Detection of a New Sub-Lithospheric Discontinuity in Central Europe with S-Receiver Functions
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Chapter 3. the Crust and Upper Mantle
Theory of the Earth Don L. Anderson Chapter 3. The Crust and Upper Mantle Boston: Blackwell Scientific Publications, c1989 Copyright transferred to the author September 2, 1998. You are granted permission for individual, educational, research and noncommercial reproduction, distribution, display and performance of this work in any format. Recommended citation: Anderson, Don L. Theory of the Earth. Boston: Blackwell Scientific Publications, 1989. http://resolver.caltech.edu/CaltechBOOK:1989.001 A scanned image of the entire book may be found at the following persistent URL: http://resolver.caltech.edu/CaltechBook:1989.001 Abstract: T he structure of the Earth's interior is fairly well known from seismology, and knowledge of the fine structure is improving continuously. Seismology not only provides the structure, it also provides information about the composition, crystal structure or mineralogy and physical state. In subsequent chapters I will discuss how to combine seismic with other kinds of data to constrain these properties. A recent seismological model of the Earth is shown in Figure 3-1. Earth is conventionally divided into crust, mantle and core, but each of these has subdivisions that are almost as fundamental (Table 3-1). The lower mantle is the largest subdivision, and therefore it dominates any attempt to perform major- element mass balance calculations. The crust is the smallest solid subdivision, but it has an importance far in excess of its relative size because we live on it and extract our resources from it, and, as we shall see, it contains a large fraction of the terrestrial inventory of many elements. In this and the next chapter I discuss each of the major subdivisions, starting with the crust and ending with the inner core. -
The Deep Structure of Continents
VOL. 84, NO. B I3 JOURNAL OF GEOPHYSICAL RESEARCH DECEMBER 10, 1979 The Deep Structure of Continents DON L. ANDERSON SeismologicalLaboratory, California Institute of Technology,Pasadena, California 91125 The Lehmann discontinuityat 220-km depth is an important global feature which occursunder both oceansand continents.It is a barrier to penetrationby younglithosphere and marks the baseof seismic- ity in regionsof continent-continentcollision. The stronglateral variationin uppermantle velocitiesoc- cursmainly abovethis depth. Continentalroots extend no deeperthan about 150-200 km. The basalt- eclogitetransformation and eclogite-harzburgiteseparation may be responsiblefor the geometryof inter- mediatedepth earthquakes.Oceanic and continentalgeotherms converge above about 200 km and be- comeless steep than the meltinggradient at greaterdepth. This impliesa low viscositychannel near 250 km. This would give a decouplingzone of maximumshear beneath continental shields. The Lehmann discontinuitymay be the interfacebetween two distinctgeochemical reservoirs. The velocityjump, and the inferreddensity jump, at 220 km are consistentwith an increasein garnetcontent. The mantle may be garnetlherzolite above and eclogiteimmediately below the Lehmanndiscontinuity. The transitionre- gion may be mainly eclogiteand be the sourceregion for oceanictholeiites. INTRODUCTION nental values[Jordan and Anderson,1974; Jordan, 1975].Hart et al. [1977] determined an attenuation corrected free oscilla- Continental lithosphereis much thicker than oceanic litho- sphere,but the question of how thick a sectionof continent tion averageearth model, QM2, which is comparedwith the translatescoherently during continental drift has not yet been continentalmodel SHR14 of Helmbergerand Engen[1974] in adequatelyaddressed. The bottom of the low-velocity zone is Figure 2. A more direct comparisonis the Pacific-easternU.S. usuallyconsidered to be the bottom of the asthenosphereand curve which is from Cara's [1979] surfacewave study. -
Upper-Mantle Low-Velocity Zone Structure Beneath the Kaapvaal Craton from S-Wave Receiver Functions
Geophys. J. Int. (2009) doi: 10.1111/j.1365-246X.2009.04178.x Upper-mantle low-velocity zone structure beneath the Kaapvaal craton from S-wave receiver functions Samantha E. Hansen,1 Andrew A. Nyblade,2 Jordi Julia,` 1 Paul H.G.M. Dirks3 and Raymond J. Durrheim3 1Department of Geosciences, 407 Deike Bldg., Pennsylvania State University, University Park, PA 16802, USA. E-mail: [email protected] 2Department of Geosciences, 447 Deike Bldg., Pennsylvania State University, University Park, PA 16802, USA 3School of Geosciences, University of the Witwatersrand, Private Bag X3, Wits 2050, South Africa Accepted 2009 March 10. Received 2009 February 9; in original form 2008 October 3 SUMMARY The southern African Plateau is marked by anomalously high elevations, reaching 1–2 km above sea level, and there is much debate as to whether this topography is compensated by a lower mantle source or by elevated temperatures in the upper mantle. In this study, we use S-wave receiver functions (SRFs) to estimate the lithospheric thickness and sublithospheric mantle velocity structure beneath the Kaapvaal craton, which forms the core of the Plateau. To fit the SRF data, a low-velocity zone (LVZ) is required below a ∼160-km-thick lithospheric lid, but the LVZ is no thicker than ∼90 km. Although the lid thickness obtained is thinner than that reported in previous SRF studies, neither the lid thickness nor the shear velocity decrease (∼4.5%) associated with the LVZ is anomalous compared to other cratonic environ- ments. Therefore, we conclude that elevated temperatures in the sublithospheric upper mantle contribute little support to the high elevations in this region of southern Africa. -
Asthenosphere–Lithospheric Mantle Interaction in an Extensional Regime
Chemical Geology 233 (2006) 309–327 www.elsevier.com/locate/chemgeo Asthenosphere–lithospheric mantle interaction in an extensional regime: Implication from the geochemistry of Cenozoic basalts from Taihang Mountains, North China Craton ⁎ Yan-Jie Tang , Hong-Fu Zhang, Ji-Feng Ying State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, P.O. Box 9825, Beijing 100029, PR China Received 25 July 2005; received in revised form 27 March 2006; accepted 30 March 2006 Abstract Compositions of Cenozoic basalts from the Fansi (26.3–24.3 Ma), Xiyang–Pingding (7.9–7.3 Ma) and Zuoquan (∼5.6 Ma) volcanic fields in the Taihang Mountains provide insight into the nature of their mantle sources and evidence for asthenosphere– lithospheric mantle interaction beneath the North China Craton. These basalts are mainly alkaline (SiO2 =44–50 wt.%, Na2O+ K2O=3.9–6.0 wt.%) and have OIB-like characteristics, as shown in trace element distribution patterns, incompatible elemental (Ba/Nb=6–22, La/Nb=0.5–1.0, Ce/Pb=15–30, Nb/U=29–50) and isotopic ratios (87Sr/86Sr=0.7038–0.7054, 143Nd/ 144 Nd=0.5124–0.5129). Based on TiO2 contents, the Fansi lavas can be classified into two groups: high-Ti and low-Ti. The Fansi high-Ti and Xiyang–Pingding basalts were dominantly derived from an asthenospheric source, while the Zuoquan and Fansi low-Ti basalts show isotopic imprints (higher 87Sr/86Sr and lower 143Nd/144Nd ratios) compatible with some contributions of sub- continental lithospheric mantle. The variation in geochemical compositions of these basalts resulted from the low degree partial melting of asthenosphere and the interaction of asthenosphere-derived magma with old heterogeneous lithospheric mantle in an extensional regime, possibly related to the far effect of the India–Eurasia collision. -
Seismic Velocity Structure of the Continental Lithosphere from Controlled Source Data
Seismic Velocity Structure of the Continental Lithosphere from Controlled Source Data Walter D. Mooney US Geological Survey, Menlo Park, CA, USA Claus Prodehl University of Karlsruhe, Karlsruhe, Germany Nina I. Pavlenkova RAS Institute of the Physics of the Earth, Moscow, Russia 1. Introduction Year Authors Areas covered J/A/B a The purpose of this chapter is to provide a summary of the seismic velocity structure of the continental lithosphere, 1971 Heacock N-America B 1973 Meissner World J i.e., the crust and uppermost mantle. We define the crust as 1973 Mueller World B the outer layer of the Earth that is separated from the under- 1975 Makris E-Africa, Iceland A lying mantle by the Mohorovi6i6 discontinuity (Moho). We 1977 Bamford and Prodehl Europe, N-America J adopted the usual convention of defining the seismic Moho 1977 Heacock Europe, N-America B as the level in the Earth where the seismic compressional- 1977 Mueller Europe, N-America A 1977 Prodehl Europe, N-America A wave (P-wave) velocity increases rapidly or gradually to 1978 Mueller World A a value greater than or equal to 7.6 km sec -1 (Steinhart, 1967), 1980 Zverev and Kosminskaya Europe, Asia B defined in the data by the so-called "Pn" phase (P-normal). 1982 Soller et al. World J Here we use the term uppermost mantle to refer to the 50- 1984 Prodehl World A 200+ km thick lithospheric mantle that forms the root of the 1986 Meissner Continents B 1987 Orcutt Oceans J continents and that is attached to the crust (i.e., moves with the 1989 Mooney and Braile N-America A continental plates). -
The Distribution of Water in the Continental Lithospheric Mantle and Its Implications for the Stability of Continents
Invited Review Geology November 2013 Vol.58 No.32: 38793889 doi: 10.1007/s11434-013-5949-1 The distribution of water in the continental lithospheric mantle and its implications for the stability of continents XIA QunKe* & HAO YanTao CAS Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China Received January 14, 2013; accepted May 14, 2013; published online July 11, 2013 The lithospheric mantle is one of the key layers controlling the stability of continents. Even a small amount of water can influence many chemical and physical properties of rocks and minerals. Consequently, it is a pivotal task to study the distribution of water in the continental lithosphere. This paper presents a brief overview of the current state of knowledge about (1) the occurrence of water in the continental lithospheric mantle, (2) the spatial and temporal variations of the water content in the continental litho- spheric mantle, and (3) the relationship between water content and continent stability. Additionally, suggestions for future re- search directions are briefly discussed. water, nominally anhydrous minerals, continental lithospheric mantle, continent stability Citation: Xia Q K, Hao Y T. The distribution of water in the continental lithospheric mantle and its implications for the stability of continents. Chin Sci Bull, 2013, 58: 38793889, doi: 10.1007/s11434-013-5949-1 The lithospheric mantle is the lowermost part of continental continental lithospheric mantle is tightly related to its vis- plates; its viscosity contrast with the underlying astheno- cosity and stability [23,25–28]. -
MAPS CCP STACKS of P- & S-Wave RECEIVER
LITHOSPHERIC STRUCTURE BENEATH FENNOSCANDIA BASED ON P- AND S-WAVE CONTACT ME: RECEIVER FUNCTIONS [email protected] Anna Makushkina 1, Benoit Tauzin 1,2, Meghan Miller 1, Hans Thybo 3,4,5, and Hrvoje Tkalčić 1 1 Australian National University; 2 University of Lyon, Laboratoire de Géologie de Lyon; 3 CEED, University of Oslo; 4 Eurasia Institute of Earth Sciences, Istanbul Technical University; 5 China University of Geosciences, Wuhan, China, INTRODUCTION Fennoscandia consists of geologically distinct domains of Archaean, RESULTS: MAPS Moho MLD HVZ early and late Proterozoic and Phanerozoic age at the surface. A little is known about the interrelation of these domains at depth. Moho depth obtained by picking (left) SRF CCP images (background color) and (right) PRF Map of the Mid-lithospheric discontinuity Depths of the high-velocity zone CCP images with Moho depth (background) measurements from EUNAseis [1] (diamonds) Controlled-source experiments show potential expression of suture zones extending down to 100 km depth. SRF PRF Regional studies show evidence for the mid-lithospheric (MLD), 8-degree discontinuity or the lithosphere– asthenosphere boundary (LAB), that are markers of continent formation and evolution. But each study samples a small portion of Sketch of the expected discontinuities. Fennoscandia and does not provide a Red color indicates discontinuity with increase of velocity with depth, blue – Topography map (m); white circles are stations used comprehensive model for the whole decrease. MLD – mid-lithospheric in this study system [e.g. 2,3,4]. discontinuity; HVZ – high velocity zone; Our goal is to image structural differences of the upper mantle in 3 geological domains LVZ – low velocity zone; LAB – create a unified model of Fennoscandia. -
Plate Tectonics
Plate tectonics tive motion determines the type of boundary; convergent, divergent, or transform. Earthquakes, volcanic activity, mountain-building, and oceanic trench formation occur along these plate boundaries. The lateral relative move- ment of the plates typically varies from zero to 100 mm annually.[2] Tectonic plates are composed of oceanic lithosphere and thicker continental lithosphere, each topped by its own kind of crust. Along convergent boundaries, subduction carries plates into the mantle; the material lost is roughly balanced by the formation of new (oceanic) crust along divergent margins by seafloor spreading. In this way, the total surface of the globe remains the same. This predic- The tectonic plates of the world were mapped in the second half of the 20th century. tion of plate tectonics is also referred to as the conveyor belt principle. Earlier theories (that still have some sup- porters) propose gradual shrinking (contraction) or grad- ual expansion of the globe.[3] Tectonic plates are able to move because the Earth’s lithosphere has greater strength than the underlying asthenosphere. Lateral density variations in the mantle result in convection. Plate movement is thought to be driven by a combination of the motion of the seafloor away from the spreading ridge (due to variations in topog- raphy and density of the crust, which result in differences in gravitational forces) and drag, with downward suction, at the subduction zones. Another explanation lies in the different forces generated by the rotation of the globe and the tidal forces of the Sun and Moon. The relative im- portance of each of these factors and their relationship to each other is unclear, and still the subject of much debate. -
The Mid-Lithospheric Discontinuity Caused by Channel Flow in the Cratonic Lithosphere
The Mid-Lithospheric Discontinuity caused by channel flow in the cratonic lithosphere Haibin Yang *a, b, Irina M. Artemieva c,d,e, Hans Thybo e,f,g a. School of Earth Sciences, University of Melbourne, Melbourne, Australia b. Research School of Earth Sciences, Australian National University, Canberra, Australia c. Department of Geophysics, Stanford University, Stanford, CA 94305, USA d. Section of Oceanic Dynamics, GEOMAR Helmholtz Center for Ocean Research, Kiel 24148, Germany e. State Key Laboratory of Geological Processes and Mineral Resources, School of Earth Sciences, China University of Geosciences, Wuhan, China f. Eurasia Institute of Earth Science, Istanbul Technical University, Maslak, 34469 Istanbul, Turkey g. Centre for Earth Evolution and Dynamics (CEED), University of Oslo, Blindern, 0316 Oslo, Norway Corresponding author: Haibin Yang Email: [email protected] This is a non-peer reviewed preprint submitted to EarthArXiv. 1 Abstract 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. -
Origin and Evolution of Asthenospheric Layers
Two mechanisms of formation of asthenospheric layers L. Czechowski and M. Grad Institute of Geophysics, Faculty of Physics, University of Warsaw Ul. Pasteura 5, 02-093 Warszawa, Poland Phone: +48 22 5532003 E-mail: [email protected] Corresponding author: Leszek Czechowski: [email protected] The theory of plate tectonics describes some basic global tectonic processes as a result of motion of lithospheric plates. The boundary between lithosphere and asthenosphere (LAB) is defined by a difference in response to stress. Position of LAB is determined by: (i) the ratio (melting temperature)/( temperature) and (ii) an invariant of the stress tensor. We consider the role of these both factors for origin and decay of asthenosphere. We find that the asthenosphere of shear stress origin could be a transient, time-dependent feature. Key words: asthenosphere, evolution, LAB, origin of asthenosphere 1. Introduction The plate tectonics theory describes some of the basic tectonic processes on the Earth as motion of lithospheric plates. The plates are moved by large-scale thermal convection in the mantle. The lithosphere is mechanically resistant. Its thickness varies from ~50 to ~250 km. The lithosphere is underlain by the asthenosphere. The boundary between the lithosphere and the asthenosphere (LAB) is defined by a difference in response to stress: the asthenosphere deforms viscously. The bulk of asthenosphere is not melted (1), but at the deformation rate typical for the mantle convection (about 10-14 s-1) it behaves as a fluid with the viscosity η of about 5 1019 kg m-1 s-1. The mantle below has higher effective viscosity (e.g. -