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  • 1
    Online Resource
    Online Resource
    Cambridge :Cambridge University Press,
    Keywords: Lithosphere. ; Geodynamics. ; Earth -- Crust. ; Electronic books.
    Description / Table of Contents: Presents a coherent synthesis of lithosphere studies, based on a full set of geophysical methods and complemented by petrologic and laboratory data on rock properties. This is a multidisciplinary resource for researchers and advanced students in geophysics, geodynamics, tectonics, petrology, and geochemistry, and for petroleum and mining industry professionals.
    Type of Medium: Online Resource
    Pages: 1 online resource (796 pages)
    Edition: 1st ed.
    ISBN: 9781139185578
    DDC: 551.13
    Language: English
    Note: Cover -- The lithosphere -- Title -- Copyright -- Dedication -- Contents -- Foreword -- Preface -- Acknowledgements -- 1 What is the lithosphere? -- 1.1 Historical note -- 1.2 Lithosphere definitions -- 1.2.1 Defining the lithospheric base -- 1.2.2 Elastic lithosphere -- 1.2.3 Thermal lithosphere -- 1.2.4 Seismic lithosphere -- 1.2.5 Electrical lithosphere -- 1.2.6 Petrologic lithosphere -- 1.3 Concepts related to the lithosphere -- 1.3.1 Boundary layers -- 1.3.2 Perisphere and tectosphere -- 1.4 An unnecessarily confusing concept? -- 2 Age of the lithosphere -- 2.1 Introduction to isotope geochronology -- 2.1.1 Geochemical classification of elements -- Lithophile, siderophile, and chalcophile elements -- Melting, partitioning, and depletion -- Chondrites, Bulk Earth, and Bulk Silicate Earth -- 2.1.2 Radioactive decay and the isochron equation -- 2.1.3 K/Ar -- 2.1.4 Rb/Sr -- 2.1.5 U/Pb -- 2.1.6 Sm/Nd -- 2.1.7 Re/Os -- 2.1.8 Lu/Hf -- 2.1.9 Mantle evolution from Hf and Nd isotopes -- 2.1.10 Model ages -- 2.2 Age of the crust and the lithospheric mantle -- 2.2.1 Continental crust -- Tectono-thermal and geological ages -- Old lithosphere in tectonically young regions -- Old crust-young lithospheric mantle in continental settings -- 2.2.2 Oceanic crust -- Continental crust trapped in mid-ocean ridge -- Recycled Precambrian lithosphere in mantle plumes -- 3 Seismic structure of the lithosphere -- 3.1 Laboratory studies of seismic properties of rocks -- 3.1.1 Introduction: Major elastic and anelastic parameters -- 3.1.2 Effects of pressure and temperature -- Seismic velocities -- Seismic attenuation, anelasticity, and effect of frequency -- 3.1.3 Effect of grain size variations -- 3.1.4 Effect of mineralogy -- 3.1.5 Anisotropy -- Pores and microcracks -- LPO anisotropy -- 3.1.6 Melt and fluid inclusions -- 3.1.7 Melt-depletion and mantle composition. , Oceanic melting trend -- Continental melting trend -- 3.1.8 Density-velocity relationship -- 3.2 Summary of seismic methods -- 3.2.1 Types of seismic waves -- 3.2.2 Theoretical limits on seismic wave resolution -- 3.2.3 Methods of seismic data interpretation -- One-dimensional techniques -- Ray theory -- The Herglotz-Wiechert-Bateman inversion -- Non-uniqueness of 1D velocity inversions -- 1D reference models of the Earth -- Two-dimensional techniques -- Three-dimensional techniques -- Preamble -- Regularization methods and damping -- Resolution tests and sensitivity analysis -- Earthquake location problem -- 3.3 Major seismic discontinuities in the lithosphere -- 3.3.1 The crust -- Continental crust -- Crustal layers -- The Moho and crustal thickness -- Principal types of the continental crust -- Stable parts of the continents -- Active parts of the continents -- Oceanic crust -- General patterns -- Anomalous oceanic crust -- 3.3.2 Seismic discontinuities in the upper mantle -- LVZ, G-discontinuity and the base of seismic lithosphere -- Lehmann (L-) discontinuity -- 3.4 Receiver function (converted waves) studies -- 3.4.1 The method -- P- and S-converted waves -- "Receiver functions" -- Limitations of the RF method -- The depth-velocity trade-off -- Moho and intracrustal discontinuities -- Mantle discontinuities and the S-receiver functions -- 3.4.2 Examples of PRF and SRF studies of the crust and the upper mantle -- Thickness of Precambrian crust in Greenland -- Lithosphere thickness in the collisional orogens of Central Asia -- Compositional boundary within the cratonic lithospheric mantle? -- Mantle transition zone and thermal state of the upper mantle -- 3.5 Controlled source methods: reflection/refraction studies of the upper mantle -- 3.5.1 Seismic reflection studies -- The method and its resolution -- Preamble. , Resolution of reflection methods -- Origin of crustal and mantle reflectivity -- Crustal reflectivity -- Reflection Moho -- Seismic discontinuities in the upper mantle -- Seismic reflection expression of tectonic styles -- Extended continental crust -- Collisional orogens and modern subduction zones -- Mantle reflectors and paleosubduction zones -- Dipping tectonic boundaries in the lithosphere -- 3.5.2 Seismic refraction and wide-angle reflection -- The method -- Heterogeneous upper mantle of Eurasia -- Preamble -- LVZs -- Teleseismic Pn -- Seismic discontinuities in the upper mantle beneath North America -- 3.6 Teleseismic seismology -- 3.6.1 Elastic tomography: methods and uncertainties -- Body-wave seismic tomography: uncertainty and resolution -- Surface-wave tomography: uncertainty and resolution -- Dispersion, vertical resolution, and depth leakage -- Ray path coverage and lateral resolution -- Crustal corrections -- Absolute versus relative velocities -- 3.6.2 Elastic tomography models of the upper mantle -- Global patterns -- Continents -- North America and Greenland -- South America -- Europe -- Siberia and Kazakhstan -- China, Mongolia, and India -- Australia -- Africa -- Antarctica -- Oceans -- Synopsis for some tectonic settings -- Stable continents -- Continental rifts -- Past and present subduction zones -- Mantle plumes and hotspots -- 3.6.3 Origin of seismic velocity anomalies in the upper mantle -- Correlations with the thermal regime -- Effect of water -- Effect of grain size -- Compositional anomalies -- Density-to-shear-wave velocity scaling factor -- 3.6.4 Seismic anisotropy in the upper mantle -- Types of anisotropy -- Origin of mantle anisotropy -- Body-wave studies -- Preamble -- Frozen versus asthenospheric anisotropy -- Global patterns -- Surface-wave anisotropy -- Preamble -- Continents -- Oceans. , 3.6.5 Lithosphere thickness from elastic tomography -- Definitions and uncertainties -- Global patterns -- 3.6.6 Anelastic tomography -- General remarks -- Correlations with surface tectonics -- Correlations with temperature and surface heat flow -- Correlations with seismic velocities -- 3.7 Seismic lithosphere: summary -- Factors affecting seismic velocities and attenuation -- Resolution problems -- Major results and global trends -- Thickness of seismic lithosphere: results and uncertainties -- 4 Thermal regime of the lithosphere from heat flow data -- 4.1 Field observations and laboratory data -- 4.1.1 Heat flow measurements -- Mechanisms of heat transfer and dimensionless numbers -- Accuracy of heat flow measurements -- 4.1.2 Thermal conductivity -- Mineral composition -- Porosity and fluid saturation -- Effect of temperature -- Effect of pressure -- Anisotropy -- 4.1.3 Thermal expansion, thermal diffusivity, and specific heat -- 4.1.4 Heat production -- Major heat-producing isotopes -- Laboratory measurements -- Near-surface samples -- Correlation between seismic velocity and heat production -- Exposed cross-sections of the deep crust -- Bulk heat production of the crust -- Chemical constraints -- Estimates from surface heat flow -- Heat production in the mantle -- Vertical and lateral variations in heat-producing elements -- Correlation between heat flow and heat production -- Depth variations of heat production -- Theoretical constraints -- Data from the Kola Superdeep Borehole -- Reduced heat flow -- 4.2 Heat flow data -- 4.2.1 Global compilations of surface heat flow -- 4.2.2 Global trends in surface heat flow -- 4.3 Thermal regime of oceanic lithosphere -- 4.3.1 Age dependence of seafloor topography and heat flow -- 4.3.2 Normal oceans -- Cooling half-space model -- Model predictions and empirical relationships. , Mantle potential temperature -- Cooling half-space model and ocean floor flattening -- Plate model -- Traditional approaches -- Oceanic geotherms -- Alternative approaches -- Testing half-space and plate models by observation -- Small-scale convection and geoid -- Ocean floor flattening: fact or artifact? -- 4.3.3 "Anomalous" oceans -- Subduction zones, marginal basins, and accretionary prisms -- Ocean plateaus and hot spots -- 4.4 Thermal regime of continental lithosphere -- 4.4.1 Heat flow on the continents -- Global observations -- Age dependence of continental heat flow -- Heat flow across the cratonic margins -- 4.4.2 Continental geotherms -- Time-scale of thermal equilibration -- Conductive geotherms for stable continents -- Uncertainties in conductive geotherms -- Mantle heat flow and mechanisms of surface heat flow variations in stable continents -- Thermal evolution of the mantle and the "Archean paradox" -- Continental regions with transient thermal regime -- Collisional orogens -- Extended regions -- Global patterns -- 4.4.3 Thickness of thermal lithosphere -- Thermal boundary layer -- Global patterns for the continents -- Statistical analysis of thermal model constrained by surface heat flow -- Lithosphere thickness-age correlation -- Global statistical thermal model -- Bimodal thickness of Archean-Paleoproterozoic lithosphere -- Lithosphere preservation, thermal blanketing, and heat diversion -- 4.5 Heat flow balance of the Earth -- 4.6 Thermal lithosphere: summary -- Factors affecting heat flow data -- Resolution problems -- Major results and global trends -- 5 Thermal state of the lithosphere from non-thermal data -- 5.1 Xenolith data -- 5.1.1 Xenoliths: advantages and disadvantages -- Xenoliths and xenocrysts -- Limitations of xenolith data -- 5.1.2 Xenoliths and the boundary layers -- Thermal boundary layer -- Chemical boundary layer. , Rheological boundary layer.
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  • 2
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    Elsevier
    In:  Precambrian Research, 259 . pp. 34-42.
    Publication Date: 2016-11-03
    Description: The southern part of the Baltic Shield hosts a series of mafic dykes and sills of Mesoproterozoic ages, including a ca. 1.53–1.46 Ga sheet-like gabbro-dolerite sills and the Salmi plateau-basalts from the Lake Ladoga region. Based on chiefly geochemical data, the region is conventionally interpreted as an intracratonic Ladoga rift (graben). We question the validity of this geodynamic interpretation by analyzing regional geophysical data (crustal structure, heat flow, Bouguer gravity anomalies, magnetic anomalies, and mantle Vs velocities). We provide a complete list of tectonic, magmatic, and geophysical characteristics typical of continental rifts in general and demonstrate that, except for magmatic and, perhaps, some gravity signature, the Lake Ladoga region lacks any other rift features. We also compare the geophysical data from the Lake Ladoga region with similar in age Midcontinent and Valday rifts, and provide alternative explanations for Mesoproterozoic geodynamic evolution of the southern Baltic Shield. We propose that Mesoproterozoic mafic intrusions in southern Fennoscandia may be associated with a complex deformation pattern during reconfiguration of (a part of) Nuna (Columbia) supercontinent, which led to magma intrusions as a series of mafic dykes along lithosphere weakness zones and ponding of small magma pockets within the cratonic lithosphere. Consequent magma cooling and its partial transition to eclogite facies could have led to the formation of a series of basement depressions, similar to intracratonic basins of North America, while spatially heterogeneous thermo-chemical subsidence, with phase transitions locally speeded by the presence of (subduction-related) fluids, could have produced a series of faults bounding graben-like structures.
    Type: Article , PeerReviewed
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  • 3
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    Springer Nature
    In:  In: Encyclopedia of Solid Earth Geophysics. , ed. by Gupta, H. Encyclopedia of Earth Sciences Series . Springer Nature, Cham, Switzerland, , 11 pp. ISBN 978-3-030-10475-7
    Publication Date: 2021-02-10
    Description: The Trans-European Suture Zone (TESZ) is the transition zone from the Precambrian East European Craton in the north and east to the younger Phanerozoic mobile belts to the south and west. It is the most prominent lithospheric tectonic feature of Europe. The term Trans-European Suture Zone was only adapted around year 2000 during the Pan-European EUROPROBE program of the European Science Foundation. Until then, parts of the zone were termed Teisseyre-Tornquist Zone, Sorgenfrei-Tornquist Zone, Trans-European Fault, and Tornquist Fan.
    Type: Book chapter , NonPeerReviewed
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  • 4
    Publication Date: 2023-02-08
    Description: Antarctica has traditionally been considered continental inside the coastline of ice and bedrock since Press and Dewart (1959). Sixty years later, we reconsider the conventional extent of this sixth continent. Geochemical observations show that subduction was active along the whole western coast of West Antarctica until the mid-Cretaceous after which it gradually ceased towards the tip of the Antarctic Peninsula. We propose that the entire West Antarctica formed as a back-arc basin system flanked by a volcanic arc, similar to e.g. the Japan Sea, instead of a continental rift system as conventionally interpreted. Globally, the fundamental difference between oceanic and continental lithosphere is reflected in hypsometry, largely controlled by lithosphere buoyancy. The equivalent hypsometry in West Antarctica (−580 ± 335 m on average, extending down to −1.6 km) is much deeper than in any continent, but corresponds to back-arc basins and oceans proper. This first order observation questions the conventional interpretation of West Antarctica as continental, since even continental shelves do not extend deeper than −200 m in equivalent hypsometry. We present a suite of geophysical observations that supports our geodynamic interpretation: a linear belt of seismicity sub-parallel to the volcanic arc along the Pacific margin of West Antarctica; a pattern of free air gravity anomalies typical of subduction systems; and extremely thin crystalline crust typical of back-arc basins. We calculate residual mantle gravity anomalies and demonstrate that they require the presence of (1) a thick sedimentary sequence of up to ca. 50% of the total crustal thickness or (2) extremely low density mantle below the deep basins of West Antarctica and, possibly, the Wilkes Basin in East Antarctica. Case (2) requires the presence of anomalously hot mantle below the entire West Antarctica with a size much larger than around continental rifts. We propose, by analogy with back-arc basins in the Western Pacific, the existence of rotated back-arc basins caused by differential slab roll-back during subduction of the Phoenix plate under the West Antarctica margin. Our finding reduces the continental lithosphere in Antarctica to 2/3 of its traditional area. It has significant implications for global models of lithosphere-mantle dynamics and models of the ice sheet evolution.
    Type: Article , PeerReviewed
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  • 5
    Publication Date: 2023-02-08
    Description: Highlights • The Radially averaged power spectrum method is applied to calculate average magnetic susceptibility in Iran. • The results demonstrate that known occurrences of Magmatic-Ophiolite Arcs (MOA) correlate with high average susceptibility areas. • We interpret two parallel, hitherto unknown, MOAs in eastern Iran which developed in a steeply dipping (〉60° dip) subduction zone. • Neo-Tethys subduction angle was shallow (〈20° dip) of in NW Iran and steep (〉60° dip) in SE Iran which indicates slab tearing. • We define a new outline of the economically important Tabas sedimentary basin. Abstract The Iranian plateau is one of the most complex geodynamic settings within the Alpine-Himalayan belt. The Paleo-Tethys and Neo-Tethys ocean subduction is responsible for the formation of several magmatic arcs and sedimentary basins within the plateau. These zones mostly are separated by thrust faults related to paleo-suture zones, which are highlighted by ophiolites. Sediment cover and overprint of a different magmatic phase from late Triassic to the Quaternary impede identification of some magmatic arcs and ophiolite belts. We track the known magmatic arcs, such as the Urmia-Dokhtar Magmatic Arc (UDMA), and unknown, sediment covered magmatic arcs by aeromagnetic data. We present a new map of average susceptibility calculated by the radially averaged power spectrum method. High average susceptibility values indicate the presence of a number of lineaments that correlate with known occurrences of Magmatic-Ophiolite Arcs (MOA), and low average susceptibility coincides with known sedimentary basins like Zagros, Makran, Kopeh-Dagh, and Tabas. In analogy to Zagros, low average susceptibility values indicate sedimentary basins to the south of the Darouneh fault and in the northern part of the Lut, Tabas and Yazd blocks. We interpret the Tabas basin as a pull-apart or back-arc basin. We identify hitherto unknown parallel MOAs in eastern Iran and the SE part of UDMA which both indicate steeply dipping (〉60° dip) paleo-subduction zones. In contrast, we interpret shallow subduction (〈20° dip) of Neo-Tethys in the NW part of UDMA as well as in the Sabzevar-Kavir MOA.
    Type: Article , PeerReviewed
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  • 6
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    Unknown
    AGU (American Geophysical Union) | Wiley
    Publication Date: 2023-02-08
    Description: We constrain the lithospheric mantle density of the North China Craton (NCC) at both in situ and standard temperature‐pressure (STP) conditions from gravity data. The lithosphere‐asthenosphere boundary (LAB) depth is constrained by our new thermal model, which is based on a new regional heat flow data set and a recent regional crustal model NCcrust. The new thermal model shows that the thermal lithosphere thickness is 〈120 km in most of the NCC, except for the northern and southern parts with the maximum depth of 170 km. The gravity calculations reveal a highly heterogeneous density structure of the lithospheric mantle with in situ and STP values of 3.22–3.29 and 3.32–3.40 g/cm3, respectively. Thick and reduced‐density cratonic‐type lithosphere is preserved mostly in the southern NCC. Most of the Eastern Block has a thin (90–140 km) and high‐density lithospheric mantle. Most of the Western Block has a high‐density lithospheric mantle and a thin (80–110 km) lithosphere typical of Phanerozoic regions, which suggests that the Archean lithosphere is no longer present there. We conclude that in almost the entire NCC the lithosphere has lost its cratonic characteristics by geodynamic processes that include, but are not limited to, the Paleozoic closure of the Paleo‐Asian Ocean in the north, the Mesozoic Yangtze Craton flat subduction in the south, the Mesozoic Pacific subduction in the east, the Cenozoic remote response to the Indian‐Eurasian collision in the west, and the Cenozoic extensional tectonics (possibly associated with the slab roll‐back) in the center.
    Type: Article , PeerReviewed
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  • 7
    Publication Date: 2021-09-01
    Description: This data publication contains the compilation of global heat-flow data by the International Heat Flow Commission (IHFC; http://www.ihfc-iugg.org/) of the International Association of Seismology and Physics of the Earth's Interior (IASPEI). The presented data release 2021 contains data generated between 1939 and 2021 and constitutes an updated and extended version of the 2012 IHFC database release (IHFC 2012; later re-published as PANGAEA release: Global Heat Flow Compilation Group, 2013). The 2021 release contains 74,548 heat-flow data from 1,403 publications. 55% of the reported heat-flow values are from the continental domain (n ~ 40,870), while the remaining 45% are located in the oceanic domain (n ~ 33,678). The data are provided in csv and Excel formats. Compared to earlier compilations, which followed the structure defined by Jessop et al. (1976), the new data release was transformed to the recently redefined structure for reporting and storing heat-flow data in the Global Heat Flow Database (Fuchs et al., 2021). Therefore, the notation and structure of the database was adopted, transforming the database field entries defined after Jessop et al. (1976) to the new field structure. Old code notations are not continued and the dataset was cleaned for entries without reporting any heat-flow value. Although successfully transformed, this release marks an intermediate step as the majority of the newly defined database fields have not been filled yet. Filling these fields, checking the existing entries and assessing the quality of each entry are the aim of the upcoming Global Heat Flow Data Assessment Project, for which this data set provides the basis. Consequently, we kindly ask the user to take notice that the current release still suffers similar problems as previously published compilations in terms of data heterogeneity, documentation and quality.
    Type: Other , NonPeerReviewed
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  • 8
    Publication Date: 2022-12-13
    Description: This data publication contains the compilation of global heat-flow data by the International Heat Flow Commission (IHFC; http://www.ihfc-iugg.org/) of the International Association of Seismology and Physics of the Earth's Interior (IASPEI). The presented data release 2021 contains data generated between 1939 and 2021 and constitutes an updated and extended version of the 2012 IHFC database release (IHFC 2012; later re-published as PANGAEA release: Global Heat Flow Compilation Group, 2013). The 2021 release contains 74,548 heat-flow data from 1,403 publications. 55% of the reported heat-flow values are from the continental domain (n ~ 40,870), while the remaining 45% are located in the oceanic domain (n ~ 33,678). The data are provided in csv and Excel formats. Compared to earlier compilations, which followed the structure defined by Jessop et al. (1976), the new data release was transformed to the recently redefined structure for reporting and storing heat-flow data in the Global Heat Flow Database (Fuchs et al., 2021). Therefore, the notation and structure of the database was adopted, transforming the database field entries defined after Jessop et al. (1976) to the new field structure. Old code notations are not continued and the dataset was cleaned for entries without reporting any heat-flow value. Although successfully transformed, this release marks an intermediate step as the majority of the newly defined database fields have not been filled yet. Filling these fields, checking the existing entries and assessing the quality of each entry are the aim of the upcoming Global Heat Flow Data Assessment Project, for which this data set provides the basis. Consequently, we kindly ask the user to take notice that the current release still suffers similar problems as previously published compilations in terms of data heterogeneity, documentation and quality.
    Type: Report , NonPeerReviewed
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  • 9
    Publication Date: 2023-03-21
    Description: Stable cratons with a thick (〉 200 km) and cold lithosphere form rheologically strong plates that move atop a ductile asthenospheric mantle. Various types of seismic observations show the presence of a potentially rheologically weak zone at depths of ca. 80 – 150 km termed the Mid-Lithosphere Discontinuity (MLD). While various mechanisms may explain the MLD, the dynamic processes leading to the seismic observations are unclear. We propose that the MLD can be caused by channel flow in the lower lithosphere, triggered by negative Rayleigh-Taylor instabilities at cratonic margins in the Archean, when the mantle was hotter than at present. Presence of a chemically distinct, low-density cratonic lithospheric root is required to initiate the process. Numerical modeling shows that the top of the channel flow creates a shear zone at a depth comparable to the globally observed seismic MLD. Grain size reduction in the shear zone and accumulation of percolated melts or fluids along the channel top may reduce seismic wave speeds as observed in the MLD, while the channel flow itself may explain radial anisotropy of seismic wave speeds. Secular cooling of the Earth deepens the top of the channel flow on a 1 Gyr scale, and early-stage large-scale (1000’s km long) channel flow deformation switches to a different deformation style with a smaller (100’s km) wavelength. These different flow patterns may explain the different seismic response of the MLD and the lithosphere base.
    Type: Article , NonPeerReviewed
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  • 10
    Publication Date: 2024-02-07
    Description: All models of the magmatic and plate tectonic processes that create continental crust predict the presence of a mafic lower crust. Earlier proposed crustal doubling in Tibet and the Himalayas by underthrusting of the Indian plate requires the presence of a mafic layer with high seismic P-wave velocity (Vp 〉 7.0 km/s) above the Moho. Our new seismic data demonstrates that some of the thickest crust on Earth in the middle Lhasa Terrane has exceptionally low velocity (Vp 〈 6.7 km/s) throughout the whole 80 km thick crust. Observed deep crustal earthquakes throughout the crustal column and thick lithosphere from seismic tomography imply low temperature crust. Therefore, the whole crust must consist of felsic rocks as any mafic layer would have high velocity unless the temperature of the crust were high. Our results form basis for alternative models for the formation of extremely thick juvenile crust with predominantly felsic composition in continental collision zones.
    Type: Article , PeerReviewed
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