@phdthesis{QuirogaCarrasco2023, author = {Quiroga Carrasco, Rodrigo Adolfo}, title = {Cenozoic style of deformation and spatiotemporal variations of the tectonic stress field in the southern central Andes}, doi = {10.25932/publishup-61038}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-610387}, school = {Universit{\"a}t Potsdam}, pages = {228}, year = {2023}, abstract = {The central Andean plateau is the second largest orogenic plateau in the world and has formed in a non-collisional orogenic system. It extends from southern Peru (15°S) to northern Argentina and Chile (27°30'S) and reaches an average elevation of 4,000 m.a.s.l. South of 24°S, the Andean plateau is called Puna and it is characterized by a system of endorheic basins with thick sequences where clastic and evaporitic strata are preserved. Between 26° and 27°30'S, the Puna terminates in a structurally complex zone which coincides with the transition from a normal subduction zone to a flat subduction ("flat slab") zone, which extends to 33°S. This transition zone also coincides with important morphostructural provinces that, from west to east, correspond to i) the Cordillera Frontal, where the Maricunga Belt is located; ii) the Famatina system; and iv) the north-western, thick-skinned Sierras Pampeanas. Various structural, sedimentological, thermochronological and geochronological studies in this region have documented a complex history of deformation and uplift during successive Cenozoic deformation events. These processes caused the increase of crustal thickness, as well as episodes of diachronic uplift, which attained its present configuration during the late Miocene. Subsequently, the plateau experienced a change in deformation style from contraction to extension and transtension documented by ubiquitous normal faults, earthquakes, and magmatic rocks. However, at the southern edge of the Puna plateau and in the transition to the other morphostructural provinces, the variation of deformation processes and the changes in the tectonic stress field are not fully understood. This location is thus ideally located to evaluate how the tectonic stress field may have evolved and how it may have been affected by the presence/absence of an orogenic plateau, as well as by the existence of inherited structural anisotropies within the different tectonic provinces. This thesis investigates the relationship between shallow crustal deformation and the spatiotemporal evolution of the tectonic stress field in the southern sector of the Andean plateau, during pre-, syn- and post-uplift periods of this plateau. To carry out this research, multiple methodological approaches were chosen that include (U-Pb) radiometric dating; the analysis of mesoscopic faults to obtain stress tensors and the orientation of the principal stress axes; the determination of magnetic susceptibility anisotropy in sedimentary and volcanoclastic rocks to identify shortening directions or directions of sedimentary transport; kinematic modeling to infer deep crustal structures and deformation; and finally, a morphometric analysis to identify geomorphological indicators associated with Quaternary tectonism. Combining the obtained results with data from published studies, this study reveals a complex history of the tectonic stress field that has been characterized by changes in orientation and by vertical permutations of the principal stress axes during each deformation regime over the last ~24 Ma. The evolution of the tectonic stress field can be linked with three orogenic phases at this latitude of the Andean orogen: (1) a first phase with an E-W-oriented compression documented between Eocene and middle Miocene, which coincided with Andean crustal thickening, lateral growth, and topographic uplift; (2) a second phase characterized by a compressive transpressional stress regime, starting at ~11 Ma and ~5 Ma on the western and eastern edge of the Puna plateau, respectively, and a compressive stress regime in the Famatina system and the Sierras Pampeanas, which is interpreted to reflect a transition between Neogene orogenic construction and the maximum accumulation of deformation and topographic uplift of the Puna plateau; and (3) a third phase, when the tectonic regime caused a changeover to a tensional stress state that followed crustal thickening and the maximum uplift of the plateau between ~5-4 Ma; this is especially well expressed in the Puna, in its western border area with the Maricunga-Valle Ancho Belt, and along its eastern border in the transition with the Sierras Pampeanas. The results of the study thus document that the plateau rim experienced a shift from a compressional to a transtensional regime, which differs from the tensional state of stress of the Andean Plateau in the northern sectors for the same period. Similar stress changes have been documented during the construction of the Tibetan plateau, where a predominantly compressional stress regime changed to a transtensional regime, but which was superseded by a purely tensional regime, between 14 and 4 Ma.}, language = {es} } @phdthesis{Pilz2008, author = {Pilz, Peter}, title = {Ein neues magmatisch-tektonisches Modell zur Asthenosph{\"a}rendynamik im Bereich der zentralandinen Subduktionszone S{\"u}damerikas}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-20206}, school = {Universit{\"a}t Potsdam}, year = {2008}, abstract = {Im Rahmen der Dissertation wurden an W{\"a}ssern und freien Gasen aus Thermalquellen sowie an weniger als 5 Millionen Jahre alten basischen Vulkaniten des zentralandinen Puna-Hochplateaus (NE-Argentinien) umfangreiche element- und isotopengeochemische Untersuchungen durchgef{\"u}hrt und die Edelgasgehalte und -isotopensignaturen in diesen Medien bestimmt. Damit soll ein Beitrag zum besseren Verst{\"a}ndnis der j{\"u}ngeren Subduktionsgeschichte im Bereich der s{\"u}dlichen Zentralanden geleistet, die Wechselwirkungen zwischen ozeanischer Unter- und kontinentaler Oberplatte sichtbar gemacht und die Edelgassystematik verbessert werden. Wie die Ergebnisse der Untersuchungen an Gasen aus den Thermalquellen der Puna-Region zeigen, ist der Anteil an Mantel-Helium in den Thermalquellen dieser Region mit bis zu 67 \% wesentlich h{\"o}her als in der westlich gelegenen vulkanisch aktiven Westkordillere und den anderen angrenzenden Gebieten. In einigen Quellen konnten sogar Anteile an Mantel-Neon nachgewiesen werden, was aufgrund von {\"U}berlagerungen mit Neon atmosph{\"a}rischen und krustalen Ursprungs weltweit bisher nur vereinzelt gelungen ist. F{\"u}r kontinentale Bereiche mit großer Krustendicke ist ein solch starker Mantelgasfluss {\"a}ußerst ungew{\"o}hnlich und bedeutet, dass Mantelschmelzen bis in die Kruste aufgedrungen sind und tief reichende Wegsamkeiten existieren, so dass die Mantelgase aufsteigen k{\"o}nnen, ohne stark krustal beeinflusst zu werden. Dass im Bereich der Puna rezent Mantelmaterial in die Kruste aufsteigt, zu diesem Ergebnis kommen auch aktuelle seismologische Untersuchungen. Zudem wurden junge, vorwiegend monogenetische Basalte bis basaltische Andesite geochemisch auf ihre Haupt-, Neben- und Spurenbestandteile sowie ihre Gehalte an Seltenenerdenelementen hin untersucht. Auch wurden die Isotopenverh{\"a}ltnisse von Sr, Nd und Pb in den Gesteinen bestimmt und petrographisch-mineralogische Analysen der darin enthaltenen Olivine und Pyroxene durchgef{\"u}hrt. Wie die Resultate belegen, haben die Magmen bei ihrem Aufstieg durch die Erdkruste insbesondere Material aus der Oberkruste assimiliert und sind zudem durch Fluide aus der abtauchenden Platte beeinflusst worden. Damit konnte gezeigt werden, dass einfache geochemische Methoden allein nicht ausreichen, um die Mantelquelle der Magmen ermitteln oder Aussagen {\"u}ber die Asthenosph{\"a}rendynamik in der Region machen zu k{\"o}nnen. Im Gegensatz dazu zeigen die Messungen der Edelgasisotopenverh{\"a}ltnisse in den Fluideinschl{\"u}ssen der Olivine und Pyroxene, dass deren Edelgaszusammensetzung nicht durch Krustenkontamination beeinflusst wurde, weil die Magmen erst nach der Olivin- bzw. Pyroxen-Kristallisation Schmelzen aus der Oberkruste assimiliert haben. Dar{\"u}ber hinaus konnten durch die Edelgasisotopenmessungen die bisher h{\"o}chsten magmatischen He- und Ne-Isotopenverh{\"a}ltnisse von ganz S{\"u}damerika nachgewiesen werden. Aus der unterschiedlichen H{\"o}he der Messwerte ist zu schließen, dass die im Osten der Puna vorkommenden {\"a}lteren Laven aus einem nichtkonvektiven (lithosph{\"a}rischen) Mantel stammen, w{\"a}hrend die am vulkanischen Bogen und Westrand der Puna gelegenen j{\"u}ngeren Laven, ihren Ursprung in einer konvektiven (asthenosph{\"a}rischen) Mantelquelle haben. Zudem konnte gezeigt werden, dass der Mantelgasfluss in der Region in den letzten 5 Millionen Jahren stark zunahm und sich die Eruption von mantelst{\"a}mmigen basischen Laven in dieser Zeit kontinuierlich in westliche Richtung zum aktiven Vulkanbogen hin verlagerte. Im daraus abgeleiteten Modell beruht dieser Prozess (1) auf einer an die Kontinentalverschiebung gekoppelten W-Drift des Kontinents und (2) auf einem mit der Versteilung der Unterplatte verbundenen Vordringen des subkontinentalen asthenosph{\"a}rischen Mantels nach W, nach dem Ende der Subduktion des unterseeischen aseismischen Juan Fern{\´a}ndez-R{\"u}ckens in der Region. Zudem gibt es starke Argumente daf{\"u}r, dass die asthenosph{\"a}rischen Magmen aus einer fluidreichen Zone in 500 - 600 km Tiefe parallel zur subduzierten Platte aufsteigen und nicht, wie bisher angenommen, durch Schmelzbildung in Bereichen unter 200 km Tiefe, allein durch Entw{\"a}sserung der abtauchenden Platte erzeugt werden. Zu diesem Resultat f{\"u}hrt vor allem die Kombination der He-Isotopenverh{\"a}ltnisse mit Ergebnissen seismologischer Untersuchungen.}, language = {de} } @article{OrtizSaezAlvaradoetal.2022, author = {Ortiz, Gustavo and Saez, Mauro and Alvarado, Patricia and Rivas, Carolina and Garc{\´i}a, V{\´i}ctor Hugo and Alonso, Ricardo and Zullo, Fernando Morales}, title = {Seismotectonic characterization of the 1948 (M-W 6.9) Anta earthquake Santa Barbara System, central Andes broken foreland of northwestern Argentina}, series = {Journal of South American earth sciences}, volume = {116}, journal = {Journal of South American earth sciences}, publisher = {Elsevier}, address = {Oxford}, issn = {0895-9811}, doi = {10.1016/j.jsames.2022.103822}, pages = {15}, year = {2022}, abstract = {The region of the Andean back-arc of northwestern Argentina has been struck by several magnitude >= 6 crustal earthquakes since the first historically recorded event in 1692. One of these events corresponds to the Anta earthquake on 25 August 1948, with epicenter in the Santa Barbara System causing three deaths and severe damage in Salta and Jujuy provinces with maximum Modified Mercalli seismic intensities (MMI) of IX. We collected and digitized analog seismograms of this earthquake from worldwide seismic observatories in order to perform first-motion analysis and modeling of long-period teleseismic P-waveforms. Our results indicate a simple seismic source of M0 = 2.85 x 1019 N m consistent with a moment magnitude Mw = 6.9. We have also tested for the focal depth determining a shallow source at 8 km with a reverse focal mechanism solution with a minor dextral strike-slip component (strike 20 degrees, dip 30 degrees, rake 120 degrees) from the best fit of waveforms. Using magnitude size empirical relationships, the comparison of the obtained Mw 6.9 magnitude value and the ca. 10,000 km2 area of MMI >= IX from our seismic intensity map, which was obtained from newspaper and many historical reports, indicates a rupture length of 42 +/- 8 km for the Anta earthquake. We show our results in a 3D geological model around the epicentral area, which integrates modern seismicity, geological data, and information of a previously studied east-west cross section located a few kilometers south of the 1948 epicenter. The integration of all available information provides evidence of the re-activation of the Pie de la Sierra del Gallo fault during the 1948 Mw 6.9 shallow earthquake; this thrust fault bounds the Santa Barbara System along its western foothill.}, language = {en} } @article{NouryBernetSchildgenetal.2016, author = {Noury, M. and Bernet, M. and Schildgen, Taylor F. and Simon-Labric, T. and Philippon, M. and Sempere, T.}, title = {Crustal-scale block tilting during Andean trench-parallel extension: Structural and geo-thermochronological insights}, series = {Tectonics}, volume = {35}, journal = {Tectonics}, publisher = {American Geophysical Union}, address = {Washington}, issn = {0278-7407}, doi = {10.1002/2016TC004231}, pages = {2052 -- 2069}, year = {2016}, abstract = {Despite a long history of plate convergence at the western margin of the South American plate that has been ongoing since at least the Early Paleozoic, the southern Peruvian fore-arc displays little to no evidence of shortening. In the light of this observation, we assess the deformation history of the southern Peruvian fore-arc and its geodynamic implications. To accomplish this, we present a new structural and geo-thermochronological data set (zircon U-Pb, mica Ar-40/Ar-39, apatite and zircon fission-track and zircon (U-Th)/He analyses) for samples collected along a 400km long transect parallel to the trench. Our results show that the Mesoproterozoic gneissic basement was mainly at temperatures 350 degrees C since the Neoproterozoic and was later intruded by Jurassic volcanic arc plutons. Along the coast, a peculiar apatite fission-track age pattern, coupled with field observations and a synthesis of available geological maps, allows us to identify crustal-scale tilted blocks that span the coastal Peruvian fore-arc. These blocks, bounded by normal faults that are orthogonal to the trench, suggest post-60Ma trench-parallel extension that potentially accommodated oroclinal bending in this region. Block tilting is consistent with the observed and previously described switch in the location of sedimentary sources in the fore-arc basin. Our data set allows us to estimate the cumulative slip on these faults to be less than 2km and questions the large amount of trench-parallel extension suggested to have accommodated this bending.}, language = {en} } @article{LiuSobolevBabeykoetal.2022, author = {Liu, Sibiao and Sobolev, Stephan and Babeyko, Andrey and Pons, Micha{\"e}l}, title = {Controls of the foreland deformation pattern in the orogen-foreland shortening system}, series = {Tectonics}, volume = {41}, journal = {Tectonics}, number = {2}, publisher = {American Geophysical Union}, address = {Washington}, issn = {0278-7407}, doi = {10.1029/2021TC007121}, pages = {18}, year = {2022}, abstract = {Controls on the deformation pattern (shortening mode and tectonic style) of orogenic forelands during lithospheric shortening remain poorly understood. Here, we use high-resolution 2D thermomechanical models to demonstrate that orogenic crustal thickness and foreland lithospheric thickness significantly control the shortening mode in the foreland. Pure-shear shortening occurs when the orogenic crust is not thicker than the foreland crust or thick, but the foreland lithosphere is thin (<70-80 km, as in the Puna foreland case). Conversely, simple-shear shortening, characterized by foreland underthrusting beneath the orogen, arises when the orogenic crust is much thicker. This thickened crust results in high gravitational potential energy in the orogen, which triggers the migration of deformation to the foreland under further shortening. Our models present fully thick-skinned, fully thin-skinned, and intermediate tectonic styles in the foreland. The first tectonics forms in a pure-shear shortening mode whereas the others require a simple-shear mode and the presence of thick (>similar to 4 km) sediments that are mechanically weak (friction coefficient 95th percentile) along an E-W traverse across the southern Central Andes using rain-gauge and high-resolution gridded datasets (CPC-uni and TRMM 3B42 V7). We generated different climate indices and made three key observations: (1) an increase of the annual rainfall has occurred at the transition between low (< 0.5 km) and intermediate (0.5-3 km) elevations between 1950 and 2014. Also, rainfall increases during the wet season and, to a lesser degree, decreases during the dry season. Increasing trends in annual total amounts characterize the period 1979-2014 in the arid, high-elevation southern Andean Plateau, whereas trend reversals with decreasing annual total amounts were found at low elevations. (2) For all analyzed periods, we observed small or no changes in the median values of the rainfall-frequency distribution, but significant trends with intensification or attenuation in the 95th percentile. (3) In the southern Andean Plateau, extreme rainfall events exhibit trends towards increasing magnitude and, to a lesser degree, frequency during the wet season, at least since 1979. Our analysis revealed that low (< 0.5 km), intermediate (0.5-3 km), and high-elevation (> 3 km) areas respond differently to changing climate conditions, and the transition zone between low and intermediate elevations is characterized by the most significant changes.}, language = {en} } @article{CastinoBookhagenStrecker2017, author = {Castino, Fabiana and Bookhagen, Bodo and Strecker, Manfred}, title = {Oscillations and trends of river discharge in the southern Central Andes and linkages with climate variability}, series = {Journal of hydrology}, volume = {555}, journal = {Journal of hydrology}, publisher = {Elsevier}, address = {Amsterdam}, issn = {0022-1694}, doi = {10.1016/j.jhydrol.2017.10.001}, pages = {108 -- 124}, year = {2017}, abstract = {This study analyzes the discharge variability of small to medium drainage basins (10(2)-10(4) km(2)) in the southern Central Andes of NW Argentina. The Hilbert-Huang Transform (HHT) was applied to evaluate non-stationary oscillatory modes of variability and trends, based on four time series of monthly normalized discharge anomaly between 1940 and 2015. Statistically significant trends reveal increasing discharge during the past decades and document an intensification of the hydrological cycle during this period. An Ensemble Empirical Mode Decomposition (EEMD) analysis revealed that discharge variability in this region can be best described by five quasi-periodic statistically significant oscillatory modes, with mean periods varying from 1 to 20 y. Moreover, we show that discharge variability is most likely linked to the phases of the Pacific Decadal Oscillation (PDO) at multi-decadal timescales (similar to 20 y) and, to a lesser degree, to the Tropical South Atlantic SST anomaly (TSA) variability at shorter timescales (similar to 2-5 y). Previous studies highlighted a rapid increase in discharge in the southern Central Andes during the 1970s, inferred to have been associated with the global 1976-77 climate shift. Our results suggest that the rapid discharge increase in the NW Argentine Andes coincides with the periodic enhancement of discharge, which is mainly linked to a negative to positive transition of the PDO phase and TSA variability associated with a long-term increasing trend. We therefore suggest that variations in discharge in this region are largely driven by both natural variability and the effects of global climate change. We furthermore posit that the links between atmospheric and hydrologic processes result from a combination of forcings that operate on different spatiotemporal scales. (C) 2017 Elsevier B.V. All rights reserved.}, language = {en} }