Magnetic Memory of Rocks: the Kazakhstan Orocline and Climatic Record of the Indian Monsoon.

The Kazakhstan orocline, a pair of concentric horseshoe-shaped volcanic arcs of Devonian (external) and late Paleozoic (internal) age, is thought to have formed during the amalgamation of Eurasia. Paleomagnetic investigations of several volcanic complexes ranging in age from Silurian to Permian are described in Chapters 2, 3 and 4 of this thesis. These studies have resulted in the construction of a tectonic model for the formation of the Kazakhstan orocline. Our results suggest that in the Middle Devonian, a nearly straight, northwest-southeast trending volcanic arc delineated the northeastern margin of the Kazakhstania landmass. In the Late Devonian, an initial collision with Tarim pinned Kazakhstania’s southern corner, while dextral shear motion and the considerable clockwise rotation of Siberia dragged its northern end. Relative convergence between Siberia and Tarim caused initial buckling of the Kazakhstania continent trapped between them, subdividing the volcanic arc into three (southwestern, middle, and northeastern) segments. Continued subduction under the established limbs of the orocline, with an estimated outward-directed subduction velocity of ~6mm/yr, gradually led to the closure of the intervening Junggar-Balkhash Ocean and tightening of the orocline. By the Late Permian, the Junggar-Balkhash Ocean no longer existed and the Kazakhstan orocline had obtained its present-day strongly curved shape. The ratio of two pedogenic iron oxides, goethite and hematite, has been demonstrated to be a good proxy for precipitation in soil-forming (terrestrial) environments. A similar interpretation of the mineral ratio has been increasingly applied to studies of marine sediments, in which variation in the goethite to hematite ratio is thought to reflect variation in the precipitation regime at the source area of the sediments. The rock magnetic study of Bengal Fan sediments described in Chapter 5 of this thesis suggests that in some intervals of the studied sedimentary section, variation in the ratio reflects a change in the degree of diagenetic alteration of the initial detrital assemblage rather than a climatic signal. Therefore, when assigning climatic interpretation to changes in the relative abundance of goethite and hematite in marine sediments, the possibility of diagenetic modification should be evaluated.Ph.D.GeologyUniversity of Michigan, Horace H. Rackham School of Graduate Studieshttp://deepblue.lib.umich.edu/bitstream/2027.42/60781/1/alexabra_1.pd

Magnetic fingerprint of southern Portuguese speleothems and implications for paleo- and environmental magnetism

Environmental magnetism of speleothems is still in its early stage of development. Here we report on our investigation of the environmental and paleomagnetic information that has been recorded in speleothems, and what are the factors that control its preservation and reliability. To address these issues, we used a multidisciplinary approach, including rock magnetism, petrography, scanning electron microscopy, stable carbon and oxygen isotope compositions, and major and trace element concentrations. We applied this to a set of samples from different stages of speleothem evolution: present-day dripwater (glass plates), a weathered stalactite, a fresh stalagmite, cave sediments, and terra rossa soils. These samples come from the Penico and Excentricas caves, located in two distinct aquifers of the Algarve region, South Portugal. Our results show that the main magnetic carriers of the speleothems under study are primary (detrital) and consist of maghemite (and magnetite?). Similarities in coercivity and temperature dependence of the studied set of samples suggest that iron oxides are inherited from the terra rossa soils that cap the cave and were transported to the speleothems by dripwater. Hence, they represent a regional environmental signature. Interestingly, a stable and probably detrital remanent magnetization could be isolated in the fresh stalagmite, whereas the weathered stalactite yielded chaotic magnetic directions and very low remanent intensities. We propose that these low intensities can be the result from(i) different remanence acquisition mechanisms between stalagmite and stalactite and/or (ii) iron dissolution by fungal activity. We also suggest that magnetic properties and color and the content in detrital elements in the fresh speleothem inform about environmental processes acting on the interface of rock (soil)-atmosphere, while oxygen isotope composition and alkaline-earth element concentrations inform about calcite-water interaction processes. These results provide a better understanding of how environmental information is recorded in speleothems and what the factors are that control the reliability of the paleomagnetic and paleo-environmental signal.info:eu-repo/semantics/acceptedVersio

Editorial: Magnetic Records of Extreme Geological Events

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When and where did India and Asia collide?

Timing of the collision between India and Asia is the key boundary condition in all models for the evolution of the Himalaya-Tibetan orogenic system. Thus it profoundly affects the interpretation of the rates of a multitude of associated geological processes ranging from Tibetan Plateau uplift through continental extrusion across eastern Asia, as well as our understanding of global climate change during the Cenozoic. Although an abrupt slowdown in the rate of convergence between India and Asia around 55 Ma is widely regarded as indicating the beginning of the collision, most of the effects attributed to this major tectonic episode do not occur until more than 20 Ma later. Refined estimates of the relative positions of India and Asia indicate that they were not close enough to one another to have collided at 55 Ma. On the basis of new field evidence from Tibet and a reassessment of published data we suggest that continent-continent collision began around the Eocene/Oligocene boundary (∼34 Ma) and propose an alternative explanation for events at 55 Ma. Copyright 2007 by the American Geophysical Union.published_or_final_versio

Bainang Terrane, Yarlung-Tsangpo suture, southern Tibet (Xizang, China): A record of intra-Neotethyan subduction-accretion processes preserved on the roof of the world

The Bainang terrane, an intra-oceanic island are subduction complex into which Tethyan oceanic rocks were accreted during the Cretaceous, is preserved within the Yarlung-Tsangpo suture zone of Tibet. The lithostratigraphic succession established from field mapping records a long history of sedimentation in different portions of the central Tethyan domain from Late Triassic to mid-Cretaceous time. These rocks are preserved within a south-verging imbricate thrust stack of thin (≪ 1 km thick) northward younging tectonic slices. Five lithotectonic units were mapped in the terrane and these units are assigned to two distinct tracts. The northern tract, which accumulated on the north side of Neotethys, was probably separated from its southern counterpart by a mid-ocean ridge. Detailed radiolarian biostratigraphy is used to constrain the timing of depositional events within each tract. Oceanic plate stratigraphy of the northern tract records its northward travel and mid-Cretaceous (late Aptian) approach towards a south-facing intra-oceanic subduction zone. Rocks in the southern tract developed closer to the Indian subcontinent and experienced thermotectonic subsidence and Mid-Jurassic basic alkaline intraplate magmatism. They were probably accreted late in the Cretaceous. Variations in structural style across the terrane indicate deformation at different depths and vertical growth of the wedge rather than lateral accretion. The overall tectonostratigraphy of the terrane reflects its development in a remote intra-oceanic setting.published_or_final_versio

Precise radiolarian age constraints on the timing of ophiolite generation and sedimentation in the Dazhuqu terrane, Yarlung-Tsangpo suture zone, Tibet

Well-preserved, abundant radiolarians provide high-precision biostratigraphic age constraints on the timing of the eruption of ophiolitic basalts exposed along the Yarlung-Tsangpo suture zone in southern Tibet. Dazhuqu terrane ophiolites were generated in an intra-oceanic supra-subduction zone setting within a relatively short (<10 Ma) interval from late Barremian to late Aptian. Accumulation of sediments upon the newly generated ophiolite initially occurred in a series of discrete rift-controlled sub-basins associated with various spreading centres. An increasing flux of arc-derived volcaniclastic sediment up-section indicates nearby volcanic are activity. The Dazhuqu terrane developed in an intra-oceanic setting within Tethys where it was isolated from any continental influence.published_or_final_versio

Snowball Earth climate dynamics and Cryogenian geology–geobiology

Geological evidence indicates that grounded ice sheets reached sea level at all latitudes during the long‐lived Sturtian (717–659 Ma) and Marinoan (ca 645–635 Ma) glaciations. Combined U-­‐Pb and Re-­‐Os geochronology suggests that the Sturtian glacial onset and both terminations were globally synchronous. Geochemical data imply that atmospheric pCO2 was 102x modern at the Marinoan termination, consistent with Snowball Earth hysteresis. Sturtian glaciation followed the breakup of a tropical supercontinent, and its onset coincided with the equatorial emplacement of a large igneous province. Modeling shows that the small thermal inertia of a globally frozen surface reverses the annual-mean Hadley circulation, resulting in equatorial net sublimation and net deposition elsewhere. Oceanic ice thickens, forming a sea glacier that flows gravitationally toward the equator, sustained by the hydrologic cycle and by basal freeze-on and melting. Tropical ice sheets flow faster as CO2 rises, but lose mass and become sensitive to orbital forcing. Dust accumulation in the equatorial zone engenders supraglacial oligotrophic meltwater ecosystems, favorable for cyanobacteria and many eukaryotes. Meltwater flushing through moulins enables organic burial and submarine deposition of subaerially-­‐erupted volcanic ash. The subglacial ocean is turbulent and well­‐mixed, in response to geothermal heating and conductive heat loss through the ice cover, increasing with latitude. Cap carbonates, unique to Snowball Earth terminations, are products of intense weathering and ocean stratification. Whole-­ocean warming and ice-sheet forebulge collapse allow marine coastal inundations to progress long after ice-sheet disappearance. The evolutionary legacy of Snowball Earth is perceptible in fossils and living organisms

Hematite (a-Fe2O3) quantification in sedimentary magnetism: limitations of existing proxies and ways forward

Determination of hematite contributions to sedimentary magnetizations is an important but difficult task in quantitative environmental studies. The poorly crystalline and fine-grained nature of hematite nanoparticles makes quantification of their concentrations in natural environments challenging using mineralogical and spectroscopic methods, while the weak magnetization of hematite and often significant superparamagnetic nanoparticle concentrations make quantification difficult using magnetic remanence measurements. We demonstrate here that much-used magnetic parameters, such as the S-ratio and "hard" isothermal remanent magnetization (HIRM), tend to significantly underestimate relative and absolute hematite contents, respectively. Unmixing of isothermal remanent magnetization (IRM) acquisition curves is among the more suitable approaches for defining magnetic mineral contributions, although it has under-appreciated uncertainties that limit hematite quantification. Diffuse reflectance spectroscopy and other methods can enable relative hematite and goethite content quantification under some conditions. Combined use of magnetic, mineralogical, and spectroscopic approaches provides valuable cross-checks on estimated hematite contents; such an integrated approach is recommended here. Further work is also needed to rise to the challenge of developing improved methods for hematite quantification

НОВЫЕ ПАЛЕОМАГНИТНЫЕ ДАННЫЕ ПО СИЛУРИЙСКИМ И ДЕВОНСКИМ ВУЛКАНИТАМ ЧИНГИЗСКОЙ ОСТРОВНОЙ ДУГИ КАЗАХСТАНА И ИХ ВКЛАД В ПРЕДСТАВЛЕНИЯ О ТЕКТОНИЧЕСКОЙ ЭВОЛЮЦИИ УРАЛО-МОНГОЛЬСКОГО ПОЯСА

The tectonic and paleogeographic evolution of the Ural-Mongol belt between the cratons of Baltica, Siberia, and Tarim is the key to the formation of the Eurasian supercontinent during Paleozoic time, but the views on this complicated process remain very disparate and sometimes controversial. Three volcanic formations of the Middle Silurian, LowertoMiddle Devonian and Middle Devonian age from the southwestern boundary of the Chingiz Range (NE Kazakhstan) yields what are interpreted as primary paleomagnetic directions that help clarify the evolution of the belt. A singlepolarity characteristic component in midSilurian andesites yields a positive intraformational conglomerate test, whereas dualpolarity prefolding components are isolated from the two Devonian collections. These new data were evaluated together with previously published paleomagnetic results from Paleozoic rocks in the Chingiz Range, and allow us to establish with confidence the hemisphere in which the area was located at a given time. We conclude that NE Kazakhstan was steadily moving northward crossing the equator in Silurian time. These new paleomagnetic data from the Chingiz range also agree with and reinforce the hypothesis that the strongly curved volcanic belts of Kazakhstan underwent oroclinal bending between Middle Devonian and Late Carboniferous time. A comparison of the Chingiz paleolatitudes with those of Siberia shows similarities between the northward motion and rotational history of the Chingiz unit and those of Siberia, which imposes important constraints on the evolving paleogeography of the Ural-Mongol belt.Тектоническая эволюция Урало-Монгольского подвижного пояса (УМП) многие десятилетия является предметом исследования огромного количества авторов. Однако, несмотря на все усилия, тектонические реконструкции разных авторов различаются самым радикальным образом, а во многом являются взаимоисключающими. Один из способов прояснить ситуацию – получить последовательности разновозрастных палеомагнитных определений и на их основе оценить кинематику ключевых структур УМП. При палеомагнитных исследованиях среднепалеозойских вулканитов Чингизской палеоостровной дуги на северо-востоке Казахстана в андезитах середины силура была выделена первичная компонента намагниченности, что подтверждается положительным тестом галек для внутриформационного конгломерата. В двух среднедевонских объектах также была выделена первичная намагниченность, для которой тест складки и тест обращения положительны. Объединив все имеющиеся данные по этому региону, мы получили последовательность палеомагнитных определений в интервале с позднего кембрия до поздней перми, что позволило уверенно определить, в каком полушарии находилась Чингизская палеодуга. Сделан вывод, что эта структура устойчиво смещалась к северу и пересекла экватор в силуре. Имеющиеся данные так же уверенно указывают на вторичную природу изгиба вулканических поясов Казахстана, имеющих подковообразные очертания. Сравнение этих данных с кривой кажущейся миграции полюса Сибирской платформы позволяет говорить о том, что большую часть палеозоя Чингизская палеодуга двигалась согласованно с Сибирской платформой, что накладывает жесткие ограничения на эволюцию УМП