TY - JOUR A1 - Pilz, Marco A1 - Cotton, Fabrice A1 - Razafindrakoto, Hoby Njara Tendrisoa A1 - Weatherill, Graeme A1 - Spies, Thomas T1 - Regional broad-band ground-shaking modelling over extended and thick sedimentary basins BT - An example from the Lower Rhine Embayment (Germany) JF - Bulletin of earthquake engineering : official publication of the European Association for Earthquake Engineering N2 - The simulation of broad-band (0.1 to 10 + Hz) ground-shaking over deep and spatially extended sedimentary basins at regional scales is challenging. We evaluate the ground-shaking of a potential M 6.5 earthquake in the southern Lower Rhine Embayment, one of the most important areas of earthquake recurrence north of the Alps, close to the city of Cologne in Germany. In a first step, information from geological investigations, seismic experiments and boreholes is combined for deriving a harmonized 3D velocity and attenuation model of the sedimentary layers. Three alternative approaches are then applied and compared to evaluate the impact of the sedimentary cover on ground-motion amplification. The first approach builds on existing response spectra ground-motion models whose amplification factors empirically take into account the influence of the sedimentary layers through a standard parameterization. In the second approach, site-specific 1D amplification functions are computed from the 3D basin model. Using a random vibration theory approach, we adjust the empirical response spectra predicted for soft rock conditions by local site amplification factors: amplifications and associated ground-motions are predicted both in the Fourier and in the response spectra domain. In the third approach, hybrid physics-based ground-motion simulations are used to predict time histories for soft rock conditions which are subsequently modified using the 1D site-specific amplification functions computed in method 2. For large distances and at short periods, the differences between the three approaches become less notable due to the significant attenuation of the sedimentary layers. At intermediate and long periods, generic empirical ground-motion models provide lower levels of amplification from sedimentary soils compared to methods taking into account site-specific 1D amplification functions. In the near-source region, hybrid physics-based ground-motions models illustrate the potentially large variability of ground-motion due to finite source effects. KW - ground-motion modelling KW - site effects KW - scenario KW - random vibration KW - theory KW - hybrid modelling Y1 - 2020 U6 - https://doi.org/10.1007/s10518-020-01004-w SN - 1570-761X SN - 1573-1456 VL - 19 IS - 2 SP - 581 EP - 603 PB - Springer CY - Dordrecht ER - TY - JOUR A1 - Pilz, Tobias A1 - Francke, Till A1 - Baroni, Gabriele A1 - Bronstert, Axel T1 - How to Tailor my process-based hydrological model? BT - dynamic identifiability analysis of flexible model structures JF - Water resources research N2 - In the field of hydrological modeling, many alternative representations of natural processes exist. Choosing specific process formulations when building a hydrological model is therefore associated with a high degree of ambiguity and subjectivity. In addition, the numerical integration of the underlying differential equations and parametrization of model structures influence model performance. Identifiability analysis may provide guidance by constraining the a priori range of alternatives based on observations. In this work, a flexible simulation environment is used to build an ensemble of semidistributed, process-based hydrological model configurations with alternative process representations, numerical integration schemes, and model parametrizations in an integrated manner. The flexible simulation environment is coupled with an approach for dynamic identifiability analysis. The objective is to investigate the applicability of the framework to identify the most adequate model. While an optimal model configuration could not be clearly distinguished, interesting results were obtained when relating model identifiability with hydro-meteorological boundary conditions. For instance, we tested the Penman-Monteith and Shuttleworth & Wallace evapotranspiration models and found that the former performs better under wet and the latter under dry conditions. Parametrization of model structures plays a dominant role as it can compensate for inadequate process representations and poor numerical solvers. Therefore, it was found that numerical solvers of high order of accuracy do often, though not necessarily, lead to better model performance. The proposed coupled framework proved to be a straightforward diagnostic tool for model building and hypotheses testing and shows potential for more in-depth analysis of process implementations and catchment functioning. KW - identifiability analysis KW - flexible model KW - numerics KW - model structure KW - WASA-SED KW - ECHSE Y1 - 2020 U6 - https://doi.org/10.1029/2020WR028042 SN - 0043-1397 SN - 1944-7973 VL - 56 IS - 8 PB - American Geophysical Union CY - Washington ER - TY - JOUR A1 - Powali, Debarchan A1 - Sharma, Shubham A1 - Mandal, Riddhi A1 - Mitra, Supriyo T1 - A reappraisal of the 2005 Kashmir (M-w 7.6) earthquake and its aftershocks BT - seismotectonics of NW Himalaya JF - Tectonophysics : international journal of geotectonics and the geology and physics of the interior of the earth N2 - We study the source properties of the 2005 Kashmir earthquake and its aftershocks to unravel the seismotectonics of the NW Himalayan syntaxis. The mainshock and larger aftershocks have been simultaneously relocated using phase data. We use back-projection of high-frequency energy from multiple teleseismic arrays to model the spatio-temporal evolution of the mainshock rupture. Our analysis reveal a bilateral rupture, which initially propagated SE and then NW of the epicenter, with an average rupture velocity of similar to 2 km s(-1). The area of maximum energy release is parallel to and bound by the surface rupture. Incorporating rupture propagation and velocity, we model the mainshock as a line source using P- and SH-waveform inversion. Our result confirms that the mainshock occurred on a NE dipping (similar to 35 degrees) fault plane, with centroid depth of similar to 10 km. Integrated source time function show that majority of the energy was released in the first similar to 20 s, and was confined above the hypocenter. From waveform inverted fault dimension and seismic moment, we argue that the mainshock had an additional similar to 25 km blind rupture beyond the NW Himalayan syntaxis. Combining this with findings from previous studies, we conjecture that the blind rupture propagated NW of the syntaxis underneath a weak detachment overlain by infra-Cambrian salt layer, and terminated in a wedge thrust. All moderate-to-large aftershocks, NW of the mainshock rupture, are concentrated at the edge of the blind rupture termination. Source modeling of these aftershocks reveal thrust mechanism with centroid depths of 2-10 km, and fault planes oriented subparallel to the mainshock rupture. To study the influence of mainshock rupture on aftershock occurrence, we compute Coulomb failure stress on aftershock faults. All these aftershocks lie in the positive Coulomb stress change region. This suggest that the aftershocks have been triggered by either co-seismic or post-seismic slip on the mainshock fault. KW - Kashmir earthquake KW - Aftershocks KW - High frequency back-projection KW - Source KW - mechanism KW - Coulomb failure stress KW - Seismo-tectonics Y1 - 2020 U6 - https://doi.org/10.1016/j.tecto.2020.228501 SN - 0040-1951 SN - 1879-3266 VL - 789 PB - Elsevier CY - Amsterdam ER - TY - JOUR A1 - Pradhan, Prajal A1 - Kriewald, Steffen A1 - Costa, Luís Fílípe Carvalho da A1 - Rybski, Diego A1 - Benton, Tim G. A1 - Fischer, Günther A1 - Kropp, Jürgen T1 - Urban food systems: how regionalization can contribute to climate change mitigation JF - Environmental science & technology N2 - Cities will play a key role in the grand challenge of nourishing a growing global population, because, due to their population density, they set the demand. To ensure that food systems are sustainable, as well as nourishing, one solution often suggested is to shorten their supply chains toward a regional rather than a global basis. While such regional systems may have a range of costs and benefits, we investigate the mitigation potential of regionalized urban food systems by examining the greenhouse gas emissions associated with food transport. Using data on food consumption for 7108 urban administrative units (UAUs), we simulate total transport emissions for both regionalized and globalized supply chains. In regionalized systems, the UAUs' demands are fulfilled by peripheral food production, whereas to simulate global supply chains, food demand is met from an international pool (where the origin can be any location globally). We estimate that regionalized systems could reduce current emissions from food transport. However, because longer supply chains benefit from maximizing comparative advantage, this emission reduction would require closing yield gaps, reducing food waste, shifting toward diversified farming, and consuming seasonal produce. Regionalization of food systems will be an essential component to limit global warming to well below 2 degrees C in the future. Y1 - 2020 U6 - https://doi.org/10.1021/acs.est.0c02739 SN - 0013-936X SN - 1520-5851 VL - 54 IS - 17 SP - 10551 EP - 10560 PB - American Chemical Society CY - Washington ER - TY - THES A1 - Purinton, Benjamin T1 - Remote sensing applications to earth surface processes in the Eastern Central Andes T1 - Fernerkundungsanwendungen für Erdoberflächenprozesse in den östlichen Zentralanden N2 - Geomorphology seeks to characterize the forms, rates, and magnitudes of sediment and water transport that sculpt landscapes. This is generally referred to as earth surface processes, which incorporates the influence of biologic (e.g., vegetation), climatic (e.g., rainfall), and tectonic (e.g., mountain uplift) factors in dictating the transport of water and eroded material. In mountains, high relief and steep slopes combine with strong gradients in rainfall and vegetation to create dynamic expressions of earth surface processes. This same rugged topography presents challenges in data collection and process measurement, where traditional techniques involving detailed observations or physical sampling are difficult to apply at the scale of entire catchments. Herein lies the utility of remote sensing. Remote sensing is defined as any measurement that does not disturb the natural environment, typically via acquisition of images in the visible- to radio-wavelength range of the electromagnetic spectrum. Remote sensing is an especially attractive option for measuring earth surface processes, because large areal measurements can be acquired at much lower cost and effort than traditional methods. These measurements cover not only topographic form, but also climatic and environmental metrics, which are all intertwined in the study of earth surface processes. This dissertation uses remote sensing data ranging from handheld camera-based photo surveying to spaceborne satellite observations to measure the expressions, rates, and magnitudes of earth surface processes in high-mountain catchments of the Eastern Central Andes in Northwest Argentina. This work probes the limits and caveats of remote sensing data and techniques applied to geomorphic research questions, and presents important progress at this disciplinary intersection. N2 - Die Geomorphologie versucht die Art, Geschwindigkeit und Ausmaße des Sediment- und Wassertransports zu charakterisieren welche zur Formung der Landschaften beitragen. Diese werden im Allgemeinen als Erdoberflächenprozesse bezeichnet, welche den Einfluss biologischer (z.B. Vegetation), klimatischer (z.B. Niederschlag) und tektonischer (z.B. Gebirgshebung) Faktoren auf den Transport von Wasser und das erodierte Material beschreiben. Im Hochgebirge entsteht eine dynamische Wechselwirkung zwischen hohen Reliefs und steilen Hängen und infolge dessen starke Regen- und Vegetationsgradienten. Die gleiche raue Topographie stellt wiederum eine Herausforderung bei der Datenerfassung und Prozessmessung dar, da hier herkömmliche Techniken zur detaillierten Beobachtung oder physikalischen Probenahmen im Maßstab ganzer Einzugsgebiete an ihre Grenzen stoßen. Hier zeigt sich der Nutzen der Fernerkundung. Fernerkundung ist definiert als Messung, welche die natürliche Umgebung nicht stört, typischerweise durch Aufnahme von Bildern im sichtbaren bis Radio-Wellenlängenbereich des elektromagnetischen Spektrums. Fernerkundung ist eine besonders vorteilhafte Option für die Messung von Erdoberflächenprozessen, da großflächige Messungen mit wesentlich geringerem Aufwand als bei herkömmlichen Methoden durchgeführt werden können. Diese Messungen ermöglichen nicht nur das Erfassen der topografischen Form, sondern auch das der Klima- und Umwelteinflüsse, die wiederum bei der Untersuchung von Erdoberflächenprozessen miteinander verknüpft sind. In dieser Dissertation werden Fernerkundungsdaten verwendet, die von kamerabasierten Handaufnahmen bis zu weltraumgestützten Satellitenbeobachtungen reichen, um die Auswirkungen, Geschwindigkeiten und das Ausmaß von Erdoberflächenprozessen in hochgebirgigen Einzugsgebieten der östlichen Zentralanden im Nordwesten Argentiniens zu messen. Diese Arbeit untersucht die Möglichkeiten und Grenzen von Fernerkundungsdaten und -techniken, die auf geomorphologische Forschungsfragen angewendet werden und präsentiert wichtige Fortschritte an diesem disziplinären Schnittpunkt. KW - Fernerkundung KW - remote sensing KW - Geomorphologie KW - geomorphology KW - Anden KW - Andes Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-445926 ER - TY - JOUR A1 - Putra, Muhammad Panji Islam Fajar A1 - Pradhan, Prajal A1 - Kropp, Jürgen T1 - A systematic analysis of Water-Energy-Food security nexus BT - a South Asian case study JF - The science of the total environment : an international journal for scientific research into the environment and its relationship with man N2 - Most South Asian countries have challenges in ensuring water, energy, and food (WEF) security, which are often interacting positively or negatively. To address these challenges, the nexus approach provides a framework to identify the interactions of the WEF sectors as an integrated system. However, most nexus studies only qualitatively discuss the interactions between these sectors. This study conducts a systematic analysis of the WEF security nexus in South Asia by using open data sources at the country scale. We analyze interactions between the WEF sectors statistically, defining positive and negative correlations between the WEF security indicators as synergies and trade-offs, respectively. By creating networks of the synergies and trade-offs, we further identify most positively and negatively influencing indicators in the WEF security nexus. We observe a larger share of trade-offs than synergies within the water and energy sectors and a larger share of synergies than trade-offs among the WEF sectors for South Asia. However, these observations vary across the South Asian countries. Our analysis highlights that strategies on promoting sustainable energy and discouraging fossil fuel use could have overall positive effects on the WEF security nexus in the countries. This study provides evidence for considering the WEF security nexus as an integrated system rather than just a combination of three different sectors or securities. KW - water security KW - food security KW - energy security KW - network analysis KW - water-energy-food nexus KW - sustainable development Y1 - 2020 U6 - https://doi.org/10.1016/j.scitotenv.2020.138451 SN - 0048-9697 SN - 1879-1026 VL - 728 PB - Elsevier CY - Amsterdam ER - TY - JOUR A1 - Racano, Simone A1 - Jara Muñoz, Julius A1 - Cosentino, Domenico A1 - Melnick, Daniel T1 - Variable quaternary uplift along the Southern Margin of the Central Anatolian Plateau inferred from modeling Marine Terrace sequences JF - Tectonics N2 - The southern margin of the Central Anatolian Plateau (CAP) records a strong uplift phase after the early Middle Pleistocene, which has been related to the slab break-off of the subducting Arabian plate beneath the Anatolian microplate. During the last 450 kyr the area underwent an uplift phase at a mean rate of similar to 3.2 m/kyr, as suggested by Middle Pleistocene marine sediments exposed at similar to 1,500 m above sea level. These values are significantly higher than the 1.0-1.5 m/kyr estimated since the Late Pleistocene, suggesting temporal variations in uplift rate. To estimate changes in uplift rate during the Pleistocene we studied the marine terraces along the CAP southern margin, mapping the remnants of the platforms and their associated deposits in the field, and used the TerraceM software to identify the position and elevation of associated shoreline angles. We used shoreline angles and the timing of Quaternary marine sedimentation as constrains for a Landscape Evolution Model that simulates wave erosion of an uplifting coast. We applied random optimization algorithms and minimization statistics to find the input parameters that better reproduce the morphology of CAP marine terraces. The best-fitting uplift rate history suggests a significative increase from 1.9 to 3.5 m/kyr between 500 and 200 kyr, followed by an abrupt decrease to 1.4 m/kyr until the present. Our results agree with slab break-off models, which suggest a strong uplift pulse during slab rupture followed by a smoother decrease. Y1 - 2020 U6 - https://doi.org/10.1029/2019TC005921 SN - 0278-7407 SN - 1944-9194 VL - 39 IS - 12 PB - American Geophysical Union CY - Washington ER - TY - BOOK A1 - Rahmstorf, Stefan A1 - Schellnhuber, Hans Joachim T1 - Der Klimawandel T3 - Schriftenreihe / Bundeszentrale für politische Bildung ; Band 10520 Y1 - 2020 SN - 978-3-7425-0520-0 PB - Bundeszentrale für politische Bildung CY - Bonn ER - TY - JOUR A1 - Rajaonarison, Tahiry A. A1 - Stamps, D. Sarah A1 - Fishwick, Stewart A1 - Brune, Sascha A1 - Glerum, Anne A1 - Hu, Jiashun T1 - Numerical modeling of mantle flow beneath Madagascar to constrain upper mantle rheology beneath continental regions JF - Journal of geophysical research : Solid earth N2 - Over the past few decades, azimuthal seismic anisotropy measurements have been widely used proxy to study past and present-day deformation of the lithosphere and to characterize convection in the mantle. Beneath continental regions, distinguishing between shallow and deep sources of anisotropy remains difficult due to poor depth constraints of measurements and a lack of regional-scale geodynamic modeling. Here, we constrain the sources of seismic anisotropy beneath Madagascar where a complex pattern cannot be explained by a single process such as absolute plate motion, global mantle flow, or geology. We test the hypotheses that either Edge-Driven Convection (EDC) or mantle flow derived from mantle wind interactions with lithospheric topography is the dominant source of anisotropy beneath Madagascar. We, therefore, simulate two sets of mantle convection models using regional-scale 3-D computational modeling. We then calculate Lattice Preferred Orientation that develops along pathlines of the mantle flow models and use them to calculate synthetic splitting parameters. Comparison of predicted with observed seismic anisotropy shows a good fit in northern and southern Madagascar for the EDC model, but the mantle wind case only fits well in northern Madagascar. This result suggests the dominant control of the measured anisotropy may be from EDC, but the role of localized fossil anisotropy in narrow shear zones cannot be ruled out in southern Madagascar. Our results suggest that the asthenosphere beneath northern and southern Madagascar is dominated by dislocation creep. Dislocation creep rheology may be dominant in the upper asthenosphere beneath other regions of continental lithosphere. KW - seismic anisotropy KW - edge-driven convection KW - mantle flow modeling KW - lattice preferred orientations KW - lithosphere-mantle wind interactions KW - splitting parameters Y1 - 2019 U6 - https://doi.org/10.1029/2019JB018560 SN - 2169-9313 SN - 2169-9356 VL - 125 IS - 2 PB - American Geophysical Union CY - Washington ER - TY - JOUR A1 - Ramachandran, Srikanthan A1 - Rupakheti, Maheswar A1 - Lawrence, Mark T1 - Black carbon dominates the aerosol absorption over the Indo-Gangetic Plain and the Himalayan foothills JF - Environment international : a journal of science, technology, health, monitoring and policy N2 - This study, based on new and high quality in situ observations, quantifies for the first time, the individual contributions of light-absorbing aerosols (black carbon (BC), brown carbon (BrC) and dust) to aerosol absorption over the Indo-Gangetic Plain (IGP) and the Himalayan foothill region, a relatively poorly studied region with several sensitive ecosystems of global importance, as well as highly vulnerable populations. The annual and seasonal average single scattering albedo (SSA) over Kathmandu is the lowest of all the locations. The SSA over Kathmandu is < 0.89 during all seasons, which confirms the dominance of light-absorbing carbonaceous aerosols from local and regional sources over Kathmandu. It is observed here that the SSA decreases with increasing elevation, confirming the dominance of light absorbing carbonaceous aerosols at higher elevations. In contrast, the SSA over the IGP does not exhibit a pronounced spatial variation. BC dominates (>= 75%) the aerosol absorption over the IGP and the Himalayan foothills throughout the year. Higher BC concentration at elevated locations in the Himalayas leads to lower SSA at elevated locations in the Himalayas. The contribution of dust to aerosol absorption is higher throughout the year over the IGP than over the Himalayan foothills. The aerosol absorption over South Asia is very high, exceeding available observations over East Asia, and also exceeds previous model estimates. This quantification will be valuable as observational constraints to help improve regional simulations of climate change, impacts on the glaciers and the hydrological cycle, and will help to direct the focus towards BC as the main contributor to aerosol-induced warming in the region. KW - atmospheric aerosols KW - characteristics KW - absorption KW - black carbon KW - brown KW - carbon KW - dust KW - Himalayas KW - IGP KW - South Asia Y1 - 2020 U6 - https://doi.org/10.1016/j.envint.2020.105814 SN - 0160-4120 SN - 1873-6750 VL - 142 PB - Elsevier CY - Oxford ER - TY - THES A1 - Ramezani Ziarani, Maryam T1 - Characterization of atmospheric processes related to hydro-meteorological extreme events over the south-central Andes N2 - The significant environmental and socioeconomic consequences of hydrometeorological extreme events, such as extreme rainfall, are constituted as a most important motivation for analyzing these events in the south-central Andes of NW Argentina. The steep topographic and climatic gradients and their interactions frequently lead to the formation of deep convective storms and consequently trigger extreme rainfall generation. In this dissertation, I focus on identifying the dominant climatic variables and atmospheric conditions and their spatiotemporal variability leading to deep convection and extreme rainfall in the south-central Andes. This dissertation first examines the significant contribution of temperature on atmospheric humidity (dew-point temperature, Td) and on convection (convective available potential energy, CAPE) for deep convective storms and hence, extreme rainfall along the topographic and climatic gradients. It was found that both climatic variables play an important role in extreme rainfall generation. However, their contributions differ depending on topographic and climatic sub-regions, as well as rainfall percentiles. Second, this dissertation explores if (near real-time) the measurements conducted by the Global Navigation Satellite System (GNSS) on integrated water vapor (IWV) provide reliable data for explaining atmospheric humidity. I argue that GNSS-IWV, in conjunction with other atmospheric stability parameters such as CAPE, is able to decipher the extreme rainfall in the eastern central Andes. In my work, I rely on a multivariable regression analysis described by a theoretical relationship and fitting function analysis. Third, this dissertation identifies the local impact of convection on extreme rainfall in the eastern Andes. Relying on a Principal Component Analysis (PCA) it was found that during the existence of moist and warm air, extreme rainfall is observed more often during local night hours. The analysis includes the mechanisms for this observation. Exploring the atmospheric conditions and climatic variables leading to extreme rainfall is one of the main findings of this dissertation. The conditions and variables are a prerequisite for understanding the dynamics of extreme rainfall and predicting these events in the eastern Andes. N2 - Die entscheidenden ökologischen und sozioökonomischen Folgen hydrometeorologischer Extremereignisse, wie z.B. extremer Niederschläge, stellen eine wichtige Motivation für die Analyse dieser Ereignisse in den südlich-zentralen Anden von NW Argentinien dar. Die steilen topographischen und klimatischen Gradienten und deren Wechselwirkungen führen häufig zu einer starken konvektiven Regenfallbildung und sind häufig auch die Auslöser von Starkniederschlägen. In dieser Dissertation konzentriere ich mich auf die Identifizierung der dominanten klimatischen Variablen und atmosphärischen Rahmenbedingungen und ihrer räumlich-zeitliche Variabilität, die zu starker Konvektion und extremen Niederschlägen in den südlich-zentralen Anden führt. Diese Dissertation untersucht zunächst den wichtigen Beitrag der Temperatur zur Luftfeuchtigkeit(Taupunkttemperatur, Td) und zur Konvektion (konvektive verfügbare potenzielle Energie, CAPE) für starke, konvektive Stürme und damit extreme Niederschläge entlang der topographischen und klimatischen Gradienten. Es wurde festgestellt, dass beide klimatischen Variablen eine wichtige Rolle bei der Erzeugung extremer Niederschläge spielen. Ihr Beitrag hängt jedoch von den topographischen und klimatischen Teilregionen sowie den Niederschlagsperzentilen ab. Zweitens, auf der Grundlage einer multivariablen Regressionsanalyse, die durch eine theoretische Beziehungs- und Anpassungsfunktionsanalyse beschrieben wird, untersucht diese Arbeit, ob integrierter Wasserdampf (IWV) auf der Grundlage von GNSS (Global Navigation Satellite System) Messungen zuverlässige Daten sind, um die Luftfeuchtigkeit zu erklären. Das GNSS-IWV in Verbindung mit anderen atmosphärischen Stabilitätsparametern wie z.B. CAPE ist in der Lage, die extremen Niederschläge in den östlichen zentralen Anden zu entschlüsseln. Drittens, diese Dissertation identifiziert die lokalen Auswirkungen der Konvektion auf extreme Niederschläge in den östlichen Anden. Auf der Grundlage einer Hauptkomponentenanalyse (PCA) wurde festgestellt, dass die extremen Niederschläge häufiger während der lokalen Nachtstunden beobachtet werden, wenn feuchte und warme Luft vorhanden ist. Die Erforschung der atmosphärischen Rahmenbedingungen und klimatischen Variablen, die zu extremen Niederschlägen führen, ist eines der wichtigste Ergebnisse dieser Arbeit. Sie ist Voraussetzung für das Verständnis der Dynamik von extremen Niederschlägen und wichtig für die Vorhersage dieser Ereignisse in den östlichen Anden. T2 - Charakterisierung der atmosphärischen Prozesse im Zusammenhang mit hydro-meteorologischen Extremereignissen über den süd-zentralen Anden KW - eastern south–central Andes KW - extreme rainfall KW - deep convection KW - östlich-südzentrale Anden KW - Extremniederschläge KW - starker Konvektion Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-471755 ER - TY - JOUR A1 - Rein, Theresa A1 - Hannemann, Katrin A1 - Thomas, Christine A1 - Korn, Michael T1 - Location and characteristics of the X-discontinuity beneath SW Morocco and the adjacent shelf area using P-wave receiver functions JF - Geophysical journal international N2 - Receiver function approaches have proven to be valuable for the investigation of crustal and upper mantle discontinuities whose sharp changes in seismic velocities cause wave conversions. While the crustal and mantle transition zone discontinuities are largely understood, the X-discontinuity at 250-350 km depth is still an object of controversial debate. The origin and global distribution of this structure with a velocity jump of 1.5-4.8% for compressional and shear waves is still unexplained. Although the crustal and mantle transition zone discontinuities beneath SW Morocco and surroundings have been investigated, only a few studies observed the X-discontinuity and place the depth at 260-370 km beneath the region of western Morocco. In order to better locate and characterize the X-discontinuity beneath southwest Morocco, we create P-wave receiver functions using data recorded by the Morocco-Munster array and detect the X-discontinuity at apparent depths of 285-350 km. In the western part of our study region we find apparent depths of similar to 310-340 km. The eastern part of the study area appears more complex: we locate two velocity jumps at apparent depths of around 285-295 km and 330-350 km in the northeast, and in the southeast we find a discontinuity at apparent depths of 340-350 km. Due to the large depth range and the twofold appearance of the X-discontinuity, we suggest that two different phase transitions cause the X-discontinuity beneath SW Morocco. The velocity contrasts at larger depths likely point to the coesite-stishovite phase transition occurring in deep eclogitic pools. The shallower depths can be explained by the transition from orthoenstatite to high-pressure clinoenstatite which requires the reaction between eclogite and peridotite to form orthopyroxene-rich peridotite. This reaction is likely related to previously proposed small-scale mantle upwellings beneath SW Morocco. Since both phase transitions require eclogite occurrence, the location of the X-discontinuity in this region can be used to indicate the location of recycled oceanic crust. KW - body waves KW - mantle discontinuities KW - NW Morocco KW - P-waves Y1 - 2020 U6 - https://doi.org/10.1093/gji/ggaa379 SN - 0956-540X SN - 1365-246X VL - 223 IS - 3 SP - 1780 EP - 1793 PB - Oxford Univ. Press CY - Oxford ER - TY - GEN A1 - Repasch, Marisa A1 - Wittmann, Hella A1 - Scheingross, Joel S. A1 - Sachse, Dirk A1 - Szupiany, Ricardo A1 - Orfeo, Oscar A1 - Fuchs, Margret A1 - Hovius, Niels T1 - Sediment Transit Time and Floodplain Storage Dynamics in Alluvial Rivers Revealed by Meteoric 10Be T2 - Postprints der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe N2 - Quantifying the time scales of sediment transport and storage through river systems is fundamental for understanding weathering processes, biogeochemical cycling, and improving watershed management, but measuring sediment transit time is challenging. Here we provide the first systematic test of measuring cosmogenic meteoric Beryllium-10 (10Bem) in the sediment load of a large alluvial river to quantify sediment transit times. We take advantage of a natural experiment in the Rio Bermejo, a lowland alluvial river traversing the east Andean foreland basin in northern Argentina. This river has no tributaries along its trunk channel for nearly 1,300 km downstream from the mountain front. We sampled suspended sediment depth profiles along the channel and measured the concentrations of 10Bem in the chemically extracted grain coatings. We calculated depth-integrated 10Bem concentrations using sediment flux data and found that 10Bem concentrations increase 230% from upstream to downstream, indicating a mean total sediment transit time of 8.4 ± 2.2 kyr. Bulk sediment budget-based estimates of channel belt and fan storage times suggest that the 10Bem tracer records mixing of old and young sediment reservoirs. On a reach scale, 10Bem transit times are shorter where the channel is braided and superelevated above the floodplain, and longer where the channel is incised and meandering, suggesting that transit time is controlled by channel morphodynamics. This is the first systematic application of 10Bem as a sediment transit time tracer and highlights the method's potential for inferring sediment routing and storage dynamics in large river systems. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 1119 KW - meteoric 10Be KW - sediment transit time KW - river sediment KW - floodplains KW - sediment routing Y1 - 2021 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-494324 SN - 1866-8372 IS - 1119 ER - TY - JOUR A1 - Repasch, Marisa A1 - Wittmann, Hella A1 - Scheingross, Joel S. A1 - Sachse, Dirk A1 - Szupiany, Ricardo A1 - Orfeo, Oscar A1 - Fuchs, Margret A1 - Hovius, Niels T1 - Sediment Transit Time and Floodplain Storage Dynamics in Alluvial Rivers Revealed by Meteoric 10Be JF - Journal of Geophysical Research: Earth Surface N2 - Quantifying the time scales of sediment transport and storage through river systems is fundamental for understanding weathering processes, biogeochemical cycling, and improving watershed management, but measuring sediment transit time is challenging. Here we provide the first systematic test of measuring cosmogenic meteoric Beryllium-10 (10Bem) in the sediment load of a large alluvial river to quantify sediment transit times. We take advantage of a natural experiment in the Rio Bermejo, a lowland alluvial river traversing the east Andean foreland basin in northern Argentina. This river has no tributaries along its trunk channel for nearly 1,300 km downstream from the mountain front. We sampled suspended sediment depth profiles along the channel and measured the concentrations of 10Bem in the chemically extracted grain coatings. We calculated depth-integrated 10Bem concentrations using sediment flux data and found that 10Bem concentrations increase 230% from upstream to downstream, indicating a mean total sediment transit time of 8.4 ± 2.2 kyr. Bulk sediment budget-based estimates of channel belt and fan storage times suggest that the 10Bem tracer records mixing of old and young sediment reservoirs. On a reach scale, 10Bem transit times are shorter where the channel is braided and superelevated above the floodplain, and longer where the channel is incised and meandering, suggesting that transit time is controlled by channel morphodynamics. This is the first systematic application of 10Bem as a sediment transit time tracer and highlights the method's potential for inferring sediment routing and storage dynamics in large river systems. KW - meteoric 10Be KW - sediment transit time KW - river sediment KW - floodplains KW - sediment routing Y1 - 2019 U6 - https://doi.org/10.1029/2019JF005419 SN - 2169-9011 SN - 2169-9003 VL - 125 PB - Wiley CY - Hoboken, NJ ER - TY - JOUR A1 - Reschke, Maria A1 - Kröner, Igor A1 - Laepple, Thomas T1 - Testing the consistency of Holocene and Last Glacial Maximum spatial correlations in temperature proxy records JF - Journal of quaternary science : JQS N2 - Holocene temperature proxy records are commonly used in quantitative synthesis and model-data comparisons. However, comparing correlations between time series from records collected in proximity to one another with the expected correlations based on climate model simulations indicates either regional or noisy climate signals in Holocene temperature proxy records. In this study, we evaluate the consistency of spatial correlations present in Holocene proxy records with those found in data from the Last Glacial Maximum (LGM). Specifically, we predict correlations expected in LGM proxy records if the only difference to Holocene correlations would be due to more time uncertainty and more climate variability in the LGM. We compare this simple prediction to the actual correlation structure in the LGM proxy records. We found that time series data of ice-core stable isotope records and planktonic foraminifera Mg/Ca ratios were consistent between the Holocene and LGM periods, while time series of Uk'37 proxy records were not as we found no correlation between nearby LGM records. Our results support the finding of highly regional or noisy marine proxy records in the compilation analysed here and suggest the need for further studies on the role of climate proxies and the processes of climate signal recording and preservation. KW - Holocene KW - LGM KW - spatial correlation KW - temperature KW - Uk'37 Y1 - 2020 U6 - https://doi.org/10.1002/jqs.3245 SN - 0267-8179 SN - 1099-1417 VL - 36 IS - 1 SP - 20 EP - 28 PB - Wiley CY - New York ER - TY - JOUR A1 - Richter, Gudrun A1 - Hainzl, Sebastian A1 - Dahm, Torsten A1 - Zöller, Gert T1 - Stress-based, statistical modeling of the induced seismicity at the Groningen gas field BT - the Netherlands JF - Environmental earth sciences N2 - Groningen is the largest onshore gas field under production in Europe. The pressure depletion of the gas field started in 1963. In 1991, the first induced micro-earthquakes have been located at reservoir level with increasing rates in the following decades. Most of these events are of magnitude less than 2.0 and cannot be felt. However, maximum observed magnitudes continuously increased over the years until the largest, significant event with ML=3.6 was recorded in 2014, which finally led to the decision to reduce the production. This causal sequence displays the crucial role of understanding and modeling the relation between production and induced seismicity for economic planing and hazard assessment. Here we test whether the induced seismicity related to gas exploration can be modeled by the statistical response of fault networks with rate-and-state-dependent frictional behavior. We use the long and complete local seismic catalog and additionally detailed information on production-induced changes at the reservoir level to test different seismicity models. Both the changes of the fluid pressure and of the reservoir compaction are tested as input to approximate the Coulomb stress changes. We find that the rate-and-state model with a constant tectonic background seismicity rate can reproduce the observed long delay of the seismicity onset. In contrast, so-called Coulomb failure models with instantaneous earthquake nucleation need to assume that all faults are initially far from a critical state of stress to explain the delay. Our rate-and-state model based on the fluid pore pressure fits the spatiotemporal pattern of the seismicity best, where the fit further improves by taking the fault density and orientation into account. Despite its simplicity with only three free parameters, the rate-and-state model can reproduce the main statistical features of the observed activity. KW - induced seismicity KW - modeling KW - statistical seismology KW - forecast Y1 - 2020 U6 - https://doi.org/10.1007/s12665-020-08941-4 SN - 1866-6280 SN - 1866-6299 VL - 79 IS - 11 PB - Springer CY - New York ER - TY - JOUR A1 - Riedl, Simon A1 - Melnick, Daniel A1 - Mibei, Geoffrey K. A1 - Njue, Lucy A1 - Strecker, Manfred T1 - Continental rifting at magmatic centres BT - structural implications from the Late Quaternary Menengai Caldera, central Kenya Rift JF - Journal of the geological society N2 - The structural evolution of calderas in rifts helps to characterize the spatiotemporal relationships between magmatism, long wavelength crustal deformation and the formation of tectonic deformation zones along the rift axis. We document the structural characteristics of the c. 36 ka old Menengai Caldera located within a young zone of extension in the central Kenya Rift. Field mapping and high-resolution digital surface models show that NNE-striking Holocene normal faults perpendicular to the regional ESE-WNWextension direction dominate the interior sectors of the rift. Inside the caldera, these structures are overprinted by post-collapse doming and faulting of the magmatic centre, resulting in obliquely slipping normal faults bounding a resurgence horst. Radiocarbon dating of faulted units as young as 5 ka cal BP and the palaeo-shorelines of a lake formed during the African Humid Period in the Nakuru Basin indicate that volcanism and fault activity inside and in the vicinity of Menengai must have been sustained during the Holocene. Our analysis confirms that the caldera is located at the centre of an extending rift segment and suggests that other magmatic centres and young zones of faulting along the volcano-tectonic axis of the Kenya Rift may constitute nucleation points of faulting that ultimately foster future continental break-up. Y1 - 2020 U6 - https://doi.org/10.1144/jgs2019-021 SN - 0016-7649 SN - 2041-479X VL - 177 IS - 1 SP - 153 EP - 169 PB - Geological Soc. Publ. House CY - Bath ER - TY - GEN A1 - Rodriguez Piceda, Constanza A1 - Scheck Wenderoth, Magdalena A1 - Gomez Dacal, Maria Laura A1 - Bott, Judith A1 - Prezzi, Claudia Beatriz A1 - Strecker, Manfred T1 - Lithospheric density structure of the southern Central Andes constrained by 3D data-integrative gravity modelling T2 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe N2 - The southern Central Andes (SCA) (between 27 degrees S and 40 degrees S) is bordered to the west by the convergent margin between the continental South American Plate and the oceanic Nazca Plate. The subduction angle along this margin is variable, as is the deformation of the upper plate. Between 33 degrees S and 35 degrees S, the subduction angle of the Nazca plate increases from sub-horizontal (< 5 degrees) in the north to relatively steep (similar to 30 degrees) in the south. The SCA contain inherited lithological and structural heterogeneities within the crust that have been reactivated and overprinted since the onset of subduction and associated Cenozoic deformation within the Andean orogen. The distribution of the deformation within the SCA has often been attributed to the variations in the subduction angle and the reactivation of these inherited heterogeneities. However, the possible influence that the thickness and composition of the continental crust have had on both short-term and long-term deformation of the SCA is yet to be thoroughly investigated. For our investigations, we have derived density distributions and thicknesses for various layers that make up the lithosphere and evaluated their relationships with tectonic events that occurred over the history of the Andean orogeny and, in particular, investigated the short- and long-term nature of the present-day deformation processes. We established a 3D model of lithosphere beneath the orogen and its foreland (29 degrees S-39 degrees S) that is consistent with currently available geological and geophysical data, including the gravity data. The modelled crustal configuration and density distribution reveal spatial relationships with different tectonic domains: the crystalline crust in the orogen (the magmatic arc and the main orogenic wedge) is thicker (similar to 55 km) and less dense (similar to 2900 kg/m(3)) than in the forearc (similar to 35 km, similar to 2975 kg/m(3)) and foreland (similar to 30 km, similar to 3000 kg/m(3)). Crustal thickening in the orogen probably occurred as a result of stacking of low-density domains, while density and thickness variations beneath the forearc and foreland most likely reflect differences in the tectonic evolution of each area following crustal accretion. No clear spatial relationship exists between the density distribution within the lithosphere and previously proposed boundaries of crustal terranes accreted during the early Paleozoic. Areas with ongoing deformation show a spatial correlation with those areas that have the highest topographic gradients and where there are abrupt changes in the average crustal-density contrast. This suggests that the short-term deformation within the interior of the Andean orogen and its foreland is fundamentally influenced by the crustal composition and the relative thickness of different crustal layers. A thicker, denser, and potentially stronger lithosphere beneath the northern part of the SCA foreland is interpreted to have favoured a strong coupling between the Nazca and South American plates, facilitating the development of a sub-horizontal slab. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 1369 KW - Central andes KW - Lithospheric structure KW - Crustal density KW - Gravity KW - modelling KW - Subduction Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-562628 SN - 1866-8372 IS - 7 ER - TY - JOUR A1 - Rodriguez Piceda, Constanza A1 - Scheck Wenderoth, Magdalena A1 - Gomez Dacal, Maria Laura A1 - Bott, Judith A1 - Prezzi, Claudia Beatriz A1 - Strecker, Manfred T1 - Lithospheric density structure of the southern Central Andes constrained by 3D data-integrative gravity modelling JF - International journal of earth sciences N2 - The southern Central Andes (SCA) (between 27 degrees S and 40 degrees S) is bordered to the west by the convergent margin between the continental South American Plate and the oceanic Nazca Plate. The subduction angle along this margin is variable, as is the deformation of the upper plate. Between 33 degrees S and 35 degrees S, the subduction angle of the Nazca plate increases from sub-horizontal (< 5 degrees) in the north to relatively steep (similar to 30 degrees) in the south. The SCA contain inherited lithological and structural heterogeneities within the crust that have been reactivated and overprinted since the onset of subduction and associated Cenozoic deformation within the Andean orogen. The distribution of the deformation within the SCA has often been attributed to the variations in the subduction angle and the reactivation of these inherited heterogeneities. However, the possible influence that the thickness and composition of the continental crust have had on both short-term and long-term deformation of the SCA is yet to be thoroughly investigated. For our investigations, we have derived density distributions and thicknesses for various layers that make up the lithosphere and evaluated their relationships with tectonic events that occurred over the history of the Andean orogeny and, in particular, investigated the short- and long-term nature of the present-day deformation processes. We established a 3D model of lithosphere beneath the orogen and its foreland (29 degrees S-39 degrees S) that is consistent with currently available geological and geophysical data, including the gravity data. The modelled crustal configuration and density distribution reveal spatial relationships with different tectonic domains: the crystalline crust in the orogen (the magmatic arc and the main orogenic wedge) is thicker (similar to 55 km) and less dense (similar to 2900 kg/m(3)) than in the forearc (similar to 35 km, similar to 2975 kg/m(3)) and foreland (similar to 30 km, similar to 3000 kg/m(3)). Crustal thickening in the orogen probably occurred as a result of stacking of low-density domains, while density and thickness variations beneath the forearc and foreland most likely reflect differences in the tectonic evolution of each area following crustal accretion. No clear spatial relationship exists between the density distribution within the lithosphere and previously proposed boundaries of crustal terranes accreted during the early Paleozoic. Areas with ongoing deformation show a spatial correlation with those areas that have the highest topographic gradients and where there are abrupt changes in the average crustal-density contrast. This suggests that the short-term deformation within the interior of the Andean orogen and its foreland is fundamentally influenced by the crustal composition and the relative thickness of different crustal layers. A thicker, denser, and potentially stronger lithosphere beneath the northern part of the SCA foreland is interpreted to have favoured a strong coupling between the Nazca and South American plates, facilitating the development of a sub-horizontal slab. KW - Central andes KW - Lithospheric structure KW - Crustal density KW - Gravity KW - modelling KW - Subduction Y1 - 2020 U6 - https://doi.org/10.1007/s00531-020-01962-1 SN - 1437-3254 SN - 1437-3262 VL - 110 IS - 7 SP - 2333 EP - 2359 PB - Springer CY - New York ER - TY - THES A1 - Rodriguez Zuluaga, Juan T1 - Electric and magnetic characteristics of equatorial plasma depletions T1 - Elektrische und magnetische Beschreibung von äquatorialen Plasma-Verarmungen BT - an observational assessment using the Swarm mission BT - eine empirische Beurteilung mit der Satellitenmission Swarm N2 - Near-Earth space represents a significant scientific and technological challenge. Particularly at magnetic low-latitudes, the horizontal magnetic field geometry at the dip equator and its closed field-lines support the existence of a distinct electric current system, abrupt electric field variations and the development of plasma irregularities. Of particular interest are small-scale irregularities associated with equatorial plasma depletions (EPDs). They are responsible for the disruption of trans-ionospheric radio waves used for navigation, communication, and Earth observation. The fast increase of satellite missions makes it imperative to study the near-Earth space, especially the phenomena known to harm space technology or disrupt their signals. EPDs correspond to the large-scale structure (i.e., tens to hundreds of kilometers) of topside F region irregularities commonly known as Spread F. They are observed as depleted-plasma density channels aligned with the ambient magnetic field in the post-sunset low-latitude ionosphere. Although the climatological variability of their occurrence in terms of season, longitude, local time and solar flux is well-known, their day to day variability is not. The sparse observations from ground-based instruments like radars and the few simultaneous measurements of ionospheric parameters by space-based instruments have left gaps in the knowledge of EPDs essential to comprehend their variability. In this dissertation, I profited from the unique observations of the ESA’s Swarm constellation mission launched in November 2013 to tackle three issues that revealed novel and significant results on the current knowledge of EPDs. I used Swarm’s measurements of the electron density, magnetic, and electric fields to answer, (1.) what is the direction of propagation of the electromagnetic energy associated with EPDs?, (2.) what are the spatial and temporal characteristics of the electric currents (field-aligned and diamagnetic currents) related to EPDs, i.e., seasonal/geographical, and local time dependencies?, and (3.) under what conditions does the balance between magnetic and plasma pressure across EPDs occur? The results indicate that: (1.) The electromagnetic energy associated with EPDs presents a preference for interhemispheric flows; that is, the related Poynting flux directs from one magnetic hemisphere to the other and varies with longitude and season. (2.) The field-aligned currents at the edges of EPDs are interhemispheric. They generally close in the hemisphere with the highest Pedersen conductance. Such hemispherical preference presents a seasonal/longitudinal dependence. The diamagnetic currents increase or decrease the magnetic pressure inside EPDs. These two effects rely on variations of the plasma temperature inside the EPDs that depend on longitude and local time. (3.) EPDs present lower or higher plasma pressure than the ambient. For low-pressure EPDs the plasma pressure gradients are mostly dominated by variations of the plasma density so that variations of the temperature are negligible. High-pressure EPDs suggest significant temperature variations with magnitudes of approximately twice the ambient. Since their occurrence is more frequent in the vicinity of the South Atlantic magnetic anomaly, such high temperatures are suggested to be due to particle precipitation. In a broader context, this dissertation shows how dedicated satellite missions with high-resolution capabilities improve the specification of the low-latitude ionospheric electrodynamics and expand knowledge on EPDs which is valuable for current and future communication, navigation, and Earth-observing missions. The contributions of this investigation represent several ’firsts’ in the study of EPDs: (1.) The first observational evidence of interhemispheric electromagnetic energy flux and field-aligned currents. (2.) The first spatial and temporal characterization of EPDs based on their associated field-aligned and diamagnetic currents. (3.) The first evidence of high plasma pressure in regions of depleted plasma density in the ionosphere. These findings provide new insights that promise to advance our current knowledge of not only EPDs but the low-latitude post-sunset ionosphere environment. N2 - Der erdnahe Weltraum stellt eine bedeutende wissenschaftliche und technologische Herausforderung dar. Insbesondere in niedrigeren magnetischen Breitengraden unterstützen die horizontale Geometrie des Magnetfelds und seine geschlossenen Feldlinien das Vorhandensein eines speziellen elektrischen Stromsystems, abrupte Änderungen der elektrischen Felder und das Auftreten von Plasmairregularitäten. Von besonderem Interesse sind regionale Unregelmäßigkeiten im Zusammenhang mit äquatorialen Plasma-Verarmungen (EPDs, Abkürzung aus dem Englischen für „equatorial plasma depletions”). Sie stören trans-ionosphärischer Funkwellen, welche zur Positionierung, Kommunikation und Erd-beobachtung eingesetzt werden. Die schnelle Entwicklung von Satellitenmissionen macht das Verständnis der erdnahen Weltraumphänomene zu einer Priorität, insbesondere derjenigen, welche die Weltraumtechnologie schädigen oder ihre Signale stören können. Die EPDs und die damit verbundenen Plasmairregularitäten sind seit Beginn des Weltraumzeitalters eines der am häufigsten untersuchten Phänomene. EPDs sind großflächigen Strukturen (d. h. zehn bis hundert Kilometer), die auf Spread F Ereignisse zurückgeführt werden können. Sie äußern sich als mit dem Hintergrund-Magnetfeld ausgerichtete Kanäle verarmter Plasmadichte, welche in niedrigen Breiten in der Ionophäre nach Sonnenuntergang auftreten. Obwohl die klimatologische Variabilität des Auftretens von EPDs bezüglich der Jahreszeit, geografischen Länge, Ortszeit und des Sonnenzyklus wohl bekannt sind, trifft dies nicht für ihre Tag-zu-Tag-Variabilität zu. Die spärlichen Beobachtungen von bodengestützten Instrumenten, wie Radargeräten, und die wenigen gleichzeitigen Messungen ionosphärischer Parameter von weltraumgestützten Instrumenten auf erdnahen Umlaufbahnen haben Wissenslücken hinterlassen, die für das Verständnis der Variabilität von EPDs essentiell sind. In dieser Dissertation habe ich von einzigartigen Beobachtungen der im November 2013 gestarteten ESA Satellitenkonstellationsmission „Swarm“ profitiert, um drei Probleme zu bearbeiten, die neue und signifikante Ergebnisse zum aktuellen Wissen über EPDs enthüllten. Ich habe Swarms Messungen der Elektronendichte, des magnetischen und des elektrischen Feldes verwendet, um Folgendes zu beantworten: (1.) In welche Richtung breitet sich die mit den EPDs verbundene elektromagnetische Energie aus? (2.) Was sind die räumlichen und zeitlichen Eigenschaften der elektrischen Ströme (feldgerichtete und diamagnetische Ströme) in Bezug auf EPDs, d. h. wie hängen sie von der geografischen Länge, Jahreszeit und Lokalzeit ab? (3.) Unter welchen Bedingungen findet der mit EPDs verbundene Ausgleich zwischen magnetischem Druck und Plasmadruck statt? Die Ergebnisse zeigen, dass: (1.) Die mit EPDs verbundene elektromagnetische Energie bevorzugt interhemisphärische Strömungen, das heißt, der zugehörige Poynting-Fluss strömt von einer magnetischen Hemisphäre zur anderen und die Strömungsrichtung variiert mit geografischer Länge und Jahreszeit. (2.) Die feldgerichteten Ströme an den Rändern von EPDs sind interhemisphärisch. Im Allgemeinen schließen sie sich in der Hemisphäre mit der höchsten Pedersen-Leitfähigkeit. Die derartige hemisphärische Präferenz zeigt eine Abhängigkeit bezüglich der Jahreszeit/geografischen Länge. Die diamagnetischen Ströme erhöhen oder verringern den magnetischen Druck innerhalb der EPDs. Diese beiden Effekte beruhen auf Variationen der Plasmatemperatur innerhalb der EPDs, die von der geografischen Länge und der Lokalzeit abhängt. (3.) EPDs weisen einen höheren oder niedrigeren Plasmadruck als ihre Umgebung auf. In Niederdruck-EPDs werden die Plasmadruckgradienten meist durch Variationen der Plasmadichte hervorgerufen, sodass Temperaturschwankungen vernachlässigbar sind. Hochdruck-EPDs deuten auf hohe innere Temperaturen hin, etwa das Zweifache der Umgebungstemperatur. Aufgrund ihres häufigeren Auftretens in der Nähe der Südatlantischen Magnetfeldanomalie wird vermutet, dass solche hohen Temperaturen auf den Einfall hochenergetischer Teilchen zurückzuführen sind. In einem breiteren Kontext zeigt diese Dissertation auf, wie spezielle Satellitenmissionen mit hohem Auflösungsvermögen die Spezifikation der ionoshärischen Elektrodynamik in niedrigen Breiten und das Verständnis von EPDs verbessern, was wertvoll für aktuelle und zukünfte Kommunikatoins-, Positionierungs- sowie Erdbeobachtungsmissionen ist. Die Beiträge dieser Arbeit stellen gleich mehrere "Premieren" in der EPD-Forschung dar: (1.) Der erste empirische Nachweis interhemisphärischer elektromagnetischer Energieflüsse und feldgerichteter Ströme. (2.) Die erste raum-zeitliche Beschreibung von EPDs auf der Grundlage ihrer assoziierten feldgerichteten und diamagnetischen Ströme. (3.) Der erste Nachweis hohen Plasmadrucks in Regionen verminderter Plasmadichte in der Ionosphäre. Diese Forschungsergebnisse liefern neue Erkenntnisse, die nicht nur unser derzeitiges Wissen über EPDs, sondern auch jenes über die ionosphärische Domaine in niedrigen Breiten nach Sonnenuntergang fördert. KW - equatorial plasma depletions KW - electric and magnetic fields KW - spread F KW - ionosphere KW - swarm mission KW - äquatorialen Plasma-Verarmungen KW - elektrische und magnetische Felder KW - Spread F KW - Ionosphäre KW - Satellitenmission Swarm Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-445873 ER -