@phdthesis{Neuharth2022,
  author    = {Neuharth, Derek},
  title     = {Evolution of divergent and strike-slip boundaries in response to surface processes},
  doi       = {10.25932/publishup-54940},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-549403},
  school      = {Universit{\"a}t Potsdam},
  pages     = {xiii, 108},
  year      = {2022},
  abstract  = {Plate tectonics describes the movement of rigid plates at the surface of the Earth as well as their complex deformation at three types of plate boundaries: 1) divergent boundaries such as rift zones and mid-ocean ridges, 2) strike-slip boundaries where plates grind past each other, such as the San Andreas Fault, and 3) convergent boundaries that form large mountain ranges like the Andes. The generally narrow deformation zones that bound the plates exhibit complex strain patterns that evolve through time. During this evolution, plate boundary deformation is driven by tectonic forces arising from Earth's deep interior and from within the lithosphere, but also by surface processes, which erode topographic highs and deposit the resulting sediment into regions of low elevation. Through the combination of these factors, the surface of the Earth evolves in a highly dynamic way with several feedback mechanisms. At divergent boundaries, for example, tensional stresses thin the lithosphere, forcing uplift and subsequent erosion of rift flanks, which creates a sediment source. Meanwhile, the rift center subsides and becomes a topographic low where sediments accumulate. This mass transfer from foot- to hanging wall plays an important role during rifting, as it prolongs the activity of individual normal faults. When rifting continues, continents are eventually split apart, exhuming Earth's mantle and creating new oceanic crust. Because of the complex interplay between deep tectonic forces that shape plate boundaries and mass redistribution at the Earth's surface, it is vital to understand feedbacks between the two domains and how they shape our planet. In this study I aim to provide insight on two primary questions: 1) How do divergent and strike-slip plate boundaries evolve? 2) How is this evolution, on a large temporal scale and a smaller structural scale, affected by the alteration of the surface through erosion and deposition? This is done in three chapters that examine the evolution of divergent and strike-slip plate boundaries using numerical models. Chapter 2 takes a detailed look at the evolution of rift systems using two-dimensional models. Specifically, I extract faults from a range of rift models and correlate them through time to examine how fault networks evolve in space and time. By implementing a two-way coupling between the geodynamic code ASPECT and landscape evolution code FastScape, I investigate how the fault network and rift evolution are influenced by the system's erosional efficiency, which represents many factors like lithology or climate. In Chapter 3, I examine rift evolution from a three-dimensional perspective. In this chapter I study linkage modes for offset rifts to determine when fast-rotating plate-boundary structures known as continental microplates form. Chapter 4 uses the two-way numerical coupling between tectonics and landscape evolution to investigate how a strike-slip boundary responds to large sediment loads, and whether this is sufficient to form an entirely new type of flexural strike-slip basin.},
  language  = {en}
}
@phdthesis{Riedl2021,
  author    = {Riedl, Simon},
  title     = {Active tectonics in the Kenya Rift},
  doi       = {10.25932/publishup-53855},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-538552},
  school      = {Universit{\"a}t Potsdam},
  pages     = {xi, 207},
  year      = {2021},
  abstract  = {Magmatische und tektonisch aktive Grabenzonen (Rifts) stellen die Vorstufen entstehender Plattengrenzen dar. Diese sich spreizenden tektonischen Provinzen zeichnen sich durch allgegenw{\"a}rtige Abschiebungen aus, und die r{\"a}umliche Verteilung, die Geometrie, und das Alter dieser Abschiebungen l{\"a}sst R{\"u}ckschl{\"u}sse auf die r{\"a}umlichen und zeitlichen Zusammenh{\"a}nge zwischen tektonischer Deformation, Magmatismus und langwelliger Krustendeformation in Rifts zu. Diese Arbeit konzentriert sich auf die St{\"o}rungsaktivit{\"a}t im Kenia-Rift des k{\"a}nozoischen Ostafrikanischen Grabensystems im Zeitraum zwischen dem mittleren Pleistoz{\"a}n und dem Holoz{\"a}n. Um die fr{\"u}hen Stadien der Entstehung kontinentaler Plattengrenzen zu untersuchen, wird in dieser Arbeit eine zeitlich gemittelte minimale Extensionsrate f{\"u}r den inneren Graben des N{\"o}rdlichen Kenia-Rifts (NKR) f{\"u}r die letzten 0,5 Mio Jahre abgeleitet. Die Analyse beruht auf Messungen mit Hilfe des digitalen TanDEM-X-H{\"o}henmodells, um die Abschiebungen entlang der vulkanisch-tektonischen Achse des inneren Grabens des NKR zu kartieren und deren Versatzbetr{\"a}ge zu bestimmen. Mithilfe von vorhandenen Geochronologiedaten der deformierten vulkanischen Einheiten sowie in dieser Arbeit erstellten ⁴⁰Ar/³⁹Ar-Datierungen werden zeitlich gemittelte Extensionsraten berechnet. Die Auswertungen zeigen, dass im inneren Graben des NKR die langfristige Extensionsrate f{\"u}r mittelpleistoz{\"a}ne bis rezente St{\"o}rungen Mindestwerte von 1,0 bis 1,6 mm yr⁻¹ aufweist und lokal allerdings auch Werte bis zu 2,0 mm yr⁻¹ existieren. In Anbetracht der nahezu inaktiven Randst{\"o}rungen des NKR zeigt sich somit, dass sich die Extension auf die Region der aktiven vulkanisch-tektonischen Achse im inneren Graben konzentriert und somit ein fortgeschrittenes Stadium kontinentaler Extensionsprozesse im NKR vorliegt. In dieser Arbeit wird diese r{\"a}umlich fokussierte Extension zudem im Rahmen einer St{\"o}rungsanalyse der j{\"u}ngsten vulkanischen Erscheinungen des Kenia-Rifts betrachtet. Die Arbeit analysiert mithilfe von Gel{\"a}ndekartierungen und eines auf Luftbildern basierenden Gel{\"a}ndemodells die St{\"o}rungscharakteristika der etwa 36 tausend Jahre alten Menengai-Kaldera und der umliegenden Gebiete im zentralen Kenia-Rift. Im Allgemeinen sind die holoz{\"a}nen St{\"o}rungen innerhalb des Rifts reine, NNO-streichende Abschiebungen, die somit das gegenw{\"a}rtige tektonische Spannungsfeld wiederspiegeln; innerhalb der Menengai-Kaldera sind die jungen Strukturen jedoch von andauernder magmatischer Aktivit{\"a}t und von Aufdomung {\"u}berpr{\"a}gt. Die Kaldera befindet sich im Zentrum eines sich aktiv dehnenden Riftsegments und zusammen mit den anderen quart{\"a}ren Vulkanen des Kenia-Rifts lassen sich diese Bereiche als Kernpunkte der extensionalen St{\"o}rungsaktivit{\"a}t verstehen, die letztlich zu einer weiter entwickelten Phase magmengest{\"u}tzter Kontinentalseparation f{\"u}hren werden. Die bereits seit dem Terti{\"a}r andauernde St{\"o}rungsaktivit{\"a}t im Kenia-Rift f{\"u}hrt zur Zergliederung der gr{\"o}ßeren Rift-Senken in kleinere Segmente und beeinflusst die Sedimentologie und die Hydrologie dieser Riftbecken. Gegenw{\"a}rtig sind die meisten, durch St{\"o}rungen begrenzten Becken des Kenia-Rifts hydrologisch isoliert, sie waren aber w{\"a}hrend feuchter Klimaphasen hydrologisch miteinander verbunden; in dieser Arbeit untersuche ich deshalb auch diese hydrologische Verbindung der Rift-Becken f{\"u}r die Zeit der Afrikanischen Feuchteperiode des fr{\"u}hen Holoz{\"a}ns. Mithilfe der Analyse von digitalen Gel{\"a}ndemodellen, unter Ber{\"u}cksichtigung von geomorphologischen Anzeigern f{\"u}r Seespiegelhochst{\"a}nde, Radiokarbondatierungen und einer {\"U}bersicht {\"u}ber Fossiliendaten konnten zwei kaskadierende Flusssysteme aus diesen Daten abgeleitet werden: eine Flusskaskade in Richtung S{\"u}den und eine in Richtung Norden. Beide Kaskaden haben die derzeit isolierten Becken w{\"a}hrend des fr{\"u}hen Holoz{\"a}ns durch {\"u}berlaufende Seen und eingeschnittene Schluchten miteinander verbunden. Diese hydrologische Verbindung f{\"u}hrte zu der Ausbreitung aquatischer Fauna entlang des Rifts, und gleichzeitig stellte die Wasserscheide zwischen den beiden Flusssystemen den einzigen terrestrischen Ausbreitungskorridor dar, der eine {\"U}berquerung des Kenia-Rifts erm{\"o}glichte. Diese tektonisch-geomorphologische Rekonstruktion erkl{\"a}rt die heute isolierten Vorkommen nilotischer Fischarten in den Riftseen Kenias sowie die isolierten Vorkommen Guineo-Congolischer S{\"a}ugetiere in W{\"a}ldern {\"o}stlich des Kenia-Rifts, die sich {\"u}ber die Wasserscheide im Kenia-Rift ausbreiten konnten. Auf l{\"a}ngeren Zeitskalen sind solche Phasen hydrologischer Verbindung und Phasen der Isolation wiederholt aufgetreten und zeigen sich in wechselnden pal{\"a}o{\"o}kologischen Indikatoren in Sedimentbohrkernen. Hier stelle ich einen Sedimentbohrkern aus dem Koora-Becken des S{\"u}dlichen Kenia-Rifts vor, der einen Datensatz der Pal{\"a}o-Umweltbedingungen der letzten 1 Million Jahre beinhaltet. Dieser Datensatz zeigt, dass etwa vor 400 tausend Jahren die zuvor relativ stabilen Umweltbedingungen zum Erliegen kamen und tektonische, hydrologische und {\"o}kologische Ver{\"a}nderungen dazu f{\"u}hrten, dass die Wasserverf{\"u}gbarkeit, die Grasland-Vergesellschaftungen und die Bedeckung durch Baumvegetation zunehmend st{\"a}rkeren und h{\"a}ufigeren Schwankungen unterlagen. Diese großen Ver{\"a}nderungen fallen zeitlich mit Phasen zusammen, in denen das s{\"u}dliche Becken des Kenia-Rifts von vulkanischer und tektonischer Aktivit{\"a}t besonders betroffen war. Die vorliegende Arbeit zeigt deshalb deutlich, inwiefern die tektonischen und geomorphologischen Gegebenheiten im Zuge einer zeitlich langanhaltenden Extension die Hydrologie, die Pal{\"a}o-Umweltbedingungen sowie die Biodiversit{\"a}t einer Riftzone beeinflussen k{\"o}nnen.},
  language  = {en}
}
@phdthesis{Zeckra2020,
  author    = {Zeckra, Martin},
  title     = {Seismological and seismotectonic analysis of the northwestern Argentine Central Andean foreland},
  doi       = {10.25932/publishup-47324},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-473240},
  school      = {Universit{\"a}t Potsdam},
  pages     = {vii, 120},
  year      = {2020},
  abstract  = {After a severe M W 5.7 earthquake on October 17, 2015 in El Galp{\´o}n in the province of Salta NW Argentina, I installed a local seismological network around the estimated epicenter. The network covered an area characterized by inherited Cretaceous normal faults and neotectonic faults with unknown recurrence intervals, some of which may have been reactivated normal faults. The 13 three-component seismic stations recorded data continuously for 15 months. The 2015 earthquake took place in the Santa B{\´a}rbara System of the Andean foreland, at about 17km depth. This region is the easternmost morphostructural region of the central Andes. As a part of the broken foreland, it is bounded to the north by the Subandes fold-and-thrust belt and the Sierras Pampeanas to the south; to the east lies the Chaco-Paran{\´a} basin. A multi-stage morphotectonic evolution with thick-skinned basement uplift and coeval thin-skinned deformation in the intermontane basins is suggested for the study area. The release of stresses associated with the foreland deformation can result in strong earthquakes, as the study area is known for recurrent and historical, destructive earthquakes. The available continuous record reaches back in time, when the strongest event in 1692 (magnitude 7 or intensity IX) destroyed the city of Esteco. Destructive earthquakes and surface deformation are thus a hallmark of this part of the Andean foreland. With state-of-the-art Python packages (e.g. pyrocko, ObsPy), a semi-automatic approach is followed to analyze the collected continuous data of the seismological network. The resulting 1435 hypocenter locations consist of three different groups: 1.) local crustal earthquakes (nearly half of the events belong to this group), 2.) interplate activity, of regional distance in the slab of the Nazca-plate, and 3.) very deep earthquakes at about 600km depth. My major interest focused on the first event class. Those crustal events are partly aftershock events of the El Galp{\´o}n earthquake and a second earthquake, in the south of the same fault. Further events can be considered as background seismicity of other faults within the study area. Strikingly, the seismogenic zone encompass the whole crust and propagates brittle deformation down, close to the Moho. From the collected seismological data, a local seismic velocity model is estimated, using VELEST. After the execution of various stability tests, the robust minimum 1D-velocity model implies guiding values for the composition of the local, subsurface structure of the crust. Afterwards, performing a hypocenter relocation enables the assignment of individual earthquakes to aftershock clusters or extended seismotectonic structures. This allows the mapping of previously unknown seismogenic faults. Finally, focal mechanisms are modeled for events with acurately located hypocenters, using the newly derived local velocity model. A compressive regime is attested by the majority of focal mechanisms, while the strike direction of the individual seismogenic structures is in agreement with the overall north - south orientation of the Central Andes, its mountain front, and individual mountain ranges in the southern Santa-B{\´a}rbara-System.},
  language  = {en}
}
@phdthesis{Smirnov2023,
  author    = {Smirnov, Artem},
  title     = {Understanding the dynamics of the near-earth space environment utilizing long-term satellite observations},
  doi       = {10.25932/publishup-61371},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-613711},
  school      = {Universit{\"a}t Potsdam},
  pages     = {xxxvi, 286},
  year      = {2023},
  abstract  = {The near-Earth space environment is a highly complex system comprised of several regions and particle populations hazardous to satellite operations. The trapped particles in the radiation belts and ring current can cause significant damage to satellites during space weather events, due to deep dielectric and surface charging. Closer to Earth is another important region, the ionosphere, which delays the propagation of radio signals and can adversely affect navigation and positioning. In response to fluctuations in solar and geomagnetic activity, both the inner-magnetospheric and ionospheric populations can undergo drastic and sudden changes within minutes to hours, which creates a challenge for predicting their behavior. Given the increasing reliance of our society on satellite technology, improving our understanding and modeling of these populations is a matter of paramount importance. In recent years, numerous spacecraft have been launched to study the dynamics of particle populations in the near-Earth space, transforming it into a data-rich environment. To extract valuable insights from the abundance of available observations, it is crucial to employ advanced modeling techniques, and machine learning methods are among the most powerful approaches available. This dissertation employs long-term satellite observations to analyze the processes that drive particle dynamics, and builds interdisciplinary links between space physics and machine learning by developing new state-of-the-art models of the inner-magnetospheric and ionospheric particle dynamics. The first aim of this thesis is to investigate the behavior of electrons in Earth's radiation belts and ring current. Using ~18 years of electron flux observations from the Global Positioning System (GPS), we developed the first machine learning model of hundreds-of-keV electron flux at Medium Earth Orbit (MEO) that is driven solely by solar wind and geomagnetic indices and does not require auxiliary flux measurements as inputs. We then proceeded to analyze the directional distributions of electrons, and for the first time, used Fourier sine series to fit electron pitch angle distributions (PADs) in Earth's inner magnetosphere. We performed a superposed epoch analysis of 129 geomagnetic storms during the Van Allen Probes era and demonstrated that electron PADs have a strong energy-dependent response to geomagnetic activity. Additionally, we showed that the solar wind dynamic pressure could be used as a good predictor of the PAD dynamics. Using the observed dependencies, we created the first PAD model with a continuous dependence on L, magnetic local time (MLT) and activity, and developed two techniques to reconstruct near-equatorial electron flux observations from low-PA data using this model. The second objective of this thesis is to develop a novel model of the topside ionosphere. To achieve this goal, we collected observations from five of the most widely used ionospheric missions and intercalibrated these data sets. This allowed us to use these data jointly for model development, validation, and comparison with other existing empirical models. We demonstrated, for the first time, that ion density observations by Swarm Langmuir Probes exhibit overestimation (up to ~40-50\%) at low and mid-latitudes on the night side, and suggested that the influence of light ions could be a potential cause of this overestimation. To develop the topside model, we used 19 years of radio occultation (RO) electron density profiles, which were fitted with a Chapman function with a linear dependence of scale height on altitude. This approximation yields 4 parameters, namely the peak density and height of the F2-layer and the slope and intercept of the linear scale height trend, which were modeled using feedforward neural networks (NNs). The model was extensively validated against both RO and in-situ observations and was found to outperform the International Reference Ionosphere (IRI) model by up to an order of magnitude. Our analysis showed that the most substantial deviations of the IRI model from the data occur at altitudes of 100-200 km above the F2-layer peak. The developed NN-based ionospheric model reproduces the effects of various physical mechanisms observed in the topside ionosphere and provides highly accurate electron density predictions. This dissertation provides an extensive study of geospace dynamics, and the main results of this work contribute to the improvement of models of plasma populations in the near-Earth space environment.},
  language  = {en}
}