TY - GEN A1 - Braun, Jean T1 - Response to comment by Japsen et al. on "A review of numerical modeling studies of passive margin escarpments leading to a new analytical expression for the rate of escarpment migration velocity" T2 - Gondwana research : international geoscience journal ; official journal of the International Association for Gondwana Research Y1 - 2020 U6 - https://doi.org/10.1016/j.gr.2018.10.003 SN - 1342-937X SN - 1878-0571 VL - 65 SP - 174 EP - 176 PB - Elsevier CY - Amsterdam ER - TY - THES A1 - Borghini, Alessia T1 - Melt inclusions in mafic rocks as witnesses of metasomatism in the Bohemian Massif N2 - Orogenic peridotites represent portions of upper subcontinental mantle now incorporated in mountain belts. They often contain layers, lenses and irregular bodies of pyroxenite and eclogite. The origin of this heterogeneity and the nature of these layers is still debated but it is likely to involve processes such as transient melts coming from the crust or the mantle and segregating in magma conduits, crust-mantle interaction, upwelling of the asthenosphere and metasomatism. All these processes occur in the lithospheric mantle and are often related with the subduction of crustal rocks to mantle depths. In fact, during subduction, fluids and melts are released from the slab and can interact with the overlying mantle, making the study of deep melts in this environment crucial to understand mantle heterogeneity and crust-mantle interaction. The aim of this thesis is precisely to better constrain how such processes take place studying directly the melt trapped as primary inclusions in pyroxenites and eclogites. The Bohemian Massif, crystalline core of the Variscan belt, is targeted for these purposes because it contains orogenic peridotites with layers of pyroxenite and eclogite and other mafic rocks enclosed in felsic high pressure and ultra-high pressure crustal rocks. Within this Massif mafic rocks from two areas have been selected: the garnet clinopyroxenite in orogenic peridotite of the Granulitgebirge and the ultra-high pressure eclogite in the diamond-bearing gneisses of the Erzgebirge. In both areas primary melt inclusions were recognized in the garnet, ranging in size between 2-25 µm and with different degrees of crystallization, from glassy to polycrystalline. They have been investigated with Micro Raman spectroscopy and EDS mapping and the mineral assemblage is kumdykolite, phlogopite, quartz, kokchetavite, phase with a main Raman peak at 430 cm-1, phase with a main Raman peak at 412 cm-1, white mica and calcite with some variability in relative abundance depending on the case study. In the Granulitgebirge osumilite and pyroxene are also present, whereas calcite is one of the main phases in the Erzgebirge. The presence of glass and the mineral assemblage in the nanogranitoids suggest that they were former droplets of melt trapped in the garnet while it was growing. Glassy inclusions and re-homogenized nanogranitoids show a silicate melt that is granitic, hydrous, high in alkalis and weakly peraluminous. The melt is also enriched in both case studies in Cs, Pb, Rb, U, Th, Li and B suggesting the involvement of crustal component, i.e. white mica (main carrier of Cs, Pb, Rb, Li and B), and a fluid (Cs, Th and U) in the melt producing reaction. The whole rock in both cases mainly consists of garnet and clinopyroxene with, in Erzgebirge samples, the additional presence of quartz both in the matrix and as a polycrystalline inclusion in the garnet. The latter is interpreted as a quartz pseudomorph after coesite and occurs in the same microstructural position as the melt inclusions. Both rock types show a crustal and subduction zone signature with garnet and clinopyroxene in equilibrium. Melt was likely present during the metamorphic peak of the rock, as it occurs in garnet. Our data suggest that the processes most likely responsible for the formation of the investigated rocks in both areas is a metasomatic reaction between a melt produced in the crust and mafic layers formerly located in the mantle wedge for the Granulitgebirge and in the subducted continental crust itself in the Erzgebirge. Thus metasomatism in the first case took place in the mantle overlying the slab, whereas in the second case metasomatism took place in the continental crust that already contained, before subduction, mafic layers. Moreover, the presence of former coesite in the same microstructural position of the melt inclusions in the Erzgebirge garnets suggest that metasomatism took place at ultra-high pressure conditions. Summarizing, in this thesis we provide new insights into the geodynamic evolution of the Bohemian Massif based on the study of melt inclusions in garnet in two different mafic rock types, combining the direct microstructural and geochemical investigation of the inclusions with the whole-rock and mineral geochemistry. We report for the first time data, directly extracted from natural rocks, on the metasomatic melt responsible for the metasomatism of several areas of the Bohemian Massif. Besides the two locations here investigated, belonging to the Saxothuringian Zone, a signature similar to the investigated melt is clearly visible in pyroxenite and peridotite of the T-7 borehole (again Saxothuringian Zone) and the durbachite suite located in the Moldanubian Zone. N2 - Die Präsenz orogener Peridotite - metamorphosierte Bestanteile des Mantels -, die in Gebirgen auftreten, belegt, dass der Erdmantel an Kontinent-Kontinent-Kollisionen beteiligt sein kann. Solche orogenen Peridotite sind häufig heterogen, da sie Pyroxenit- und Eklogitlagen und Linsen enthalten, d.h. Hochdruckgesteine, die aus Granat und Klinopyroxen bestehen. Die meisten Prozesse, die für diese Heterogenität verantwortlich sind, involvieren Schmelzen, die durch den Mantel migrieren und dabei zu dessen Metasomatose oder zu der Anreicherung von Granat und Klinopyroxen in Adern und Kanälen führen. Ein weiterer Prozess kann auch das Recyceln subduzierter ozeanischer Kruste im Erdmantel sein. Im Allgemeinen finden all diese Prozesse während der Subduktion der Kruste in Manteltiefe statt. Unter diesen Bedingungen stehen die Krustengesteine im direkten Kontakt mit den Mantelgesteinen und die dabei freigesetzten Fluide oder Schmelzen können mit den Peridotiten wechselwirken. Letztere können anschließend von den Krustengesteinen aufgenommen und zur Erdoberfläche exhumiert werden, wo sie untersucht werden können. Diese Arbeit fokussiert sich vor allem auf die Untersuchung der Pyroxenit- und Eklogitbildung sowie auf die Wechselwirkung zwischen Schmelze und Gestein während der Subduktion der Kontinentalkruste in Manteltiefe. Dafür ist das Böhmische Massiv die ideale geologische Umgebung, da es erhebliche Mengen an Pyroxeniten und Eklogiten enthält, die sich in einigen Fällen in orogenen Peridotiten befinden, und die alle in einer ehemals tief subduziertern kontinentalern Kruste eingegliedert wurden. Um die Zielstellung zu erreichen, wurde die Schmelze mit einem neuartigen Ansatz untersucht, wobei diese hier direkt in primären Schmelzeinschlüssen, die im Granat eingeschlossenen sind, untersucht wird. Es wurden zwei Gebiete mit Pyroxeniten und Eklogiten, die Schmelzeinschlüsse enthalten, ausgewählt, ein Pyroxenit aus dem Granulitgebirge und ein Ultrahochdruck-Eklogit aus dem Erzgebirge (Sachsen, Deutschland). Die Einschlüsse bestehen aus einer granitischen, wasserhaltigen Schmelze krustaler Herkunft. Das Auftreten der im Granat unregelmäßig verteilten Einschlüsse bestätigt das Vorhandensein von Schmelze während der Peakmetamorphose. Da die Schmelzen in beiden Fällen ähnlich sind, schlussfolgern wir daraus, dass beide Gesteinsarten durch metasomatische Prozesse infolge der Wechselwirkung von silikatreicher Schmelze und mafischen Lagen gebildete wurden. Im Granulitgebirge ging die Schmelze eine Wechselwirkung mit mafischen Lagen im Mantel ein und erst später wurde der Wirtsperidotit einschließlich der neugebildeten Pyroxenit- und Eklogitlagen in die subduzierte Kruste eingebaut. Im Fall der Pyroxenite und Eklogite des Erzgebirges fand die Metasomatose stattdessen in der kontinentalen Kruste statt. Hier ging die Schmelze eine Wechselwirkung mit mafischen Lagen ein, die sich bereits vor der Subduktion in der Kruste befunden hatten. Im letzteren Fall belegt der Hinweis auf ehemaligen Coesit , d. h. auf ein Mineral, das Tiefen >95 km anzeigt, welches anwesend war während der Metasomatose, dass die Prozesse in größeren Tiefen stattfanden als im Granulitgebirge. T2 - Schmelzeinschlüsse in mafischen Gesteinen als Zeugen von Metasomatose im Böhmischen Massiv KW - Petrology KW - Petrologie KW - Metamorphism KW - Melt inclusions KW - Metasomatism KW - Metamorphose KW - Schmelzeinschlüsse KW - Metasomatose Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-473639 ER - TY - THES A1 - Biedermann, Nicole T1 - Carbonate-silicate reactions at conditions of the Earth’s mantle and the role of carbonates as possible trace-element carriers N2 - Carbonates play a key role in the chemistry and dynamics of our planet. They are directly connected to the CO2 budget of our atmosphere and have a great impact on the deep carbon cycle. Moreover, recent studies have shown that carbonates are stable along the geothermal gradient down to Earth's lower mantle conditions, changing their crystal structure and related properties. Subducted carbonates may also react with silicates to form new phases. These reactions will redistribute elements, such as calcium (Ca), magnesium (Mg), iron (Fe) and carbon in the form of carbon dioxide (CO2), but also trace elements, that are carried by the carbonates. The trace elements of most interest are strontium (Sr) and rare earth elements (REE) which have been found to be important constituents in the composition of the primitive lower mantle and in mineral inclusions found in super-deep diamonds. However, the stability of carbonates in presence of mantle silicates at relevant temperatures is far from being well understood. Related to this, very little is known about distribution processes of trace elements between carbonates and mantle silicates. To shed light on these processes, we studied reactions between Sr- and REE-containing CaCO3 and Mg/Fe-bearing silicates of the system (Mg,Fe)2SiO4 - (Mg,Fe)SiO3 at high pressure and high temperature using synchrotron radiation based μ-X-ray diffraction (μ-XRD) and μ-X-ray fluorescence (μ-XRF) with μm-resolution in a laser-heated diamond anvil cell. X-ray diffraction is used to derive the structural changes of the phase reactions whereas X-ray fluorescence gives information on the chemical changes in the sample. In-situ experiments at high pressure and high temperature were performed at beamline P02.2 at PETRA III (Hamburg, Germany) and at beamline ID27 at ESRF (Grenoble, France). In addition to μ-XRD and μ-XRF, ex-situ measurements were made on the recovered sample material using transmission electron microscopy (TEM) and provided further insights into the reaction kinetics of carbonate-silicate reactions. Our investigations show that CaCO3 is unstable in presence of mantle silicates above 1700 K and a reaction takes place in which magnesite plus CaSiO3-perovskite are formed. In addition, we observed that a high content of iron in the carbonate-silicate system favours dolomite formation during the reaction. The subduction of natural carbonates with significant amounts of Sr leads to a comprehensive investigation of the stability not only of CaCO3 phases in contact with mantle silicates but also of SrCO3 (and of Sr-bearing CaCO3). We found that SrCO3 reacts with (Mg,Fe)SiO3-perovskite to form magnesite and gained evidence for the formation of SrSiO3-perovskite. To complement our study on the stability of SrCO3 at conditions of the Earth's lower mantle, we performed powder X-ray diffraction and single crystal X-ray diffraction experiments at ambient temperature and up to 49 GPa. We observed a transformation from SrCO3-I into a new high-pressure phase SrCO3-II at around 26 GPa with Pmmn crystal structure and a bulk modulus of 103(10) GPa. This information is essential to fully understand the phase behaviour and stability of carbonates in the Earth's lower mantle and to elucidate the possibility of introducing Sr into mantle silicates by carbonate-silicate reactions. Simultaneous recording of μ-XRD and μ-XRF in the μm-range over the heated areas provides spatial information not only about phase reactions but also on the elemental redistribution during the reactions. A comparison of the spatial intensity distribution of the XRF signal before and after heating indicates a change in the elemental distribution of Sr and an increase in Sr-concentration was found around the newly formed SrSiO3-perovskite. With the help of additional TEM analyses on the quenched sample material the elemental redistribution was studied at a sub-micrometer scale. Contrary to expectations from combined μ-XRD and μ-XRF measurements, we found that La and Eu were not incorporated into the silicate phases, instead they tend to form either isolated oxide phases (e.g. Eu2O3, La2O3) or hydroxyl-bastnäsite (La(CO3)(OH)). In addition, we observed the transformation from (Mg,Fe)SiO3-perovskite to low-pressure clinoenstatite during pressure release. The monoclinic structure (P21/c) of this phase allows the incorporation of Ca as shown by additional EDX analyses and, to a minor extent, Sr too. Based on our experiments, we can conclude that a detection of the trace elements in-situ at high pressure and high temperature remains challenging. However, our first findings imply that silicates may incorporate the trace elements provided by the carbonates and indicate that carbonates may have a major effect on the trace element contents of mantle phases. N2 - Karbonate spielen eine wesentliche Rolle in der Chemie und Dynamik unseres Planeten. Sie stehen im direkten Zusammenhang mit dem CO2-Haushalt unserer Atmosphäre und dem tiefen, erdinneren Kohlenstoff-Kreislauf. Darüber hinaus haben jüngste Studien gezeigt, dass subduzierte Karbonate entlang des geothermischen Gradienten bis hinunter zu unteren Erdmantelbedingungen stabil sind, wobei sich ihre Kristallstruktur und die damit verbundenen Eigenschaften ändern. Ebenso können subduzierte Karbonate mit Mantelsilikaten reagieren. Diese Reaktionen führen zu einer Umverteilung von Elementen, welche von den subduzierten Karbonaten hinunter in die Tiefen der Erde transportiert werden. Die Elemente, um die es sich hauptsächlich handelt, sind dabei Calcium (Ca), Magnesium (Mg), Eisen (Fe) und Kohlenstoff (C). Aber auch Spurenelemente, wie beispielsweise Strontium (Sr) und Seltene Erdelemente (REE), können über Karbonate in den unteren Erdmantelbereich gelangen. Die Stabilität der Karbonate in Gegenwart von Mantelsilikaten bei relevanten Erdmantelbedingungen ist jedoch bei Weitem nicht bekannt. Ebenso ist nur sehr wenig über die Verteilungsprozesse von Spurenelementen zwischen Karbonaten und Mantelsilikaten bekannt. Um diese Prozesse zu beleuchten, wurden Reaktionen zwischen Sr- und REE-haltigem CaCO3 und Mg/Fe-haltigen Silikaten aus dem System (Mg,Fe)2SiO4 - (Mg,Fe)SiO3 unter hohem Druck und hoher Temperatur mit μm-aufgelöster Röntgenbeugung (μ-XRD) und Röntgenfluoreszenz (μ-XRF) in einer lasergeheizten Diamantstempelzelle durchgeführt. Dabei wird Röntgenbeugung verwendet, um die strukturellen Änderungen der Phasenreaktionen abzuleiten, während Röntgenfluoreszenz Informationen über die chemischen Änderungen in der Probe liefert. Unsere Untersuchungen zeigen, dass sowohl SrCO3 als auch CaCO3 in Gegenwart von Mantelsilikaten bei über 1700 K instabil sind und eine Reaktion stattfindet, bei der Magnesit und CaSiO3-Perowskit bzw. SrSiO3-Perowskit gebildet werden. Ein Vergleich der räumlichen Intensitätsverteilungen von XRF Signalen vor und nach dem Heizen zeigt eine Änderung in der Elementverteilung von Sr und eine Zunahme der Sr-Konzentration um den neugebildeten SrSiO3-Perowskit. Zusätzliche Aufnahmen am zurückgewonnenen, abgeschreckten Probenmaterial mittels Transmissionselektronenmikroskopie (TEM) lieferten weitere Erkenntnisse zur Reaktionskinetik. Entgegen den Erwartungen eines Einbaus der Seltenen Erdelemente in die neugebildeten Mantelsilikate, haben wir aus kombinierten μ-XRD-, μ-XRF- und TEM-Messungen festgestellt, dass La und Eu entweder isolierte Oxidphasen (Eu2O3, La2O3) oder Hydroxyl-Bastnäsit (La(CO3)(OH)) bilden. Zusätzlich war zu beobachten, dass (Mg,Fe)SiO3-Perowskit sich während der Druckentlastung in Clinoenstatit umgewandelt hat. Die monokline Struktur dieser Phase ermöglicht den Einbau von Ca und, im geringerem Maße, Sr, wie durch zusätzliche EDX-Analysen gezeigt wurde. Ergänzend zu unserer Studie führten wir Pulver-Röntgenbeugung in Kombination mit Einkristall-Röntgenbeugung bei Umgebungstemperatur und bis zu 49 GPa am Endglied Strontianit (SrCO3) durch. Wir beobachteten eine Umwandlung von SrCO3-I in eine neue Hochdruckphase SrCO3-II bei etwa 26 GPa mit Pmmn-Kristallstruktur und einem Kompressionsmodul von 103(10) GPa. Solche Informationen sind sehr wichtig, da sie Aufschlüsse sowohl über das Phasenverhalten als auch über die Stabilität von Karbonaten in Gegenwart von Mantelsilikaten geben und helfen, sie vollständig zu verstehen. Basierend auf den Erkenntnissen aus unseren Experimenten können wir schließen, dass ein Nachweis von Spurenelementen in-situ unter hohem Druck und hoher Temperatur eine Herausforderung bleibt. Unsere Ergebnisse deuten jedoch darauf hin, dass Silikate die Spurenelemente, welche von den Karbonaten transportiert werden, aufnehmen können und demzufolge Karbonate einen wesentlichen Einfluss auf den Spurenelementgehalt von Mantelphasen haben. T2 - Karbonat-Silikat-Reaktionen bei Erdmantelbedingungen und die Rolle der Karbonate als mögliche Spurenelementträger KW - laser-heated Diamond Anvil Cell KW - Carbonate-Silicate reactions KW - Earth's mantle KW - Karbonat-Silikat-Reaktionen KW - Erdmantel KW - laser-geheizte Diamantstempelzelle Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-482772 ER - TY - JOUR A1 - Bentz, Stephan A1 - Kwiatek, Grzegorz A1 - Martinez-Garzon, Patricia A1 - Bohnhoff, Marco A1 - Dresen, Georg T1 - Seismic moment evolution during hydraulic stimulations JF - Geophysical research letters N2 - Analysis of past and present stimulation projects reveals that the temporal evolution and growth of maximum observed moment magnitudes may be linked directly to the injected fluid volume and hydraulic energy. Overall evolution of seismic moment seems independent of the tectonic stress regime and is most likely governed by reservoir specific parameters, such as the preexisting structural inventory. Data suggest that magnitudes can grow either in a stable way, indicating the constant propagation of self-arrested ruptures, or unbound, for which the maximum magnitude is only limited by the size of tectonic faults and fault connectivity. Transition between the two states may occur at any time during injection or not at all. Monitoring and traffic light systems used during stimulations need to account for the possibility of unstable rupture propagation from the very beginning of injection by observing the entire seismicity evolution in near-real time and at high resolution for an immediate reaction in injection strategy. Plain Language Summary Predicting and controlling the size of earthquakes caused by fluid injection is currently the major concern of many projects associated with geothermal energy production. Here, we analyze the magnitude and seismic moment evolution with injection parameters for prominent geothermal and scientific projects to date. Evolution of seismicity seems to be largely independent of the tectonic stress background and seemingly depends on reservoir specific characteristics. We find that the maximum observed magnitudes relate linearly to the injected volume or hydraulic energy. A linear relation suggests stable growth of induced ruptures, as predicted by current models, or rupture growth may no longer depend on the stimulated volume but on tectonics. A system may change between the two states during the course of fluid injection. Close-by and high-resolution monitoring of seismic and hydraulic parameters in near-real time may help identify these fundamental changes in ample time to change injection strategy and manage maximum magnitudes. Y1 - 2020 U6 - https://doi.org/10.1029/2019GL086185 SN - 0094-8276 SN - 1944-8007 VL - 47 IS - 5 PB - American Geophysical Union CY - Washington ER - TY - GEN A1 - Ben Dor, Yoav A1 - Neugebauer, Ina A1 - Enzel, Yehouda A1 - Schwab, Markus J. A1 - Tjallingii, Rik A1 - Erel, Yigal A1 - Brauer, Achim T1 - Reply to comment on: Ben Dor, Yoav et al. : Varves of the Dead Sea sedimentary record. - In: Quaternary science reviews : the international multidisciplinary research and review journal. - 215 (2019), S. 173 - 184. - (ISSN: 0277-3791). - https://doi.org/10.1016/j.quascirev.2019.04.011 T2 - Quaternary science reviews : the international multidisciplinary research and review journal N2 - In the comment on "Varves of the Dead Sea sedimentary record." Quaternary Science Reviews 215 (Ben Dor et al., 2019): 173-184. by R. Bookman, two recently published papers are suggested to prove that the interpretation of the laminated sedimentary sequence of the Dead Sea, deposited mostly during MIS2 and Holocene pluvials, as annual deposits (i.e., varves) is wrong. In the following response, we delineate several lines of evidence which coalesce to demonstrate that based on the vast majority of evidence, including some of the evidence provided in the comment itself, the interpretation of these sediments as varves is the more likely scientific conclusion. We further discuss the evidence brought up in the comment and its irrelevance and lack of robustness for addressing the question under discussion. Y1 - 2020 U6 - https://doi.org/10.1016/j.quascirev.2019.106063 SN - 0277-3791 VL - 231 PB - Elsevier CY - Amsterdam [u.a.] ER - TY - THES A1 - Barrionuevo, Matías T1 - The role of the upper plate in the Andean tectonic evolution (33-36°S): insights from structural geology and numerical modeling T1 - El rol de la placa superior en la evolución tectónica andina (33-36°S): aportes desde la geología estructural y el modelado numérico T1 - Die Rolle der oberen Platte in der tektonischen Entwicklung der Anden (33-36°S): Erkenntnisse aus der Strukturgeologie und der numerischen Modellierung N2 - Los Andes Centrales del Sur (33-36°S) son un gran laboratorio para el estudio de los procesos de deformación orogénica, donde las condiciones de borde, como la geometría de la placa subductada, imponen un importante control sobre la deformación andina. Por otro lado, la Placa Sudamericana presenta una serie de heterogeneidades que también imparten un control sobre el modo de deformación. El objetivo de esta tesis es probar el control de este último factor sobre la construcción del sistema orogénico andino. A partir de la integración de la información superficial y de subsuelo en el área sur (34°-36°S), se estudió la evolución de la deformación andina sobre el segmento de subducción normal. Se desarrolló un modelo estructural que evalúa el estado de esfuerzos desde el Mioceno hasta la actualidad, el rol de estructuras previas y su influencia en la migración de fluidos. Con estos datos y publicaciones previas de la zona norte del área de estudio (33°-34ºS), se realizó un modelado numérico geodinámico para probar la hipótesis del papel de las heterogeneidades de la placa superior en la evolución andina. Se utilizaron dos códigos (LAPEX-2D y ASPECT) basados en elementos finitos/diferencias finitas, que simulan el comportamiento de materiales con reologías elastoviscoplásticas bajo deformación. Los resultados del modelado sugieren que la deformación contraccional de la placa superior está significativamente controlada por la resistencia de la litósfera, que está definida por la composición de la corteza superior e inferior y por la proporción del manto litosférico, que a su vez está definida por eventos tectónicos previos. Estos eventos previos también definieron la composición de la corteza y su geometría, que es otro factor que controla la localización de la deformación. Con una composición de corteza inferior más félsica, la deformación sigue un modo de cizalla pura mientras que las composiciones más máficas provocan un modo de deformación tipo cizalla simple. Por otro lado, observamos que el espesor inicial de la litósfera controla la localización de la deformación, donde zonas con litósfera más fina es propensa a concentrar la deformación. Un límite litósfera-astenósfera asimétrico, como resultado del flujo de la cuña mantélica tiende a generar despegues vergentes al E. N2 - The Southern Central Andes (33°-36°S) are an excellent natural laboratory to study orogenic deformation processes, where boundary conditions, such as the geometry of the subducted plate, impose an important control on the evolution of the orogen. On the other hand, the South American plate presents a series of heterogeneities that additionally impart control on the mode of deformation. This thesis aims to test the control of this last factor over the construction of the Cenozoic Andean orogenic system. From the integration of surface and subsurface information in the southern area (34-36°S), the evolution of Andean deformation over the steeply dipping subduction segment was studied. A structural model was developed evaluating the stress state from the Miocene to the present-day and its influence in the migration of magmatic fluids and hydrocarbons. Based on these data, together with the data generated by other researchers in the northern zone of the study area (33-34°S), geodynamic numerical modeling was performed to test the hypothesis of the decisive role of upper-plate heterogeneities in the Andean evolution. Geodynamic codes (LAPEX-2D and ASPECT) which simulate the behavior of materials with elasto-visco-plastic rheologies under deformation, were used. The model results suggest that upper-plate contractional deformation is significantly controlled by the strength of the lithosphere, which is defined by the composition of the upper and lower crust, and by the proportion of lithospheric mantle, which in turn is determined by previous tectonic events. In addition, the previous regional tectono-magmatic events also defined the composition of the crust and its geometry, which is another factor that controls the localization of deformation. Accordingly, with more felsic lower crustal composition, the deformation follows a pure-shear mode, while more mafic compositions induce a simple-shear deformation mode. On the other hand, it was observed that initial lithospheric thickness may fundamentally control the location of deformation, with zones characterized by thin lithosphere are prone to concentrate it. Finally, it was found that an asymmetric lithosphere-astenosphere boundary resulting from corner flow in the mantle wedge of the eastward-directed subduction zone tends to generate east-vergent detachments. N2 - Die südlichen Zentralanden (33°-36°S) sind eine ausgezeichnete, natürliche Forschungsumgebung zur Untersuchung gebirgsbildender Deformationsprozesse, in der Randbedingungen, wie die Geometrie der subduzierten Platte, einen starken Einfluss auf die Evolution des Gebirges besitzen. Anderseits sind die Deformationsmechanismen geprägt von der Heterogenität der Südamerikanischen Platte. In dieser Arbeit wird die Bedeutung dieses Mechanismus für die Herausbildung der Anden während des Känozoikums untersucht. Im südlichen Teil (34-36°S), in dem die subduzierte Platte in einem steileren Winkel in den Erdmantel absinkt, wird die Entwicklung der Andendeformation mithilfe von oberflächlich aufgezeichneten und in tiefere Erdschichten reichenden Daten untersucht. Das darauf aufbauende Strukturmodell ermöglicht die Abschätzung der tektonischen Spannungen vom Miozän bis in die Neuzeit und den Einfluss der Bewegungen von magmatischen Fluiden, sowie Kohlenwasserstoffen. Auf Grundlage dieser Daten und solcher, die von Wissenschaftlern im nördlichen Bereich des Untersuchungsgebietes (33-34°S) erfasst wurden, wurde eine geodynamische, numerische Modellierung durchgeführt, um die Hypothese des Einflusses der Heterogenität der oberen Platten auf die Gebirgsbildung der Anden zu überprüfen. Die genutzte geodynamische Softwares (LAPEX-2D und ASPECT) simulieren das Verhalten von elasto-viskoplastischen Materialien, wenn diese unter Spannung stehen. Die Modellierungsergebnisse zeigen, dass die Kontraktionsprozesse hauptsächlich durch die Stärke der Lithosphäre beeinflusst werden. Diese Kenngröße wird aus der Zusammensetzung von Ober- und Unterkruste und dem Anteil des lithosphärischen Mantels, der durch vorhergehende tektonische Vorgänge überprägt ist, bestimmt. Diese räumlich begrenzten tektono-magmatischen Events definieren ebenfalls die Zusammensetzung und die Geometrie der Erdkruste, welche einen großen Einfluss auf das räumliche Auftreten von Deformationsprozessen hat. Eine eher felsische Unterkruste führt vorrangig zu pure-shear, während eine eher mafisch zusammengesetzte Unterkruste primär zu einem Deformationsmechanismus führt, der simple-shear genannt wird. Weiterhing wurde beobachtet, dass die Dicke der Lithosphäre vor der Deformation einen fundamentalen Einfluss auf die räumliche Eingrenzung von Deformation hat, wobei Regionen mit einer dünnen Lithosphärenschicht verstärkt Deformation aufweisen. Eine asymmetrische Grenzschicht zwischen Lithosphäre und Asthenosphäre ist das Resultat von Fließprozessen im Erdmantel, im Keil zwischen der obenliegenden Platte und der sich ostwärts absinkenden Subduktionszone, und verstärkt die Herausbildung von nach Osten gerichteten Abscherungen in der Erdkruste. KW - structural geology KW - tectonics KW - subduction KW - geodynamic modeling KW - geodynamische Modellierung KW - Strukturgeologie KW - Subduktion KW - Tektonik Y1 - 2021 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-515909 ER - TY - JOUR A1 - Baroni, Gabriele A1 - Francke, Till T1 - An effective strategy for combining variance- and distribution-based global sensitivity analysis JF - Environmental modelling & software with environment data news N2 - We present a new strategy for performing global sensitivity analysis capable to estimate main and interaction effects from a generic sampling design. The new strategy is based on a meaningful combination of varianceand distribution-based approaches. The strategy is tested on four analytic functions and on a hydrological model. Results show that the analysis is consistent with the state-of-the-art Saltelli/Jansen formula but to better quantify the interaction effect between the input factors when the output distribution is skewed. Moreover, the estimation of the sensitivity indices is much more robust requiring a smaller number of simulations runs. Specific settings and alternative methods that can be integrated in the new strategy are also discussed. Overall, the strategy is considered as a new simple and effective tool for performing global sensitivity analysis that can be easily integrated in any environmental modelling framework. KW - global sensitivity analysis KW - variance KW - distribution KW - generic sampling KW - design Y1 - 2020 U6 - https://doi.org/10.1016/j.envsoft.2020.104851 SN - 1364-8152 SN - 1873-6726 VL - 134 PB - Elsevier CY - Oxford ER - TY - JOUR A1 - Barbolini, Natasha A1 - Woutersen, Amber A1 - Dupont-Nivet, Guillaume A1 - Silvestro, Daniele A1 - Tardif-Becquet, Delphine A1 - Coster, Pauline M. C. A1 - Meijer, Niels A1 - Chang, Cun A1 - Zhang, Hou-Xi A1 - Licht, Alexis A1 - Rydin, Catarina A1 - Koutsodendris, Andreas A1 - Han, Fang A1 - Rohrmann, Alexander A1 - Liu, Xiang-Jun A1 - Zhang, Y. A1 - Donnadieu, Yannick A1 - Fluteau, Frederic A1 - Ladant, Jean-Baptiste A1 - Le Hir, Guillaume A1 - Hoorn, M. Carina T1 - Cenozoic evolution of the steppe-desert biome in Central Asia JF - Science Advances N2 - The origins and development of the arid and highly seasonal steppe-desert biome in Central Asia, the largest of its kind in the world, remain largely unconstrained by existing records. It is unclear how Cenozoic climatic, geological, and biological forces, acting at diverse spatial and temporal scales, shaped Central Asian ecosystems through time. Our synthesis shows that the Central Asian steppe-desert has existed since at least Eocene times but experienced no less than two regime shifts, one at the Eocene-Oligocene Transition and one in the mid-Miocene. These shifts separated three successive "stable states," each characterized by unique floral and faunal structures. Past responses to disturbance in the Asian steppe-desert imply that modern ecosystems are unlikely to recover their present structures and diversity if forced into a new regime. This is of concern for Asian steppes today, which are being modified for human use and lost to desertification at unprecedented rates. Y1 - 2020 U6 - https://doi.org/10.1126/sciadv.abb8227 SN - 2375-2548 VL - 6 IS - 41 PB - American Association for the Advancement of Science CY - Washington ER - TY - JOUR A1 - Balischewski, Christian A1 - Behrens, Karsten A1 - Zehbe, Kerstin A1 - Günter, Christina A1 - Mies, Stefan A1 - Sperlich, Eric A1 - Kelling, Alexandra A1 - Taubert, Andreas T1 - Ionic liquids with more than one metal BT - optical and rlectrochemical properties versus d-block metal vombinations JF - Chemistry - a European journal N2 - Thirteen N-butylpyridinium salts, including three monometallic [C4Py](2)[MCl4], nine bimetallic [C4Py](2)[(M1-xMxCl4)-M-a-Cl-b] and one trimetallic compound [C4Py](2)[(M1-y-zMyMz (c) Cl4)-M-a-M-b] (M=Co, Cu, Mn; x=0.25, 0.50 or 0.75 and y=z=0.33), were synthesized and their structure and thermal and electrochemical properties were studied. All compounds are ionic liquids (ILs) with melting points between 69 and 93 degrees C. X-ray diffraction proves that all ILs are isostructural. The conductivity at room temperature is between 10(-4) and 10(-8) S cm(-1). Some Cu-based ILs reach conductivities of 10(-2) S cm(-1), which is, however, probably due to IL dec. This correlates with the optical bandgap measurements indicating the formation of large bandgap semiconductors. At elevated temperatures approaching the melting points, the conductivities reach up to 1.47x10(-1) S cm(-1) at 70 degrees C. The electrochemical stability windows of the ILs are between 2.5 and 3.0 V. KW - bandgap KW - electrochemistry KW - ionic liquids KW - metal-containing ionic KW - liquids KW - tetrahalido metallates Y1 - 2020 U6 - https://doi.org/10.1002/chem.202003097 SN - 0947-6539 SN - 1521-3765 VL - 26 IS - 72 SP - 17504 EP - 17513 PB - Wiley-VCH CY - Weinheim ER - TY - JOUR A1 - Bahr, André A1 - Kolber, Gilles A1 - Kaboth-Bahr, Stefanie A1 - Reinhardt, Lutz A1 - Friedrich, Oliver A1 - Pross, Jörg T1 - Mega-monsoon variability during the late Triassic BT - re-assessing the role of orbital forcing in the deposition of playa sediments in the Germanic Basin JF - Sedimentology : the journal of the International Association of Sedimentologists N2 - The formation of the supercontinent Pangaea during the Permo-Triassic gave rise to an extreme monsoonal climate (often termed 'mega-monsoon') that has been documented by numerous palaeo-records. However, considerable debate exists about the role of orbital forcing in causing humid intervals in an otherwise arid climate. To shed new light on the forcing of monsoonal variability in subtropical Pangaea, this study focuses on sediment facies and colour variability of playa and alluvial fan deposits in an outcrop from the late Carnian (ca 225 Ma) in the southern Germanic Basin, south-western Germany. The sediments were deposited against a background of increasingly arid conditions following the humid Carnian Pluvial Event (ca 234 to 232 Ma). The ca 2 center dot 4 Myr long sedimentary succession studied shows a tripartite long-term evolution, starting with a distal mud-flat facies deposited under arid conditions. This phase was followed by a highly variable playa-lake environment that documents more humid conditions and finally a regression of the playa-lake due to a return of arid conditions. The red-green (a*) and lightness (L*) records show that this long-term variability was overprinted by alternating wet/dry cycles driven by orbital precession and ca 405 kyr eccentricity, without significant influence of obliquity. The absence of obliquity in this record indicates that high-latitude forcing played only a minor role in the southern Germanic Basin during the late Carnian. This is different from the subsequent Norian when high-latitude signals became more pronounced, potentially related to the northward drift of the Germanic Basin. The recurring pattern of pluvial events during the late Triassic demonstrates that orbital forcing, in particular eccentricity, stimulated the occurrence and intensity of wet phases. It also highlights the possibility that the Carnian Pluvial Event, although most likely triggered by enhanced volcanic activity, may also have been modified by an orbital stimulus. KW - Carnian Pluvial Event KW - Germanic Basin KW - Late Triassic KW - mega-monsoon KW - orbital forcing KW - playa-lake Y1 - 2019 U6 - https://doi.org/10.1111/sed.12668 SN - 0037-0746 SN - 1365-3091 VL - 67 IS - 2 SP - 951 EP - 970 PB - Wiley-Blackwell CY - Oxford ER - TY - GEN A1 - Baes, Marzieh A1 - Sobolev, Stephan Vladimir A1 - Gerya, Taras V. A1 - Brune, Sascha T1 - Plume-induced subduction initiation BT - Single-slab or multi-slab subduction? T2 - Postprints der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe N2 - Initiation of subduction following the impingement of a hot buoyant mantle plume is one of the few scenarios that allow breaking the lithosphere and recycling a stagnant lid without requiring any preexisting weak zones. Here, we investigate factors controlling the number and shape of retreating subducting slabs formed by plume-lithosphere interaction. Using 3-D thermomechanical models we show that the deformation regime, which defines formation of single-slab or multi-slab subduction, depends on several parameters such as age of oceanic lithosphere, thickness of the crust and large-scale lithospheric extension rate. Our model results indicate that on present-day Earth multi-slab plume-induced subduction is initiated only if the oceanic lithosphere is relatively young (<30-40 Myr, but >10 Myr), and the crust has a typical thickness of 8 km. In turn, development of single-slab subduction is facilitated by older lithosphere and pre-imposed extensional stresses. In early Earth, plume-lithosphere interaction could have led to formation of either episodic short-lived circular subduction when the oceanic lithosphere was young or to multi-slab subduction when the lithosphere was old. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 1167 KW - subduction zone KW - plume KW - numerical model KW - singleslab KW - multi-slab Y1 - 2021 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-522742 SN - 1866-8372 IS - 2 ER - TY - JOUR A1 - Baes, Marzieh A1 - Sobolev, Stephan V. A1 - Gerya, Taras V. A1 - Brune, Sascha T1 - Subduction initiation by Plume-Plateau interaction BT - insights from numerical models JF - Geochemistry, geophysics, geosystems N2 - It has recently been demonstrated that the interaction of a mantle plume with sufficiently old oceanic lithosphere can initiate subduction. However, the existence of large lithospheric heterogeneities, such as a buoyant plateau, in proximity to a rising plume head may potentially hinder the formation of a new subduction zone. Here, we investigate this scenario by means of 3-D numerical thermomechanical modeling. We explore how plume-lithosphere interaction is affected by lithospheric age, relative location of plume head and plateau border, and the strength of the oceanic crust. Our numerical experiments suggest four different geodynamic regimes: (a) oceanic trench formation, (b) circular oceanic-plateau trench formation, (c) plateau trench formation, and (d) no trench formation. We show that regardless of the age and crustal strength of the oceanic lithosphere, subduction can initiate when the plume head is either below the plateau border or at a distance less than the plume radius from the plateau edge. Crustal heterogeneity facilitates subduction initiation of old oceanic lithosphere. High crustal strength hampers the formation of a new subduction zone when the plume head is located below a young lithosphere containing a thick and strong plateau. We suggest that plume-plateau interaction in the western margin of the Caribbean could have resulted in subduction initiation when the plume head impinged onto the oceanic lithosphere close to the border between plateau and oceanic crust. KW - subduction zone KW - plume KW - plateau KW - numerical modeling KW - plume-induced KW - subduction initiation (PISI) Y1 - 2020 U6 - https://doi.org/10.1029/2020GC009119 SN - 1525-2027 VL - 21 IS - 8 PB - American Geophysical Union CY - Washington ER - TY - JOUR A1 - Baes, Marzieh A1 - Sobolev, Stephan A1 - Gerya, Taras V. A1 - Brune, Sascha T1 - Plume-induced subduction initiation BT - single-slab or multi-slab subduction? JF - Geochemistry, geophysics, geosystems N2 - Initiation of subduction following the impingement of a hot buoyant mantle plume is one of the few scenarios that allow breaking the lithosphere and recycling a stagnant lid without requiring any preexisting weak zones. Here, we investigate factors controlling the number and shape of retreating subducting slabs formed by plume-lithosphere interaction. Using 3-D thermomechanical models we show that the deformation regime, which defines formation of single-slab or multi-slab subduction, depends on several parameters such as age of oceanic lithosphere, thickness of the crust and large-scale lithospheric extension rate. Our model results indicate that on present-day Earth multi-slab plume-induced subduction is initiated only if the oceanic lithosphere is relatively young (<30-40 Myr, but >10 Myr), and the crust has a typical thickness of 8 km. In turn, development of single-slab subduction is facilitated by older lithosphere and pre-imposed extensional stresses. In early Earth, plume-lithosphere interaction could have led to formation of either episodic short-lived circular subduction when the oceanic lithosphere was young or to multi-slab subduction when the lithosphere was old. KW - subduction zone KW - plume KW - numerical model KW - singleslab KW - multi-slab Y1 - 2020 U6 - https://doi.org/10.1029/2019GC008663 SN - 1525-2027 VL - 21 IS - 2 PB - American Geophysical Union CY - Washington ER - TY - GEN A1 - Ayzel, Georgy A1 - Scheffer, Tobias A1 - Heistermann, Maik T1 - RainNet v1.0 BT - a convolutional neural network for radar-based precipitation nowcasting T2 - Postprints der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe N2 - In this study, we present RainNet, a deep convolutional neural network for radar-based precipitation nowcasting. Its design was inspired by the U-Net and SegNet families of deep learning models, which were originally designed for binary segmentation tasks. RainNet was trained to predict continuous precipitation intensities at a lead time of 5min, using several years of quality-controlled weather radar composites provided by the German Weather Service (DWD). That data set covers Germany with a spatial domain of 900km × 900km and has a resolution of 1km in space and 5min in time. Independent verification experiments were carried out on 11 summer precipitation events from 2016 to 2017. In order to achieve a lead time of 1h, a recursive approach was implemented by using RainNet predictions at 5min lead times as model inputs for longer lead times. In the verification experiments, trivial Eulerian persistence and a conventional model based on optical flow served as benchmarks. The latter is available in the rainymotion library and had previously been shown to outperform DWD's operational nowcasting model for the same set of verification events. RainNet significantly outperforms the benchmark models at all lead times up to 60min for the routine verification metrics mean absolute error (MAE) and the critical success index (CSI) at intensity thresholds of 0.125, 1, and 5mm h⁻¹. However, rainymotion turned out to be superior in predicting the exceedance of higher intensity thresholds (here 10 and 15mm h⁻¹). The limited ability of RainNet to predict heavy rainfall intensities is an undesirable property which we attribute to a high level of spatial smoothing introduced by the model. At a lead time of 5min, an analysis of power spectral density confirmed a significant loss of spectral power at length scales of 16km and below. Obviously, RainNet had learned an optimal level of smoothing to produce a nowcast at 5min lead time. In that sense, the loss of spectral power at small scales is informative, too, as it reflects the limits of predictability as a function of spatial scale. Beyond the lead time of 5min, however, the increasing level of smoothing is a mere artifact – an analogue to numerical diffusion – that is not a property of RainNet itself but of its recursive application. In the context of early warning, the smoothing is particularly unfavorable since pronounced features of intense precipitation tend to get lost over longer lead times. Hence, we propose several options to address this issue in prospective research, including an adjustment of the loss function for model training, model training for longer lead times, and the prediction of threshold exceedance in terms of a binary segmentation task. Furthermore, we suggest additional input data that could help to better identify situations with imminent precipitation dynamics. The model code, pretrained weights, and training data are provided in open repositories as an input for such future studies. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 964 KW - weather KW - models KW - skill Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-472942 SN - 1866-8372 IS - 964 ER - TY - JOUR A1 - Ayzel, Georgy A1 - Scheffer, Tobias A1 - Heistermann, Maik T1 - RainNet v1.0 BT - a convolutional neural network for radar-based precipitation nowcasting JF - Geoscientific Model Development N2 - In this study, we present RainNet, a deep convolutional neural network for radar-based precipitation nowcasting. Its design was inspired by the U-Net and SegNet families of deep learning models, which were originally designed for binary segmentation tasks. RainNet was trained to predict continuous precipitation intensities at a lead time of 5min, using several years of quality-controlled weather radar composites provided by the German Weather Service (DWD). That data set covers Germany with a spatial domain of 900km × 900km and has a resolution of 1km in space and 5min in time. Independent verification experiments were carried out on 11 summer precipitation events from 2016 to 2017. In order to achieve a lead time of 1h, a recursive approach was implemented by using RainNet predictions at 5min lead times as model inputs for longer lead times. In the verification experiments, trivial Eulerian persistence and a conventional model based on optical flow served as benchmarks. The latter is available in the rainymotion library and had previously been shown to outperform DWD's operational nowcasting model for the same set of verification events. RainNet significantly outperforms the benchmark models at all lead times up to 60min for the routine verification metrics mean absolute error (MAE) and the critical success index (CSI) at intensity thresholds of 0.125, 1, and 5mm h⁻¹. However, rainymotion turned out to be superior in predicting the exceedance of higher intensity thresholds (here 10 and 15mm h⁻¹). The limited ability of RainNet to predict heavy rainfall intensities is an undesirable property which we attribute to a high level of spatial smoothing introduced by the model. At a lead time of 5min, an analysis of power spectral density confirmed a significant loss of spectral power at length scales of 16km and below. Obviously, RainNet had learned an optimal level of smoothing to produce a nowcast at 5min lead time. In that sense, the loss of spectral power at small scales is informative, too, as it reflects the limits of predictability as a function of spatial scale. Beyond the lead time of 5min, however, the increasing level of smoothing is a mere artifact – an analogue to numerical diffusion – that is not a property of RainNet itself but of its recursive application. In the context of early warning, the smoothing is particularly unfavorable since pronounced features of intense precipitation tend to get lost over longer lead times. Hence, we propose several options to address this issue in prospective research, including an adjustment of the loss function for model training, model training for longer lead times, and the prediction of threshold exceedance in terms of a binary segmentation task. Furthermore, we suggest additional input data that could help to better identify situations with imminent precipitation dynamics. The model code, pretrained weights, and training data are provided in open repositories as an input for such future studies. KW - weather KW - models KW - skill Y1 - 2020 U6 - https://doi.org/10.5194/gmd-13-2631-2020 SN - 1991-959X SN - 1991-9603 VL - 13 IS - 6 SP - 2631 EP - 2644 PB - Copernicus Publ. CY - Göttingen ER - TY - JOUR A1 - Arnous, Ahmad A1 - Zeckra, Martin A1 - Venerdini, Agostina A1 - Alvarado, Patricia A1 - Arrowsmith, Ramón A1 - Guillemoteau, Julien A1 - Landgraf, Angela A1 - Gutiérrez, Adolfo Antonio A1 - Strecker, Manfred T1 - Neotectonic Activity in the Low-Strain Broken Foreland (Santa Bárbara System) of the North-Western Argentinean Andes (26°S) JF - Lithosphere N2 - Uplift in the broken Andean foreland of the Argentine Santa Bárbara System (SBS) is associated with the contractional reactivation of basement anisotropies, similar to those reported from the thick-skinned Cretaceous-Eocene Laramide province of North America. Fault scarps, deformed Quaternary deposits and landforms, disrupted drainage patterns, and medium-sized earthquakes within the SBS suggest that movement along these structures may be a recurring phenomenon, with yet to be defined repeat intervals and rupture lengths. In contrast to the Subandes thrust belt farther north, where eastward-migrating deformation has generated a well-defined thrust front, the SBS records spatiotemporally disparate deformation along structures that are only known to the first order. We present herein the results of geomorphic desktop analyses, structural field observations, and 2D electrical resistivity tomography and seismic-refraction tomography surveys and an interpretation of seismic reflection profiles across suspected fault scarps in the sedimentary basins adjacent to the Candelaria Range (CR) basement uplift, in the south-central part of the SBS. Our analysis in the CR piedmont areas reveals consistency between the results of near-surface electrical resistivity and seismic-refraction tomography surveys, the locations of prominent fault scarps, and structural geometries at greater depth imaged by seismic reflection data. We suggest that this deformation is driven by deep-seated blind thrusting beneath the CR and associated regional warping, while shortening involving Mesozoic and Cenozoic sedimentary strata in the adjacent basins was accommodated by layer-parallel folding and flexural-slip faults that cut through Quaternary landforms and deposits at the surface. Y1 - 2019 U6 - https://doi.org/10.2113/2020/8888588 SN - 1947-4253 SN - 1941-8264 VL - 2020 IS - 1 SP - 1 EP - 25 PB - GSA CY - Boulder, Colo. ER - TY - GEN A1 - Arnous, Ahmad A1 - Zeckra, Martin A1 - Venerdini, Agostina A1 - Alvarado, Patricia A1 - Arrowsmith, Ramón A1 - Guillemoteau, Julien A1 - Landgraf, Angela A1 - Gutiérrez, Adolfo Antonio A1 - Strecker, Manfred T1 - Neotectonic Activity in the Low-Strain Broken Foreland (Santa Bárbara System) of the North-Western Argentinean Andes (26°S) T2 - Postprints der Universität Potsdam : Mathematisch Naturwissenschaftliche Reihe N2 - Uplift in the broken Andean foreland of the Argentine Santa Bárbara System (SBS) is associated with the contractional reactivation of basement anisotropies, similar to those reported from the thick-skinned Cretaceous-Eocene Laramide province of North America. Fault scarps, deformed Quaternary deposits and landforms, disrupted drainage patterns, and medium-sized earthquakes within the SBS suggest that movement along these structures may be a recurring phenomenon, with yet to be defined repeat intervals and rupture lengths. In contrast to the Subandes thrust belt farther north, where eastward-migrating deformation has generated a well-defined thrust front, the SBS records spatiotemporally disparate deformation along structures that are only known to the first order. We present herein the results of geomorphic desktop analyses, structural field observations, and 2D electrical resistivity tomography and seismic-refraction tomography surveys and an interpretation of seismic reflection profiles across suspected fault scarps in the sedimentary basins adjacent to the Candelaria Range (CR) basement uplift, in the south-central part of the SBS. Our analysis in the CR piedmont areas reveals consistency between the results of near-surface electrical resistivity and seismic-refraction tomography surveys, the locations of prominent fault scarps, and structural geometries at greater depth imaged by seismic reflection data. We suggest that this deformation is driven by deep-seated blind thrusting beneath the CR and associated regional warping, while shortening involving Mesozoic and Cenozoic sedimentary strata in the adjacent basins was accommodated by layer-parallel folding and flexural-slip faults that cut through Quaternary landforms and deposits at the surface. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 1008 Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-480183 SN - 1866-8372 IS - 1008 SP - 1 EP - 25 ER - TY - JOUR A1 - Angelopoulos, Michael A1 - Overduin, Pier Paul A1 - Westermann, Sebastian A1 - Tronicke, Jens A1 - Strauss, Jens A1 - Schirrmeister, Lutz A1 - Biskaborn, Boris A1 - Liebner, Susanne A1 - Maksimov, Georgii A1 - Grigoriev, Mikhail N. A1 - Grosse, Guido T1 - Thermokarst lake to lagoon transitions in Eastern Siberia BT - do submerged taliks refreeze? JF - Journal of geophysical research : Earth surface N2 - As the Arctic coast erodes, it drains thermokarst lakes, transforming them into lagoons, and, eventually, integrates them into subsea permafrost. Lagoons represent the first stage of a thermokarst lake transition to a marine setting and possibly more saline and colder upper boundary conditions. In this research, borehole data, electrical resistivity surveying, and modeling of heat and salt diffusion were carried out at Polar Fox Lagoon on the Bykovsky Peninsula, Siberia. Polar Fox Lagoon is a seasonally isolated water body connected to Tiksi Bay through a channel, leading to hypersaline waters under the ice cover. The boreholes in the center of the lagoon revealed floating ice and a saline cryotic bed underlain by a saline cryotic talik, a thin ice-bearing permafrost layer, and unfrozen ground. The bathymetry showed that most of the lagoon had bedfast ice in spring. In bedfast ice areas, the electrical resistivity profiles suggested that an unfrozen saline layer was underlain by a thick layer of refrozen talik. The modeling showed that thermokarst lake taliks can refreeze when submerged in saltwater with mean annual bottom water temperatures below or slightly above 0 degrees C. This occurs, because the top-down chemical degradation of newly formed ice-bearing permafrost is slower than the refreezing of the talik. Hence, lagoons may precondition taliks with a layer of ice-bearing permafrost before encroachment by the sea, and this frozen layer may act as a cap on gas migration out of the underlying talik. KW - thermokarst lake KW - talik KW - lagoon KW - subsea permafrost KW - salt diffusion KW - Siberia Y1 - 2020 U6 - https://doi.org/10.1029/2019JF005424 SN - 2169-9003 SN - 2169-9011 VL - 125 IS - 10 PB - American Geophysical Union CY - Washington ER - TY - THES A1 - Angelopoulos, Michael T1 - Mechanisms of sub-aquatic permafrost evolution in Arctic coastal environments BT - field observations and modelling of submerged ice-rich permafrost deposits and thermokarst lagoons in northeastern Siberia N2 - Subsea permafrost is perennially cryotic earth material that lies offshore. Most submarine permafrost is relict terrestrial permafrost beneath the Arctic shelf seas, was inundated after the last glaciation, and has been warming and thawing ever since. It is a reservoir and confining layer for gas hydrates and has the potential to release greenhouse gases and affect global climate change. Furthermore, subsea permafrost thaw destabilizes coastal infrastructure. While numerous studies focus on its distribution and rate of thaw over glacial timescales, these studies have not been brought together and examined in their entirety to assess rates of thaw beneath the Arctic Ocean. In addition, there is still a large gap in our understanding of sub-aquatic permafrost processes on finer spatial and temporal scales. The degradation rate of subsea permafrost is influenced by the initial conditions upon submergence. Terrestrial permafrost that has already undergone warming, partial thawing or loss of ground ice may react differently to inundation by seawater compared to previously undisturbed ice-rich permafrost. Heat conduction models are sufficient to model the thaw of thick subsea permafrost from the bottom, but few studies have included salt diffusion for top-down chemical degradation in shallow waters characterized by mean annual cryotic conditions on the seabed. Simulating salt transport is critical for assessing degradation rates for recently inundated permafrost, which may accelerate in response to warming shelf waters, a lengthening open water season, and faster coastal erosion rates. In the nearshore zone, degradation rates are also controlled by seasonal processes like bedfast ice, brine injection, seasonal freezing under floating ice conditions and warm freshwater discharge from large rivers. The interplay of all these variables is complex and needs further research. To fill this knowledge gap, this thesis investigates sub-aquatic permafrost along the southern coast of the Bykovsky Peninsula in eastern Siberia. Sediment cores and ground temperature profiles were collected at a freshwater thermokarst lake and two thermokarst lagoons in 2017. At this site, the coastline is retreating, and seawater is inundating various types of permafrost: sections of ice-rich Pleistocene permafrost (Yedoma) cliffs at the coastline alternate with lagoons and lower elevation previously thawed and refrozen permafrost basins (Alases). Electrical resistivity surveys with floating electrodes were carried out to map ice-bearing permafrost and taliks (unfrozen zones in the permafrost, usually formed beneath lakes) along the diverse coastline and in the lagoons. Combined with the borehole data, the electrical resistivity results permit estimation of contemporary ice-bearing permafrost characteristics, distribution, and occasionally, thickness. To conceptualize possible geomorphological and marine evolutionary pathways to the formation of the observed layering, numerical models were applied. The developed model incorporates salt diffusion and seasonal dynamics at the seabed, including bedfast ice. Even along coastlines with mean annual non-cryotic boundary conditions like the Bykovsky Peninsula, the modelling results show that salt diffusion minimizes seasonal freezing of the seabed, leading to faster degradation rates compared to models without salt diffusion. Seasonal processes are also important for thermokarst lake to lagoon transitions because lagoons can generate cold hypersaline conditions underneath the ice cover. My research suggests that ice-bearing permafrost can form in a coastal lagoon environment, even under floating ice. Alas basins, however, may degrade more than twice as fast as Yedoma permafrost in the first several decades of inundation. In addition to a lower ice content compared to Yedoma permafrost, Alas basins may be pre-conditioned with salt from adjacent lagoons. Considering the widespread distribution of thermokarst in the Arctic, its integration into geophysical models and offshore surveys is important to quantify and understand subsea permafrost degradation and aggradation. Through numerical modelling, fieldwork, and a circum-Arctic review of subsea permafrost literature, this thesis provides new insights into sub-aquatic permafrost evolution in saline coastal environments. KW - permafrost KW - subsea KW - submarine KW - thermokarst KW - lagoons KW - salt diffusion KW - electrical resistivity Y1 - 2020 ER - TY - JOUR A1 - Allroggen, Niklas A1 - Beiter, Daniel A1 - Tronicke, Jens T1 - Ground-penetrating radar monitoring of fast subsurface processes JF - Geophysics N2 - Earth and environmental sciences rely on detailed information about subsurface processes. Whereas geophysical techniques typically provide highly resolved spatial images, monitoring subsurface processes is often associated with enormous effort and, therefore, is usually limited to point information in time or space. Thus, the development of spatial and temporal continuous field monitoring methods is a major challenge for the understanding of subsurface processes. We have developed a novel method for ground-penetrating-radar (GPR) reflection monitoring of subsurface flow processes under unsaturated conditions and applied it to a hydrological infiltration experiment performed across a periglacial slope deposit in northwest Luxembourg. Our approach relies on a spatial and temporal quasicontinuous data recording and processing, followed by an attribute analysis based on analyzing differences between individual time steps. The results demonstrate the ability of time-lapse GPR monitoring to visualize the spatial and temporal dynamics of preferential flow processes with a spatial resolution in the order of a few decimeters and temporal resolution in the order of a few minutes. We observe excellent agreement with water table information originating from different boreholes. This demonstrates the potential of surface-based GPR reflection monitoring to observe the spatiotemporal dynamics of water movements in the subsurface. It provides valuable, and so far not accessible, information for example in the field of hydrology and pedology that allows studying the actual subsurface processes rather than deducing them from point information. Y1 - 2020 U6 - https://doi.org/10.1190/GEO2019-0737.1 SN - 0016-8033 SN - 1942-2156 VL - 85 IS - 3 SP - A19 EP - A23 PB - Society of Exploration Geophysicists CY - Tulsa ER -