TY - THES A1 - Senftleben, Robin T1 - Earth's magnetic field over the last 1000 years N2 - To investigate the reliability and stability of spherical harmonic models based on archeo/-paleomagnetic data, 2000 Geomagnetic models were calculated. All models are based on the same data set but with randomized uncertainties. Comparison of these models to the geomagnetic field model gufm1 showed that large scale magnetic field structures up to spherical harmonic degree 4 are stable throughout all models. Through a ranking of all models by comparing the dipole coefficients to gufm1 more realistic uncertainty estimates were derived than the authors of the data provide. The derived uncertainty estimates were used in further modelling, which combines archeo/-paleomagnetic and historical data. The huge difference in data count, accuracy and coverage of these two very different data sources made it necessary to introduce a time dependent spatial damping, which was constructed to constrain the spatial complexity of the model. Finally 501 models were calculated by considering that each data point is a Gaussian random variable, whose mean is the original value and whose standard deviation is its uncertainty. The final model arhimag1k is calculated by taking the mean of the 501 sets of Gauss coefficients. arhimag1k fits different dependent and independent data sets well. It shows an early reverse flux patch at the core-mantle boundary between 1000 AD and 1200 AD at the location of the South Atlantic Anomaly today. Another interesting feature is a high latitude flux patch over Greenland between 1200 and 1400 AD. The dipole moment shows a constant behaviour between 1600 and 1840 AD. In the second part of the thesis 4 new paleointensities from 4 different flows of the island Fogo, which is part of Cape Verde, are presented. The data is fitted well by arhimag1k with the exception of the value at 1663 of 28.3 microtesla, which is approximately 10 microtesla lower than the model suggest. N2 - Um die Stabilität und Zuverlässigkeit von sphärisch harmonischen Erdmagnetfeldmodellen, die auf paleomagnetischen und archeomagnetischen Daten basieren zu untersuchen wurden 2000 Erdmagnetfeldmodelle berechnet. Jedes dieser Modelle berechnet sich aus Daten, die mit zufälligen Unsicherheiten in die Inversion eingehen. Ein Vergleich dieser Modelle zum historischen Erdmagnetfeldmodell gufm1 zeigt, dass großflächige magnetische Strukturen bis zum sphärischen harmonischen Grad 4 stabil in allen Modellen sind. Ein Ranking der 2000 Modelle wurde verwendet, um realistischere Fehlerabschätzungen der Daten zu bekommen, als die, die von den Autoren angebeben werden. Diese Fehlerabschätzungen werden für die weitere Modellierung benutzt, welche historische und paleo-/archeomagnetiche Daten kombiniert. Der große Unterschied in der Anzahl der Daten und der räumlichen Verteilung dieser sehr verschiedenen Datenquellen machte es notwendig, eine zeitabhängige räumliche Dämpfung einzuführen. Diese ist so konstruiert, dass die räumlich Komplexität des Modelles in einem bestimmten Zeitintervall festgelegt wird. 501 Modelle wurde berechnet, indem jeder Datenpunkt als gaußsche Zufallsvariable gesehen wird mit dem Originalwert als Mittelwert und die Fehlerabschätzung als Standardabweichung. Das finale Modell arhimag1k berechnet sich aus dem Mittelwert der Gaußkoeffizienten aller 501 Modelle. arhimag1k fittet verschiedene abhängige und unabhängige Datensätze gut. Es zeigt eine frühe Anomaly an der Kern-Mantel Grenze zwischen 1000 und 1200 AD an der Lokation, wo auch die heutige Südatlantische Anomaly liegt. Eine andere interessante Auffälligkeit ist eine starke radiale Magnetfeldkomponente an der Kern-Mantel Grenze zwischen 1200 und 1400 AD über Grönland. Das Dipolmoment zeigt ein konstantes Verhalten von 1600 bis 1840 AD. Im zweiten Teil der Arbeit werden 4 neue Paleointensitäten der Insel Fogo, welches Teil von Kap Verde ist, presentiert. Diese neuen Daten werden gut von dem Modell arhimag1k gefittet, außer der Wert von 1663 AD mit 28.3 mikrotesla , welcher etwa 10 mikrotesla niedriger ist, als das Modell zeigt. T2 - Erdmagnetfeld der letzten 1000 Jahre KW - Earth's magnetic field KW - archeomagnetism KW - paleomagnetism KW - modelling KW - spherical harmonics KW - Erdmagnetfeld KW - Archäomagnetismus KW - Paläomagnetismus KW - Modellierung KW - Kugelflächenfunktionen Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-473150 ER - TY - THES A1 - Liu, Jiabo T1 - Dynamics of the geomagnetic field during the last glacial T1 - Dynamik des geomagnetischen Feldes während der letzten Eiszeit N2 - Geomagnetic paleosecular variations (PSVs) are an expression of geodynamo processes inside the Earth’s liquid outer core. These paleomagnetic time series provide insights into the properties of the Earth’s magnetic field, from normal behavior with a dominating dipolar geometry, over field crises, such as pronounced intensity lows and geomagnetic excursions with a distorted field geometry, to the complete reversal of the dominating dipole contribution. Particularly, long-term high-resolution and high-quality PSV time series are needed for properly reconstructing the higher frequency components in the spectrum of geomagnetic field variations and for a better understanding of the effects of smoothing during the recording of such paleomagnetic records by sedimentary archives. In this doctorate study, full vector paleomagnetic records were derived from 16 sediment cores recovered from the southeastern Black Sea. Age models are based on radiocarbon dating and correlations of warming/cooling cycles monitored by high-resolution X-ray fluorescence (XRF) elementary ratios as well as ice-rafted debris (IRD) in Black Sea sediments to the sequence of ‘Dansgaard-Oeschger’ (DO) events defined from Greenland ice core oxygen isotope stratigraphy. In order to identify the carriers of magnetization in Black Sea sediments, core MSM33-55-1 recovered from the southeast Black Sea was subjected to detailed rock magnetic and electron microscopy investigations. The younger part of core MSM33-55-1 was continuously deposited since 41 ka. Before 17.5 ka, the magnetic minerals were dominated by a mixture of greigite (Fe3S4) and titanomagnetite (Fe3-xTixO4) in samples with SIRM/κLF >10 kAm-1, or exclusively by titanomagnetite in samples with SIRM/κLF ≤10 kAm-1. It was found that greigite is generally present as crustal aggregates in locally reducing micro-environments. From 17.5 ka to 8.3 ka, the dominant magnetic mineral in this transition phase was changing from greigite (17.5 – ~10.0 ka) to probably silicate-hosted titanomagnetite (~10.0 – 8.3 ka). After 8.3 ka, the anoxic Black Sea was a favorable environment for the formation of non-magnetic pyrite (FeS2) framboids. Aiming to avoid compromising of paleomagnetic data by erroneous directions carried by greigite, paleomagnetic data from samples with SIRM/κLF >10 kAm-1, shown to contain greigite by various methods, were removed from obtained records. Consequently, full vector paleomagnetic records, comprising directional data and relative paleointensity (rPI), were derived only from samples with SIRM/κLF ≤10 kAm-1 from 16 Black Sea sediment cores. The obtained data sets were used to create a stack covering the time window between 68.9 and 14.5 ka with temporal resolution between 40 and 100 years, depending on sedimentation rates. At 64.5 ka, according to obtained results from Black Sea sediments, the second deepest minimum in relative paleointensity during the past 69 ka occurred. The field minimum during MIS 4 is associated with large declination swings beginning about 3 ka before the minimum. While a swing to 50°E is associated with steep inclinations (50-60°) according to the coring site at 42°N, the subsequent declination swing to 30°W is associated with shallow inclinations of down to 40°. Nevertheless, these large deviations from the direction of a geocentric axial dipole field (I=61°, D=0°) still can not yet be termed as 'excursional', since latitudes of corresponding VGPs only reach down to 51.5°N (120°E) and 61.5°N (75°W), respectively. However, these VGP positions at opposite sides of the globe are linked with VGP drift rates of up to 0.2° per year in between. These extreme secular variations might be the mid-latitude expression of the Norwegian–Greenland Sea excursion found at several sites much further North in Arctic marine sediments between 69°N and 81°N. At about 34.5 ka, the Mono Lake excursion is evidenced in the stacked Black Sea PSV record by both a rPI minimum and directional shifts. Associated VGPs from stacked Black Sea data migrated from Alaska, via central Asia and the Tibetan Plateau, to Greenland, performing a clockwise loop. This agrees with data recorded in the Wilson Creek Formation, USA., and Arctic sediment core PS2644-5 from the Iceland Sea, suggesting a dominant dipole field. On the other hand, the Auckland lava flows, New Zealand, the Summer Lake, USA., and Arctic sediment core from ODP Site-919 yield distinct VGPs located in the central Pacific Ocean due to a presumably non-dipole (multi-pole) field configuration. A directional anomaly at 18.5 ka, associated with pronounced swings in inclination and declination, as well as a low in rPI, is probably contemporaneous with the Hilina Pali excursion, originally reported from Hawaiian lava flows. However, virtual geomagnetic poles (VGPs) calculated from Black Sea sediments are not located at latitudes lower than 60° N, which denotes normal, though pronounced secular variations. During the postulated Hilina Pali excursion, the VGPs calculated from Black Sea data migrated clockwise only along the coasts of the Arctic Ocean from NE Canada (20.0 ka), via Alaska (18.6 ka) and NE Siberia (18.0 ka) to Svalbard (17.0 ka), then looping clockwise through the Eastern Arctic Ocean. In addition to the Mono Lake and the Norwegian–Greenland Sea excursions, the Laschamp excursion was evidenced in the Black Sea PSV record with the lowest paleointensities at about 41.6 ka and a short-term (~500 years) full reversal centered at 41 ka. These excursions are further evidenced by an abnormal PSV index, though only the Laschamp and the Mono Lake excursions exhibit excursional VGP positions. The stacked Black Sea paleomagnetic record was also converted into one component parallel to the direction expected from a geocentric axial dipole (GAD) and two components perpendicular to it, representing only non-GAD components of the geomagnetic field. The Laschamp and the Norwegian–Greenland Sea excursions are characterized by extremely low GAD components, while the Mono Lake excursion is marked by large non-GAD contributions. Notably, negative values of the GAD component, indicating a fully reversed geomagnetic field, are observed only during the Laschamp excursion. In summary, this doctoral thesis reconstructed high-resolution and high-fidelity PSV records from SE Black Sea sediments. The obtained record comprises three geomagnetic excursions, the Norwegian–Greenland Sea excursion, the Laschamp excursion, and the Mono Lake excursion. They are characterized by abnormal secular variations of different amplitudes centered at about 64.5 ka, 41.0 ka and 34.5 ka, respectively. In addition, the obtained PSV record from the Black Sea do not provide evidence for the postulated 'Hilina Pali excursion' at about 18.5 ka. Anyway, the obtained Black Sea paleomagnetic record, covering field fluctuations from normal secular variations, over excursions, to a short but full reversal, points to a geomagnetic field characterized by a large dynamic range in intensity and a highly variable superposition of dipole and non-dipole contributions from the geodynamo during the past 68.9 to 14.5 ka. N2 - Die geomagnetischen Paläosäkularvarionen sind ein Ausdruck dynamischer Konvektionsprozesse im flüssigen äußeren Erdkern als Quelle des Erdmagnetfeldes, dem Geodynamo. Paläomagnetischen Zeitserien erlauben daher Rückschlüsse auf die veränderlichen Eigenschaften des Erdmagnetfeldes in Raum und Zeit, von stabilen Zuständen mit relativ hoher Feldstärke und dominierender Dipolgeometrie, bei der die magnetischen Pole nur in hohen Breiten migireren, über Feldkrisen wie Intensitätsminima und geomagnetischen Exkursionen mit komplexeren Geomentrien, bishin zur vollständigen und dauerhaften Umpolung des Dipolhauptfeldes. Eine geomagnetische Exkursion, als Extremfall der Paläosekularvariationen, ist charakterisiert durch kurzfristige (<104 Jahre) Abweichungen der paläomagnetischen Richtungen von der Richtung, die ein geozentrischer axialer Dipol produziert. Die aus paläognetisch bestimmten Richtungen abgeleiteten Positionen des virtuellen geomagnetischen (Nord-) Pols (VGP) liegen dabei per Definition südlich von 45°N. Für diese Doktoarbeit wurden sechzehn Sedimentkerne aus dem Schwarzen Meer herangezogen, um das Verhalten des Erdmagnetfeldes der letzten 70 ka zu untersuchen. Die dabei rekonstruierten Feldvariationen umfassen drei geomagnetische Exkursionen: die 'Norwegian-Greenland Sea excursion' (64.5 ka), die 'Laschamps excursion' (41.0 ka), sowie die 'Mono Lake excursion' (34.5 ka). Alle drei Ereignisse sind mit ausgeprägten Minima in der Feldintensität verbunden. Insbesondere während der 'Laschamps excursion', kam es zu einer kurzfristigen (0.5 ka) aber vollständigen Umpolung, während für die 'Mono Lake excursion' nur ein stark verzerrtes Dipolfeld anzunehmen ist. Die in der Literatur postulierte 'Hilina Pali excursion' (18.5 ka) konnte trotz in diesem Zeitraum zeitlich hochaufgelöster Datenreihen aus dem Schwarzen Meer nicht verifiziert werden. Für sie konnte, ähnlich wie für die 'Norwegian Greenland Sea excursion', lediglich stärker ausgeprägte, zum Teil zeitlich beschleunigte Änderungen in Inklination und Deklination der Magnetfeldrichtung nachgewiesen werden. KW - paleomagnetism KW - geomagnetic excursions KW - paleosecular variations KW - Black Sea KW - Paläomagnetik KW - geomagnetische Exkursionen KW - Paläosekularvariation KW - Schwarzes Meer Y1 - 2019 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-429461 ER - TY - JOUR A1 - Blayney, Tamsin A1 - Dupont-Nivet, Guillaume A1 - Najman, Yani A1 - Proust, Jean-Noel A1 - Meijer, Niels A1 - Roperch, Pierrick A1 - Sobel, Edward A1 - Millar, Ian A1 - Guo, Zhaojie T1 - Tectonic Evolution of the Pamir Recorded in the Western Tarim Basin (China) BT - Sedimentologic and Magnetostratigraphic Analyses of the Aertashi Section JF - Tectonics N2 - The northward indentation of the Pamir salient into the Tarim basin at the western syntaxis of the India-Asia collision zone is the focus of controversial models linking lithospheric to surface and atmospheric processes. Here we report on tectonic events recorded in the most complete and best-dated sedimentary sequences from the western Tarim basin flanking the eastern Pamir (the Aertashi section), based on sedimentologic, provenance, and magnetostratigraphic analyses. Increased tectonic subsidence and a shift from marine to continental fluvio-deltaic deposition at 41Ma indicate that far-field deformation from the south started to affect the Tarim region. A sediment accumulation hiatus from 24.3 to 21.6Ma followed by deposition of proximal conglomerates is linked to fault propagation into the Tarim basin. From 21.6 to 15.0Ma, increasing accumulation rates of fining upward clastics is interpreted as the expression of a major dextral transtensional system linking the Kunlun to the Tian Shan ahead of the northward Pamir indentation. At 15.0Ma, the appearance of North Pamir-sourced conglomerates followed at 11Ma by Central Pamir-sourced volcanics coincides with a shift to E-W compression, clockwise vertical-axis rotations and the onset of growth strata associated with the activation of the local east vergent Qimugen thrust wedge. Together, this enables us to interpret that Pamir indentation into Tarim had started by 24.3Ma, reached the study location by 15.0Ma and had passed it by 11Ma, providing kinematic constraints on proposed tectonic models involving intracontinental subduction and delamination. KW - India-Asia collision KW - Tarim basin KW - Pamir KW - Cenozoic KW - paleomagnetism KW - sedimentology Y1 - 2019 U6 - https://doi.org/10.1029/2018TC005146 SN - 0278-7407 SN - 1944-9194 VL - 38 IS - 2 SP - 492 EP - 515 PB - American Geophysical Union CY - Washington ER - TY - JOUR A1 - Zhang, Yang A1 - Huang, Wentao A1 - Huang, Baochun A1 - van Hinsbergen, Douwe J. J. A1 - Yang, Tao A1 - Dupont-Nivet, Guillaume A1 - Guo, Zhaojie T1 - 53-43Ma Deformation of Eastern Tibet Revealed by Three Stages of Tectonic Rotation in the Gongjue Basin JF - Journal of geophysical research : Solid earth N2 - The Gongjue basin from the eastern Qiangtang terrane is located in the transition region where the regional structural lineation curves from east-west-oriented in Tibet to north-south-oriented in Yunnan. In this study, we sampled the red beds in the basin from the lower Gongjue to upper Ranmugou formations for the first time covering the entire stratigraphic profile. The stratigraphic ages are bracketed within 53-43Ma by new detrital zircon U-Pb ages constraining the maximum deposition age to 52.51.5Ma. Rock magnetic and petrographic studies indicate that detrital magnetite and hematite are the magnetic carriers. Positive reversals and fold tests demonstrate that the characteristic remanent magnetization has a primary origin. The Gongjue and Ranmugou formations yield mean characteristic remanent magnetization directions of D-s/I-s=31.0 degrees/21.3 degrees and D-s/I-s=15.9 degrees/22.0 degrees, respectively. The magnetic inclination of these characteristic remanent magnetizations is significantly shallowed compared to the expected inclination for the locality. However, the elongation/inclination correction method does not provide a meaningful correction, likely because of syn-depositional rotation. Rotations relative to the Eurasian apparent polar wander path occurred in three stages: Stage I, 33.33.4 degrees clockwise rotation during the deposition of the Gongjue and lower Ranmugou formations; Stage II, 26.93.7 degrees counterclockwise rotation during deposition of the lower and middle Ranmugou formation; and Stage III, 17.73.3 degrees clockwise rotation after 43Ma. The complex rotation history recorded in the basin is possibly linked to sinistral shear along the Qiangtang block during India indentation into Asia and the early stage of the extrusion of the northwestern Indochina blocks away from eastern Tibet. KW - eastern Qiangtang terrane KW - Gongjue basin KW - paleomagnetism KW - inclination shallowing KW - rotation Y1 - 2018 U6 - https://doi.org/10.1002/2018JB015443 SN - 2169-9313 SN - 2169-9356 VL - 123 IS - 5 SP - 3320 EP - 3338 PB - American Geophysical Union CY - Washington ER - TY - JOUR A1 - Huang, Wentao A1 - van Hinsbergen, Douwe J. J. A1 - Lippert, Peter C. A1 - Guo, Zhaojie A1 - Dupont-Nivet, Guillaume T1 - Paleomagnetic tests of tectonic reconstructions of the India-Asia collision zone JF - Geophysical research letters N2 - Several solutions have been proposed to explain the long-standing kinematic observation that postcollisional upper crustal shortening within the Himalaya and Asia is much less than the magnitude of India-Asia convergence. Here we implement these hypotheses in global plate reconstructions and test paleolatitudes predicted by the global apparent polar wander path against independent, and the most robust paleomagnetic data. Our tests demonstrate that (1) reconstructed 600-750km postcollisional intra-Asian shortening is a minimum value; (2) a 52Ma collision age is only consistent with paleomagnetic data if intra-Asian shortening was 900km; a 56-58Ma collision age requires greater intra-Asian shortening; (3) collision ages of 34 or 65Ma incorrectly predict Late Cretaceous and Paleogene paleolatitudes of the Tibetan Himalaya (TH); and (4) Cretaceous counterclockwise rotation of India cannot explain the paleolatitudinal divergence between the TH and India. All hypotheses, regardless of collision age, require major Cretaceous extension within Greater India. KW - India-Asia collision KW - tectonic reconstruction KW - paleomagnetism Y1 - 2015 U6 - https://doi.org/10.1002/2015GL063749 SN - 0094-8276 SN - 1944-8007 VL - 42 IS - 8 SP - 2642 EP - 2649 PB - American Geophysical Union CY - Washington ER -