Reconciling Paleomagnetism and Pangea.

Although an array of geological and geophysical data support the conventional (Wegenerian) paleogeographic model of Pangea in the Late Triassic-Early Jurassic, its configuration in pre-Late Triassic time has remained controversial for the last half-century. Late Carboniferous to Middle Triassic paleomagnetic data have been repeatedly shown to be incompatible with the conventional model, leading to alternative paleogeographic reconstructions, built to accomodate the paleomagnetic records. However, these models invariably require dubious tectonic transformations that lack supporting evidence in the form of structural relics. An altogether different explanation for the model-data incongruity invokes significant non-dipole geomagnetic fields, but this undermines a core assumption in paleomagnetism: the geocentric axial dipole hypothesis. As paleomagnetic analysis is the only quantitative method for determining paleolatitude in pre-Cretaceous time, this persisting discrepancy between the conventional model and the paleomagnetic data has come to be a first-order problem in tectonics and paleomagnetism. This dissertation explores the third and final hypothetical solution to this problem: that the discrepancy is due to systemic bias in the paleomagnetic data. This hypothesis is tested by collecting new, high-quality, Permian and Triassic paleomagnetic data from Laurussia and Gondwana, by conducting tests for quality and bias on the published paleomagnetic data, and by re-evaluating Pangea reconstructions in light of these findings. It is established that with use of accurate Euler parameters and high-fidelity paleomagnetic data, the conventional paleogeographic model can be reconciled with the Carboniferous-Middle Triassic paleomagnetic record. The findings of this dissertation thus imply that neither alternative reconstructions or significant non-dipole magnetic fields need to be invoked to resolve this long-standing problem. Furthermore, the documentation of systemic bias in the studied paleomagnetic data has broader implications for paleomagnetism and derivative work; namely that erroneously shallow inclinations (in sediments), among other forms of bias, are likely to be pervasive in the present paleomagnetic data.Ph.D.GeologyUniversity of Michigan, Horace H. Rackham School of Graduate Studieshttp://deepblue.lib.umich.edu/bitstream/2027.42/91410/1/domeier_1.pd

A Tracer-Based Algorithm for Automatic Generation of Seafloor Age Grids from Plate Tectonic Reconstructions

The age of the ocean floor and its time-dependent age distribution control fundamental features of the Earth, such as bathymetry, sea level and mantle heat loss. Recently, the development of increasingly sophisticated reconstructions of past plate motions has provided models for plate kinematics and plate boundary evolution back in geological time. These models implicitly include the information necessary to determine the age of ocean floor that has since been lost to subduction. However, due to the lack of an automated and efficient method for generating global seafloor age grids, many tectonic models, most notably those extending back into the Paleozoic, are published without an accompanying set of age models for oceanic lithosphere. Here we present an automatic, tracer-based algorithm that generates seafloor age grids from global plate tectonic reconstructions with defined plate boundaries. Our method enables us to produce the first seafloor age models for the Paleozoic's lost ocean basins. Estimated changes in sea level based on bathymetry inferred from our new age grids show good agreement with sea level record estimations from proxies, providing a possible explanation for the peak in sea level during the assembly phase of Pangea. This demonstrates how our seafloor age models can be directly compared with observables from the geologic record that extend further back in time than the constraints from preserved seafloor. Thus, our new algorithm may also aid the further development of plate tectonic reconstructions by strengthening the links between geological observations and tectonic reconstructions of deeper time

Support for an “A‐type” Pangea reconstruction from high‐fidelity Late Permian and Early to Middle Triassic paleomagnetic data from Argentina

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94802/1/jgrb16956-sup-0006-fs04.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/94802/2/jgrb16956-sup-0005-fs03.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/94802/3/jgrb16956.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/94802/4/jgrb16956-sup-0008-fs06.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/94802/5/jgrb16956-sup-0004-fs02.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/94802/6/jgrb16956-sup-0007-fs05.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/94802/7/jgrb16956-sup-0003-fs01.pd

The ∼270 Ma palaeolatitude of Baltica and its significance for Pangea models

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/86901/1/j.1365-246X.2011.05061.x.pd

New Late Permian paleomagnetic data from Argentina: Refinement of the apparent polar wander path of Gondwana

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95004/1/ggge1994.pd

Early Paleozoic tectonics of Asia: Towards a full-plate model

Asia is key to a richer understanding of many important lithospheric processes such as crustal growth, continental evolution and orogenesis. But to properly decipher the secrets Asia holds, a first-order tectonic context is needed. This presents a challenge, however, because a great variety of alternative and often contradictory tectonic models of Asia have flourished. This plethora of models has in part arisen from efforts to explain limited observations (in space, time or discipline) without regard for the broader assemblage of established constraints. The way forward, then, is to endeavor to construct paleogeographic models that fully incorporate the diverse constraints available, namely from quantitative paleomagnetic data, the plentiful record of geologic and paleobiologic observations, and the principles of plate tectonics. This paper presents a preliminary attempt at such a synthesis concerning the early Paleozoic tectonic history of Asia. A review of salient geologic observations and paleomagnetic data from the various continental blocks and terranes of Asia is followed by the presentation of a new, full-plate tectonic model of the region from middle Cambrian to end-Silurian time (500–420 Ma). Although this work may serve as a reference point, the model itself can only be considered provisional and ideally it will evolve with time. Accordingly, all the model details are released so that they may be used to test and improve the framework as new discoveries unfold

Plate tectonics in the late Paleozoic

As the chronicle of plate motions through time, paleogeography is fundamental to our understanding of plate tectonics and its role in shaping the geology of the present-day. To properly appreciate the history of tectonics—and its influence on the deep Earth and climate—it is imperative to seek an accurate and global model of paleogeography. However, owing to the incessant loss of oceanic lithosphere through subduction, the paleogeographic reconstruction of ‘full-plates’ (including oceanic lithosphere) becomes increasingly challenging with age. Prior to 150 Ma ∼60% of the lithosphere is missing and reconstructions are developed without explicit regard for oceanic lithosphere or plate tectonic principles; in effect, reflecting the earlier mobilistic paradigm of continental drift. Although these ‘continental’ reconstructions have been immensely useful, the next-generation of mantle models requires global plate kinematic descriptions with full-plate reconstructions. Moreover, in disregarding (or only loosely applying) plate tectonic rules, continental reconstructions fail to take advantage of a wealth of additional information in the form of practical constraints. Following a series of new developments, both in geodynamic theory and analytical tools, it is now feasible to construct full-plate models that lend themselves to testing by the wider Earth-science community. Such a model is presented here for the late Paleozoic (410–250 Ma) together with a review of the underlying data. Although we expect this model to be particularly useful for numerical mantle modeling, we hope that it will also serve as a general framework for understanding late Paleozoic tectonics, one on which future improvements can be built and further tested

Subduction flux modulates the geomagnetic polarity reversal rate

The cause of variations in the frequency of geomagnetic polarity reversals through the Phanerozoic has remained a primary research question straddling palaeomagnetism and geodynamics for decades. Numerical models suggest the primary control on geomagnetic reversal rate on 10 to 100 Ma timescales is the changing heat flux across the core-mantle boundary, a flux which is expected to be influenced by variations in the lithosphere subducted into the mantle. A positive relationship between the time-dependent global subduction flux and magnetic reversal rate is expected, with a time delay to transmit the thermal imprint into the lowermost mantle. We perform the first test of this hypothesis using subduction flux estimates and geomagnetic reversal rate data back to the early Paleozoic. Subduction area flux is derived from global, full-plate tectonic models, and evaluated against independent subduction flux proxies based on strontium isotopes and age distribution of detrital zircons . A continuous Phanerozoic reversal rate model is built from pre-existing compilations back to ~320 Ma plus a new reversal rate model in the data-sparse mid-to-early Paleozoic. Cross-correlation of the time-dependent subduction flux and geomagnetic reversal rate series reveals a significant correlation with a time delay of ~120 Ma (with reversals trailing the subduction flux). This time delay represents a value intermediate between the seismologically constrained time expected for a subducted slab to transit from the surface to the core-mantle boundary (~150-300 Ma), and the much shorter lag time predicted by some numerical models of mantle flow (~30-60 Ma). Our novel estimate of lag time, encouragingly represents a compromise between them. Important uncertainties in our proposed relationship remain, but the results cast new light on the dynamic connections between the surface and deep Earth, and will help to constrain new models linking mantle convection, the thermal evolution of the lowermost mantle, and the geodynamo

Evidence for large disturbances of the Ediacaran geomagnetic field from West Africa

Constraining the paleogeography of the Ediacaran is crucial for understanding the extensive tectonic, biological and geochemical changes that occurred during that epoch. Paleomagnetism is an essential tool for reconstructing the Ediacaran paleogeography but it is complicated because the paleomagnetic data of that age display unusually fast and large directional oscillations. Two main competing hypotheses have been proposed: the occurrence of very fast True Polar Wander (TPW) episodes, which correspond to the motion of the planetary spin axis relative to the solid Earth, or strong geomagnetic field disturbances that could potentially be dominated by an equatorial dipole field. Their implications for paleogeographic reconstructions are radically different as TPW would result in a major latitudinal shift of continents of up to ∼ 90°. In this study, we focus on one rapid paleomagnetic change recorded in pyroclastic rocks of the Ouarzazate Group in the Anti-Atlas Belt (Morocco) that has been interpreted to reflect an exceptionally fast episode of True Polar Wander between ∼ 575 and 565 Ma. To further test this hypothesis, tight constraints on the rate of the paleomagnetic directional change are needed, as TPW is speed-limited by mantle viscosity. Here, we present high-resolution Chemical Abrasion Isotope-Dilution Thermal Ionization Mass Spectrometry (CA-ID-TIMS) U-Pb dates on zircons from seven pyroclastic levels distributed stratigraphically below, in between and above the horizons where the large paleomagnetic change is observed. Based on these new data, we estimate the associated lower bound rate of the apparent polar motion related to this abrupt paleomagnetic change to be 11.6°/Myrs [5.5 – 17.9]. This value is much higher than the TPW speed limit estimated from numerical simulations, suggesting that this large paleomagnetic change cannot be explained by TPW. It could rather be associated with intense perturbations of the Ediacaran geomagnetic field potentially oscillating from an axial to an equatorial dipole. The paleomagnetic pole that we interpret as referring to the axial dipole field would imply that West Africa was located at high latitude during the mid-Ediacaran