains poorly constrained. The time-lag between the Eocene India-Asia collision and the Miocene onset of Tian Shan exhumation is particularly enigmatic. This peculiar period is potentially recorded along the southwestern Tian Shan piedmont. There, late Eocene marine deposits of the proto-Paratethys epicontinental sea transition to continental foreland basin sediments of unknown age were recently dated. We provide magnetostratigraphic dating of these continental sediments from the 1700-m-thick Mine section integrated with previously published detrital apatite fission track and U/Pb zircon ages. The most likely correlation to the geomagnetic polarity time scale indicates an age span from 20.8 to 13.3 Ma with a marked increase in accumulation rates at 19-18 Ma. This implies that the entire Oligocene period is missing between the last marine and first continental sediments, as suggested by previous southwestern Tian Shan results. This differs from the southwestern Tarim basin where Eocene marine deposits are continuously overlain by late Eocene-Oligocene continental sediments. This supports a simple evolution model of the western Tarim basin with Eocene-Oligocene foreland basin activation to the south related to northward thrusting of the Kunlun Shan, followed by early Miocene activation of northern foreland basin related to overthrusting of the south Tian Shan. Our data also support southward propagation of the Tian Shan piedmont from 20 to 18 Ma that may relate to motion on the Talas Fergana Fault. The coeval activation of a major right-lateral strike-slip system allowing indentation of the Pamir Salient into the Tarim basin, suggests far-field deformation from the India-Asia collision zone affected the Tian Shan and the Talas Fergana fault by early Miocene. (C) 2015 Elsevier B.V. All rights reserved. KW - Magnetostratigraphy KW - Cenozoic KW - Tian Shan KW - Pamir KW - Tarim Basin KW - Tectonics Y1 - 2015 U6 - https://doi.org/10.1016/j.tecto.2015.01.003 SN - 0040-1951 SN - 1879-3266 VL - 644 SP - 122 EP - 137 PB - Elsevier CY - Amsterdam ER - TY - JOUR A1 - Loprieno, Andrea A1 - Bousquet, Romain A1 - Bucher, Stefan A1 - Ceriani, Stefano A1 - Dalla Torre, Florian H. A1 - Fügenschuh, Bernhard A1 - Schmid, Stefan M. T1 - The valais units in Savoy (France) a key area for understanding the palaeogeography and the tectonic evolution of the Western Alps JF - International journal of earth sciences N2 - The Valais units in Savoy (Zone des BrSches de Tarentaise) have been re-mapped in great detail and are subject of combined stratigraphic, structural and petrological investigations summarized in this contribution. The sediments and rare relics of basement, together with Cretaceous age mafic and ultramafic rocks of the Valais palaeogeographical domain, represent the heavily deformed relics of the former distal European margin (External Valais units) and an ocean-continent transition (Internal Valais unit or Versoyen unit) that formed during rifting. This rifting led to the opening of the Valais ocean, a northern branch of the Alpine Tethys. Post-rift sediments referred to as "Valais trilogy" stratigraphically overlie both External and Internal Valais successions above an angular unconformity formed in Barremian to Aptian times, providing robust evidence for the timing of the opening of the Valais ocean. The Valais units in Savoy are part of a second and more external mid-Eocene high-pressure belt in the Alps that sutured the Brian double dagger onnais microcontinent to Europe. Top-N D1-deformation led to the formation of a nappe stack that emplaced the largely eclogite-facies Internal Valais unit (Versoyen) onto blueschist-facies External Valais units. The latter originally consisted of, from internal to external, the Petit St. Bernard unit, the Roc de l'Enfer unit, the MoA >> tiers unit and the Quermoz unit. Ongoing top-N D2-thrusting and folding substantially modified this nappe stack. Post 35 Ma D3 folding led to relatively minor modifications of the nappe stack within the Valais units but was associated with substantial top-WNW thrusting of the Valais units over the Dauphinois units along the Roselend thrust during W-directed indentation of the Adria block contributing to the formation of the arc of the Western Alps. KW - Alpine geology KW - Valais ocean KW - Palaeogeography KW - Structural geology KW - Tectonics KW - Metamorphism Y1 - 2011 U6 - https://doi.org/10.1007/s00531-010-0595-1 SN - 1437-3254 VL - 100 IS - 5 SP - 963 EP - 992 PB - Springer CY - New York ER - TY - JOUR A1 - Kober, Florian A1 - Zeilinger, Gerald A1 - Ivy-Ochs, Susan A1 - Dolati, A. A1 - Smit, J. A1 - Kubik, Peter W. T1 - Climatic and tectonic control on fluvial and alluvial fan sequence formation in the Central Makran Range, SE-Iran JF - Global and planetary change N2 - The geomorphic evolution of the Makran Range of SE-Iran and SW-Pakistan has been controlled by the prevailing SW-Asian monsoon and Mediterranean winter rainfall climate and the surface uplift processes resulting from the Arabia-Eurasia collision. The impact of climate on Quaternary fluvial and alluvial sequence formation and their regional correlation has been little investigated due to limited age control of these sequences. Using Be-10 cosmogenic nuclide exposure ages we established a Middle to Late Pleistocene terrace chronology. Our record tentatively indicates that terrace levels were abandoned towards the transition to or during warmer/pluvial periods (interglacials and/or interstadials) back to Marine Isotope Stage (MIS) 7, but abandoned ages show a large spread. It is hypothesized that pluvial phases correspond with times of enhanced SW-monsoons and a northward shift of the Intertropical Convergence Zone (ITCZ). Furthermore, orbital periodidties can be deduced on frequencies related to obliquity and precession cycles. Overall, caution has to be placed in sampling and interpreting alluvial deposits, which may have complex inheritance patterns and spatially and temporarily variable catchment erosion histories and terrace-channel dynamics. Beside the dominant climate control on terrace formation, elevated channel steepness indices around major thrusts and numerous knickpoints indicate an additionally tectonic influence on terrace formation. Local incision rates (mean similar to 0.6-0.8 min.a(-1)) are variable in space and time but are similar to uplift rates obtained from coastal terraces and thus suggest a regional surface uplift. (C) 2013 Elsevier B.V. All rights reserved. KW - Cosmogenic nuclides KW - Monsoon KW - Climate KW - Tectonics KW - Terraces KW - Makran Y1 - 2013 U6 - https://doi.org/10.1016/j.gloplacha.2013.09.003 SN - 0921-8181 SN - 1872-6364 VL - 111 SP - 133 EP - 149 PB - Elsevier CY - Amsterdam ER -