@phdthesis{Lefebvre2019,
  author    = {Lefebvre, Marie G.},
  title     = {Two stages of skarn formation - two tin enrichments},
  doi       = {10.25932/publishup-42717},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-427178},
  school      = {Universit{\"a}t Potsdam},
  pages     = {87},
  year      = {2019},
  abstract  = {Skarn deposits are found on every continents and were formed at different times from Precambrian to Tertiary. Typically, the formation of a skarn is induced by a granitic intrusion in carbonates-rich sedimentary rocks. During contact metamorphism, fluids derived from the granite interact with the sedimentary host rocks, which results in the formation of calc-silicate minerals at the expense of carbonates. Those newly formed minerals generally develop in a metamorphic zoned aureole with garnet in the proximal and pyroxene in the distal zone. Ore elements contained in magmatic fluids are precipitated due to the change in fluid composition. The temperature decrease of the entire system, due to the cooling of magmatic fluids and the entering of meteoric water, allows retrogression of some prograde minerals. The H{\"a}mmerlein skarn deposit has a multi-stage history with a skarn formation during regional metamorphism and a retrogression of primary skarn minerals during the granitic intrusion. Tin was mobilized during both events. The 340 Ma old tin-bearing skarn minerals show that tin was present in sediments before the granite intrusion, and that the first Sn enrichment occurred during the skarn formation by regional metamorphism fluids. In a second step at ca. 320 Ma, tin-bearing fluids were produced with the intrusion of the Eibenstock granite. Tin, which has been added by the granite and remobilized from skarn calc-silicates, precipitated as cassiterite. Compared to clay or marl, the skarn is enriched in Sn, W, In, Zn, and Cu. These metals have been supplied during both regional metamorphism and granite emplacement. In addition, the several isotopic and chemical data of skarn samples show that the granite selectively added elements such as Sn, and that there was no visible granitic contribution to the sedimentary signature of the skarn The example of H{\"a}mmerlein shows that it is possible to form a tin-rich skarn without associated granite when tin has already been transported from tin-bearing sediments during regional metamorphism by aqueous metamorphic fluids. These skarns are economically not interesting if tin is only contained in the skarn minerals. Later alteration of the skarn (the heat and fluid source is not necessarily a granite), however, can lead to the formation of secondary cassiterite (SnO2), with which the skarn can become economically highly interesting.},
  language  = {en}
}
@phdthesis{Olivotos2023,
  author    = {Olivotos, Spyros-Christos},
  title     = {Reconstructing the Landscape Evolution of South Central Africa by Surface Exposure Dating of Waterfalls},
  doi       = {10.25932/publishup-60169},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-601699},
  school      = {Universit{\"a}t Potsdam},
  pages     = {159},
  year      = {2023},
  abstract  = {The East African Rift System (EARS) is a significant example of active tectonics, which provides opportunities to examine the stages of continental faulting and landscape evolution. The southwest extension of the EARS is one of the most significant examples of active tectonics nowadays, however, seismotectonic research in the area has been scarce, despite the fundamental importance of neotectonics. Our first study area is located between the Northern Province of Zambia and the southeastern Katanga Province of the Democratic Republic of Congo. Lakes Mweru and Mweru Wantipa are part of the southwest extension of the EARS. Fault analysis reveals that, since the Miocene, movements along the active Mweru-Mweru Wantipa Fault System (MMFS) have been largely responsible for the reorganization of the landscape and the drainage patterns across the southwestern branch of the EARS. To investigate the spatial and temporal patterns of fluvial-lacustrine landscape development, we determined in-situ cosmogenic 10Be and 26Al in a total of twenty-six quartzitic bedrock samples that were collected from knickpoints across the Mporokoso Plateau (south of Lake Mweru) and the eastern part of the Kundelungu Plateau (north of Lake Mweru). Samples from the Mporokoso Plateau and close to the MMFS provide evidence of temporary burial. By contrast, surfaces located far from the MMFS appear to have remained uncovered since their initial exposure as they show consistent 10Be and 26Al exposure ages ranging up to ~830 ka. Reconciliation of the observed burial patterns with morphotectonic and stratigraphic analysis reveals the existence of an extensive paleo-lake during the Pleistocene. Through hypsometric analyses of the dated knickpoints, the potential maximum water level of the paleo-lake is constrained to ~1200 m asl (present lake lavel: 917 m asl). High denudation rates (up to ~40 mm ka-1) along the eastern Kundelungu Plateau suggest that footwall uplift, resulting from normal faulting, caused river incision, possibly controlling paleo-lake drainage. The lake level was reduced gradually reaching its current level at ~350 ka. Parallel to the MMFS in the north, the Upemba Fault System (UFS) extends across the southeastern Katanga Province of the Democratic Republic of Congo. This part of our research is focused on the geomorphological behavior of the Kiubo Waterfalls. The waterfalls are the currently active knickpoint of the Lufira River, which flows into the Upemba Depression. Eleven bedrock samples along the Lufira River and its tributary stream, Luvilombo River, were collected. In-situ cosmogenic 10Be and 26Al were used in order to constrain the K constant of the Stream Power Law equation. Constraining the K constant allowed us to calculate the knickpoint retreat rate of the Kiubo Waterfalls at ~0.096 m a-1. Combining the calculated retreat rate of the knickpoint with DNA sequencing from fish populations, we managed to present extrapolation models and estimate the location of the onset of the Kiubo Waterfalls, revealing its connection to the seismicity of the UFS.},
  language  = {en}
}
@phdthesis{Rembe2023,
  author    = {Rembe, Johannes},
  title     = {Hercynian to Eocimmerian evolution of the North Pamir in Central Asia},
  doi       = {10.25932/publishup-59751},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-597510},
  school      = {Universit{\"a}t Potsdam},
  pages     = {xxvi, 154, CX},
  year      = {2023},
  abstract  = {The North Pamir, part of the India-Asia collision zone, essentially formed during the late Paleozoic to late Triassic-early Jurassic. Coeval to the subduction of the Turkestan ocean—during the Carboniferous Hercynian orogeny in the Tien Shan—a portion of the Paleo-Tethys ocean subducted northward and lead to the formation and obduction of a volcanic arc. This Carboniferous North Pamir arc is of Andean style in the western Darvaz segment and trends towards an intraoceanic arc in the eastern, Oytag segment. A suite of arc-volcanic rocks and intercalated, marine sediments together with intruded voluminous plagiogranites (trondhjemite and tonalite) and granodiorites was uplifted and eroded during the Permian, as demonstrated by widespread sedimentary unconformities. Today it constitutes a major portion of the North Pamir. In this work, the first comprehensive Uranium-Lead (U-Pb) laser-ablation inductively-coupled-plasma mass-spectrometry (LA-ICP-MS) radiometric age data are presented along with geochemical data from the volcanic and plutonic rocks of the North Pamir volcanic arc. Zircon U-Pb data indicate a major intrusive phase between 340 and 320 Ma. The magmatic rocks show an arc-signature, with more primitive signatures in the Oytag segment compared to the Darvaz segment. Volcanic rocks in the Chinese North Pamir were indirectly dated by determining the age of ocean floor alteration. We investigate calcite filled vesicles and show that oxidative sea water and the basaltic host rock are major trace element sources. The age of ocean floor alteration, within a range of 25 Ma, constrains the extrusion age of the volcanic rocks. In the Chinese Pamir, arc-volcanic basalts have been dated to the Visean-Serpukhovian boundary. This relates the North Pamir volcanic arc to coeval units in the Tien Shan. Our findings further question the idea of a continuous Tarim-Tajik continent in the Paleozoic. From the Permian (Guadalupian) on, a progressive sea-retreat led to continental conditions in the northeastern Pamir. Large parts of Central Asia were affected by transcurrent tectonics, while subduction of the Paleo-Tethys went on south of the accreted North Pamir arc, likely forming an accretionary wedge, representing an early stage of the later Karakul-Mazar tectonic unit. Graben systems dissected the Permian carbonate platforms, that formed on top of the uplifted Carboniferous arc in the central and western North Pamir. A continental graben formed in the eastern North Pamir. Zircon U-Pb dating suggest initiation of volcanic activity at ~260 Ma. Extensional tectonics prevailed throughout the Triassic, forming the Hindukush-North Pamir rift system. New geochemistry and zircon U-Pb data tie volcanic rocks, found in the Chinese Pamir, to coeval arc-related plutonic rocks found within the Karakul-Mazar arc-accretionary complex. The sedimentary environment in the continental North Pamir rift evolved from an alluvial plain, lake dominated environment in the Guadalupian to a coarser-clastic, alluvial, braided river dominated in the Triassic. Volcanic activity terminated in the early Jurassic. We conducted Potassium-Argon (K-Ar) fine-fraction dating on the Shala Tala thrust fault, a major structure juxtaposing Paleozoic marine units of lower greenschist to amphibolite facies conditions against continental Permian deposits. Fault slip under epizonal conditions is dated to 204.8 ± 3.7 Ma (2σ), implying Rhaetian nappe emplacement. This pinpoints the Central-North Pamir collision, since the Shala Tala thrust was a back-thrust at that time.},
  language  = {en}
}
@phdthesis{Warkus2002,
  author    = {Warkus, Frank},
  title     = {Die neogene Hebungsgeschichte der Patagonischen Anden im Kontext der Subduktion eines aktiven Spreizungszentrums},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-0000555},
  school      = {Universit{\"a}t Potsdam},
  year      = {2002},
  abstract  = {Das Ph{\"a}nomen der Subduktion eines aktiven Spreizungszentrums an der S{\"u}dspitze S{\"u}damerikas ist seit langem bekannt. Eine Vielzahl von geologischen Beobachtungen wurden mit diesem Ph{\"a}nomen in Verbindung gebracht, trotzdem ist der genaue Mechanismus der Beeinflussung des aktiven Kontinentalrandes weitgehend unbekannt. Die Zusammenh{\"a}nge zwischen den Subduktionsprozessen und der Entwicklung der patagonischen Anden zwischen 47\&\#176;S und 48\&\#176;S stehen im Mittelpunkt der Untersuchungen. Um eine detaillierte zeitliche Aufl{\"o}sung der zugrunde liegenden Prozesse untersuchen zu k{\"o}nnen, wurde die Entwicklung der Vorlandsedimentation, die thermische Entwicklung und die Heraushebung der Oberkruste des andinen Orogens untersucht und diese in Bezug zur Subduktion des Chile-R{\"u}ckens gesetzt. Im Bereich von 47\&\#176;30\′S wurden die synorogenen Vorlandsedimente der Santa Cruz Formation sedimentologisch untersucht. Diese fluviatilen Sedimente wurden in einem reliefarmen Vorlandgebiet durch h{\"a}ufige Rinnenverlagerung und dem Aufbau von Rinnenumlagerungsg{\"u}rteln in Kombination mit assoziierten großr{\"a}umigen {\"U}berflutungsablagerungen akkumuliert. Sie stehen in einem engen Zusammenhang mit der orogenen Entwicklung im andinen Liefergebiet. Dies spiegelt sich in dem nach oben gr{\"o}ber werdenden Zyklus der Santa Cruz Formation wider. Die magnetostratigraphischen Untersuchungen einer 270 m m{\"a}chtigen Sequenz aus der Basis der Santa Cruz Formation, die mit 329 Einzelproben aus 96 Probenpunkten beprobt wurde, ergab 7 Umkehrungen der geomagnetischen Feldrichtung. Mit Hilfe der geomagnetischen Polarit{\"a}tszeitskala (CANDE AND KENT, 1995) konnte der untersuchte Abschnitt der Santa Cruz Formation zwischen 16.2 und 18.5 Ma datiert werden. Als Tr{\"a}ger der Sedimentations-Remanenz konnten {\"u}berwiegend Pseudoeinbereichs-Magentitpartikel und untergeordnet H{\"a}matitpartikel identifiziert werden. An drei Profilen der Santa Cruz Formation wurden aus Sandsteinlagen unterschiedlicher stratigraphischer Position detritische Apatite mit Hilfe der thermochronologischen Spaltspurmethode untersucht. Die thermisch nicht r{\"u}ckgesetzten, detritischen Apatite spiegeln das Auftreten unterschiedlicher Altersdom{\"a}nen im Liefergebiet der Sedimente wider. In der Kombination mit den geochemischen Gesamtgesteinsuntersuchungen der Sedimente und den petrographischen Untersuchungen der Sandsteine, die ein {\"u}berwiegend andesitisch-vulkanisch gepr{\"a}gtes Liefergebiet widerspiegeln, kann nachgewiesen werden, dass die Erosion im Liefergebiet um 16.5 Ma in tiefere, deformierte Krustensegmente einschneidet. Dies bedeutet, dass aufgrund der Denudation im andinen Orogen erste Sockelgesteinseinheiten in den Bereich der Abtragung gelangen und dass dieser Eintrag um 12 bis 10 Ma ein Volumen einnimmt, das zu signifikanten {\"A}nderungen der Gesamtgesteinsgeochemie der Vorlandsedimente f{\"u}hrt. Die thermochronologische Untersuchung von Apatiten aus rezenten topographischen H{\"o}henprofilen aus der Kernzone der patagonischen Anden im Bereich von 47\&\#176;30\′S zeigen den Beginn einer beschleunigten Heraushebung des Orogens um 7.5 Ma. Aus diesen Untersuchungen kann eine Denudationsrate im Zeitraum der letzen 7 bis 8 Ma von 600 bis 650 m/Ma abgesch{\"a}tzt werden. Die Modellierung der Apatit-Spaltspurergebnisse zeigt eine signifikante Temperaturerh{\"o}hung im Zeitraum zwischen 12 und 8 Ma um 20 bis 30\&\#176;C f{\"u}r diesen Krustenbereich, die mit der Subduktion des aktiven Chile-R{\"u}ckens in diesem Bereich der Anden in Verbindung gebracht wird. Aus den gewonnen Daten kann ein Modell f{\"u}r die Entwicklung der patagonischen Anden seit dem fr{\"u}hen Mioz{\"a}n abgeleitet werden. In diesem Modell wird die orogene Entwicklung in den patagonischen Anden auf eine erh{\"o}hte Konvergenzrate zwischen der Nazca Platte und der S{\"u}damerikanischen Platte zur{\"u}ckgef{\"u}hrt, die f{\"u}r die Heraushebung und Denudation der Anden sowie f{\"u}r die damit verbundene Entwicklung im Vorlandbereich verantwortlich ist. Diese orogene Entwicklung wird in einer sp{\"a}ten Phase durch die nordw{\"a}rts wandernde Subduktion des aktiven Spreizungszentrums des Chile R{\"u}ckens {\"u}berpr{\"a}gt und beeinflusst. Das auf der Integration von geologischen, chronologischen sowie thermochronologischen Daten beruhende Modell kann zahlreiche geologische und geophysikalische Beobachtungen in diesem Bereich der s{\"u}dlichen Anden konsistent erkl{\"a}ren.},
  subject      = {Patagonien ; Neogen ; Hebung ; Subduktion ; Anden},
  language  = {de}
}