The Deep Structure of Continents

Total Page:16

File Type:pdf, Size:1020Kb

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. In this casethe major differencesare above 250 km. it has been presumedthat coherent translation of both oceanic and continental plates takes place above some 200 km. This Okal and Anderson[1975] and Sipkin and Jordan [1976] basicassumption of plate tectonicsis contrary to the idea that studiedthe corereflected shear phase, ScS, with conflictingin- terpretations. Okal and Anderson concluded that all differ- ontinents have roots deeper than 400-500 km [MacDonald, 963; Jordan, 1975, 1979a, b]. ences could be explained in terms of known effects above Surfacewave studieshave shownthat there are large differ- --,180 km, while Sipkin and Jordan concludedthat differences races between oceans and shields above about 220 km [Dor- in velocity must persistto great depths,perhaps extending nan et al., 1960; Brune and Dorman, 1963; Anderson, 1967a; throughout the entire upper mantle. Okal [1977] concluded Kanamori, 1970; Dziewonski, 1971]. Recently, Cara [1979] has that surfacewave data, regionalizedto take accountof the age made a detailed study of regional differencesusing higher of the oceaniclithosphere, are incompatiblewith strong,deep mode surfacewaves. He found strong regional variations be- lateralinhomogeneity anddo notrequire any substantial structure variation below 240 km. tween the Pacific Ocean, western U.S., and eastern U.S. above 250 km and no resolvable difference below this depth. Eng- The ScS phase,of course,averages the velocity throughout the mantle and cannot resolve where the differences occur. land et al. [1978] made a direct comparisonof upper-mantle structure under the North Atlantic and Arctic oceans and the There are more direct ways to isolatethe effect.The velocity old shield of the Russianplatform. Even when maximum dif- structureof the upper mantle has been studiedin many re- ferencesbetween the regions were allowed the P wave data gionsby body wave and surface wave techniques. These stud- could be satisfiedby velocity modelswhich were substantially ies give remarkablyconsistent results when the averagetravel the samebelow 300 km. Cara's modelsare shownin Figure 1. times above 200 or 250 km are calculated.Table 1 presents these results. Shields are the fastest, about 3.5 s faster than Okal and Anderson [1975] used multiple ScS phases to samplethe earth under variousgeological provinces including youngocean. Oceanic models, on the average,are about 1.5-2 oceans and shields. They' concluded that the observations s slowerthan shields,but the differencedecreases with tl•e age of the ocean. were consistent with known differences above about 180 km. We have computed the differences between the $ wave There is therefore good agreement between the body wave and surfacewave data. Jordan [1975], however, proposedthat traveltimes above 200 km for the Rayleigh•ave models and ocean-continentdifferences extend deeper than 400 km and the Jeffreys-Bullenvalues. Figure 3 displaysthe computed ScS residuals for these oceanic and shield models as a func- that the region which translatescoherently in the course of plate tectonicsmay occupy the entire upper 700 km of the tion of crustal age. Measured residualsrelative to Jeffreys- Bullen, are alsoshown. It is clear that the ScStunes can be ex- mantle. This proposalhas reopenedthe questionof the deep structure of continents. plainedby known differences in the upper 200•250 km of the mantle. THE DEEP STRUCTURE OF CONTINENTS Theaverage one-way ScSresidual f•r 'ayerage age'ocean Prior to the recognitionthat attenuationwas important in (70-90 m.y.) is +0.8 s. This can be comparedwith the average interpreting free oscillationperiods, it was thought that aver- residualof +2.0 s for all oceanicdata combined,including the age earth shearvelocities were appreciablyslower than conti- very slow young oceans[Sipkin and Jordan, 1976].This latter value is a straightaverage of all data and ignoresthe variation Copyright¸ 1979 by the Americ.•nGeophysical Union. with age. Paper number 9B0991. 7555 0148-0227/79/009B-0991501.00 7 5 56 ANDERSON:DEEP STRUCTUREOF CONTINENTS Vs, km/sec TABLE 1. Upper Mantle Vertical Shear Wave Travel Times Above 4.0 4.5 5.0 200 and 250 km 0 Travel Time, s 200 km 250 km Reference ioo Shield 45.2 _+0.3 56.1 +_0.3 (1) • J/'%"EastU.S.- Continent 45.9 +_0.5 57.0 +_0.2 (2) 200 Ocean 46.7 _+0.4 57.7 +_0.3 (3) Minimum 49.2 60.6 (4) 15 m.y. 48.7 59.8 (5)* 70 m.y. 47.1 58.1 (5)* •00 100 m.y. 46.4 57.5 (5)* 150 m.y. 45.8 56.8 (5)* Maximum 46.0 57.2 (4) 400 • D• (1) •4nderson[1967a], •4ndersonand Harkrider [1968], Brune and Fig. 1. Shear velocity versusdepth for Pacific (average age, 90 Dorman [1963], }Vickens[1971], and Massb[1973]. m.y.) and easternU.S. from Cara [1979]. CANSD is Canadian shield (2) Helmbergerand Engen [1974],•4nderson and Julian [1969], Cara from Brune and Dorman [1963]. [19791. ' (3) •4nderson[1967a], Kanamori [19701,Schlue and Knopoff[1976], The residualsfor the oldestocean, > 120 m.y., are scattered, and N. R. Burkhard and D. D. Jackson (unpublished manuscript, 1979) (average ocean). but the mean is -0.7 s. This includesanomalously slow read- (4) Yoshida[1978]; minimum and maximum age groups. ings from the mid-Pacific mountains and the Bermuda Rise. (5) N. R. Burkhard and D. D. Jackson(unpublished manuscript, Therefore the one-way difference in travel times between 1979). shields and old oceans is about 1.3 s. The difference between *SV velocitiesfrom Rayleigh waves.Horizontally traveling SH averageocean and old ocean is about the sameas determined waves(Love waves) give travel times 1.6s (15 m.y.) to 0.5 s (150 m.y.) shorter.ScS waves should be comparedwith Rayleighwave, not Love by Duschenesand Solomon[1977] usingshear waves from Pa- wave,velocities. 'Average' ocean (--,70 m.y.) is about2 s slowerthan cific events. shield.If Love wavesare usedin the comparisonoceans would ap- From the raw ScS data the mean ocean-continent differen- pear to be about 3 s slow. tial time is + 1.5 + 2.8 s, about the same as the upper 250 km alone.Correcting for attenuationreduces the differentialtime sured shear wave velocities in the LVZ are 12-15% lower than slightly. The ScS shield data overlap the shield models,which the high-frequencyvelocities for mineralogiesin assemblages differ from the average earth only above 250 km, but average ranging from pyrolite to eclogite [Anderson,1977]. In addition about I s faster (Figure 3). to the temperatureeffect an additional severalpercent varia- From independent data (Table 1) the travel times above tion is allowed by variations in mineralogy. We take 12% as a 200-250 km in shieldsaverage 1.6 _+0.6 s faster than under plausible variation between shield and ocean mantles,take a average oceans and 0.9-2.0 s faster than 70-100 m.y. old travel time of 57 s above 250 km, and assume that velocities oceans.Therefore the ScS data are in good accord with the are the same at •250 km. This gives3.4 s as a conservativees- surfacewave studies,and it appearsthat all differencescan be timate of possible upper mantle shear wave vertical travel accommodated above 250 km. time variations. This would be the difference between a cold, The ScS data, when correctedfor crust and upper mantle garnet-rich upper mantle and a warm, relaxed, garnet-poor effects above 50 km, suggestthat the mantle under shields may be as much as about 3.4 s fasterthan under old oceans. +5 OC'E•NS At this point, it is instructive to estimate the maximum CONTINENTS plausiblevariations in the upper mantle.The shearvelocity in +z the low-velocity zone (LVZ) in oceansand tectonicregions is •,••yle•ghwaves about 10% lower than subcrustal velocities. This can be ac- c•+3 - \ - counted for by a difference in chemistryor by high-temper- --'+2 - ature stress relaxation mechanisms such as dislocation or grain boundary relaxation [Andersonand Minster, 1979}.Mea- a• -i- I - , \ - Sc \ +050 Average Earth OM2 I" -I •ELDS +025_[7 -2 - -3 I , \! I04 106 i08 109 -025 Age, yeors Fig. 3. ScS residuals (vemcal bars) as functio,• o! age of litho- sphere.Data are from Okal and Anderson[1975], Okal [1978a,b], and -O50 Sipkinand Jordan[1976].
Recommended publications
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Inge Lehmann: Discoverer of the Earth's Inner Core 2/4/17, 524 PM
    Inge Lehmann: Discoverer of the Earth's Inner Core 2/4/17, 524 PM Log In | Register Select Language​▼ Search Keywords or Topics GO SHARE: (http://www.facebook.com/sharer.php?u=http://www.amnh.org/explore/resource-collections/earth-inside-and-out/inge-lehmann-discoverer-of- the-earth-s-inner-core) Explore(http://twitter.com/intent/tweet? Inge Lehmann: Discoverer of the Earth's Inner text=Inge%20Lehmann%3A%20Discoverer%20of%20the%20Earth%27s%20Inner%20Core&url=http://www.amnh.org/explore/resource- collections/earth-inside-and-out/inge-lehmann-discoverer-of-the-earth-s-inner-core)Science Topics Core Kids Guide to the How can we find out what’s happening deep inside the Earth? Collect Museum The temperatures are too hot, pressures too extreme, and distances too vast to be explored by conventional probes. So Resource Collections scientists rely on seismic waves—shock waves generated by earthquakes and explosions that travel through Earth and Biodiversity Crisis across its surface—to reveal the structure of the interior of the Cosmic Horizons planet. Thousands of earthquakes occur every year, and each Earth Inside and one provides a fleeting glimpse of the Earth’s interior. Seismic Out signals consist of several kinds of waves. Those important for understanding the Earth’s interior are P-waves, (primary, or A Conversation compressional waves), and S-waves (secondary, or shear with Jacques waves), which travel through solid and liquid material in Malavieille different ways. Forecasting Earthquakes Using Paleoseismology The seismograph, which detects and records the movement of Dr. Inge Lehmann (1888-1993), seismic waves, was invented in 1880.
    [Show full text]
  • Anisotropic Shear-Wave Velocity Structure of the Earth's Mantle
    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 113, B06306, doi:10.1029/2007JB005169, 2008 Click Here for Full Article Anisotropic shear-wave velocity structure of the Earth’s mantle: A global model B. Kustowski,1,2 G. Ekstro¨m,3 and A. M. Dziewon´ski1 Received 12 May 2007; revised 8 February 2008; accepted 14 March 2008; published 25 June 2008. [1] We combine a new, large data set of surface wave phase anomalies, long-period waveforms, and body wave travel times to construct a three-dimensional model of the anisotropic shear wave velocity in the Earth’s mantle. Our modeling approach is improved and more comprehensive compared to our earlier studies and involves the development and implementation of a new spherically symmetric reference model, simultaneous inversion for velocity and anisotropy, as well as discontinuity topographies, and implementation of nonlinear crustal corrections for waveforms. A comparison of our new three-dimensional model, S362ANI, with two other models derived from comparable data sets but using different techniques reveals persistent features: (1) strong, 200-km-thick, high-velocity anomalies beneath cratons, likely representing the continental lithosphere, underlain by weaker, fast anomalies extending below 250 km, which may represent continental roots, (2) weak velocity heterogeneity between 250 and 400 km depths, (3) fast anomalies extending horizontally up to 2000–3000 km in the mantle transition zone beneath subduction zones, (4) lack of strong long-wavelength heterogeneity below 650 km suggesting inhibiting character of the upper mantle–lower mantle boundary, and (5) slow- velocity superplumes beneath the Pacific and Africa. The shear wave radial anisotropy is strongest at 120 km depth, in particular beneath the central Pacific.
    [Show full text]
  • Seismic and Electrical Signatures of the Lithosphere–Asthenosphere System of the Normal Oceanic Mantle
    EA45CH06-Kawakatsu ARI 14 August 2017 12:51 Annual Review of Earth and Planetary Sciences Seismic and Electrical Signatures of the Lithosphere–Asthenosphere System of the Normal Oceanic Mantle Hitoshi Kawakatsu and Hisashi Utada Earthquake Research Institute, The University of Tokyo, Tokyo 113-0032, Japan; email: [email protected] Annu. Rev. Earth Planet. Sci. 2017. 45:139–67 Keywords The Annual Review of Earth and Planetary Sciences is lithosphere, asthenosphere, Lid, low-velocity zone, G-discontinuity, plate online at earth.annualreviews.org tectonics, anisotropy, electrical conductivity https://doi.org/10.1146/annurev-earth-063016- 020319 Abstract Copyright c 2017 by Annual Reviews. Although plate tectonics started as a theory of the ocean basins nearly 50 years All rights reserved ago, the mechanical details of how it works are still poorly known. Our Annu. Rev. Earth Planet. Sci. 2017.45:139-167. Downloaded from www.annualreviews.org understanding of these details has been hampered partly by our inability to characterize the physical nature of the lithosphere–asthenosphere system ANNUAL (LAS) beneath the ocean. We review the existing observational constraints REVIEWS Further Click here to view this article's on the seismic and electrical properties of the LAS, particularly for normal Access provided by University of Tokyo - Library Earthquake Research Institute on 09/08/17. For personal use only. online features: oceanic regions away from mid-oceanic ridges, hot spots, and subduction • Download figures as PPT slides • Navigate linked references zones, where plate tectonics is expected to present its simplest form. Whereas • Download citations • Explore related articles a growing volume of seismic data on land has provided remarkable advances • Search keywords in large-scale pictures, seafloor observations have been shedding new light on essential details.
    [Show full text]
  • Earth's Internal Structure: a Seismologist's View
    Earth’s internal structure: a seismologist’s view Types of waves used by seismologists Organizing the information • Seismic travel times • Dispersion curves • Free oscillation frequencies Putting it all together Mantle 1-D seismic structure summary • Between 10-50 km have Mohorovicic discon;nuity – this marks the CRUST/ MANTLE boundary •At 50-200 km have a LOW VELOCITY ZONE – par;cularly under oceans and younger con;nents The crust Mohorovicic 1909 The lithosphere The asthenosphere Compositional interpretation of 1-D seismic profiles Seismic discontinuities and velocity gradients can arise from • A chemical change (e.g. the Moho) • A phase change (reorganisation of atoms into a different crystalline structure) The relative roles of phase changes and chemical changes provide a major challenge in interpreting seismology. Mantle 1-D seismic structure summary • Several seismological methods indicate a discon;nuity near 220 km depth. •Although present on PREM, it is now generally accepted not to be a global feature •Some;mes called the “Lehmann discon;nuity” aer Inge Lehmann NB: The 220-km Lehmann Discontinuity Not global in character! May reflect local anisotropy due to shearing of the asthenosphere i.e. a textural rather than chemical or phase change Mantle 1-D seismic structure summary • Between 410 and up to ~1000 km we are in the MANTLE TRANSITION ZONE • A number of sharp discon;nui;es separate regions of high velocity gradients •Main discon;nui;es are at 410 and 660 km. •660-discon;nuity widely taken as the UPPER MANTLE/LOWER MANTLE boundary The transition zone • Characterized by discontinuities in velocity and density models.
    [Show full text]
  • Mantle Flow and Melting Beneath Young Oceanic Lithosphere: Seismic
    MANTLE FLOW AND MELTING BENEATH YOUNG OCEANIC LITHOSPHERE: SEISMIC STUDIES OF THE GALÁPAGOS ARCHIPELAGO AND THE JUAN DE FUCA PLATE by JOSEPH STEPHEN BYRNES A DISSERTATION Presented to the Department of Earth Sciences and the Graduate School of the University of Oregon in partial fulfillment of the requirements for the degree of Doctor of Philosophy June 2017 DISSERTATION APPROVAL PAGE Student: Joseph Stephen Byrnes Title: Mantle Flow and Melting beneath Young Oceanic Lithosphere: Seismic Studies of the Galápagos Archipelago and the Juan de Fuca Plate This dissertation has been accepted and approved in partial fulfillment of the requirements for the Doctor of Philosophy degree in the Department of Earth Sciences by: Douglas Toomey Chairperson Emilie Hooft Core Member Eugene Humphreys Core Member Alan Rempel Core Member Allen Malony Institutional Representative and Scott L. Pratt Dean of the Graduate School Original approval signatures are on file with the University of Oregon Graduate School. Degree awarded June 2017 ii © 2017 Joseph Stephen Byrnes iii DISSERTATION ABSTRACT Joseph Stephen Byrnes Doctor of Philosophy Department of Earth Sciences June 2017 Title: Mantle Flow and Melting beneath Young Oceanic Lithosphere: Seismic Studies of the Galápagos Archipelago and the Juan de Fuca Plate In this dissertation, I use seismic imaging techniques to constrain the physical state of the upper mantle beneath regions of young oceanic lithosphere. Mantle convection is investigated beneath the Galápagos Archipelago and then beneath the Juan de Fuca (JdF) plate, with a focus on the JdF and Gorda Ridges before turning to the off-axis asthenosphere. In the Galápagos Archipelago, S-to-p receiver functions reveal a discontinuity in seismic velocity that is attributed to the dehydration of the upper mantle.
    [Show full text]
  • Kshamayaa Dharithri 1 (Oh Tolerant Mother Earth! Forgive Me)
    CHAPTER Kshamayaa Dharithri 1 (Oh Tolerant Mother Earth! Forgive Me) O’MY SILENT INNER VIBES (O’M S I V – 1) The mother Earth has greatest tolerance that she bears all our mistakes and misdeeds. She gives us everything such as minerals, food, shelter etc. But she can smash everything if we cross our limits. So,..... I bow to Mother Earth to save the mankind! I pray to mankind to save the mother Earth! Oh! Mother Earth... Forgive us and give us your blessings! Though ploughed through your belly, you fill our stomachs fully Though cared never gratefully, you fulfil our needs gracefully, I stand before Thee! Maa... with folded hands Forgive us and give us your blessings! Even when your body is split parts and parts, you never move apart Though made you victim of our party, But you never leave our party I kneel down! Maa... eyes filled with tears Forgive us and give us your blessings! Even if your heart’s ‘mine’ is broken, you give us gold and diamonds Even if garbage is thrown on you! You grab in your lap and garb us I lay down on thee! Maa... to prostrate with stretched hands Forgive us and give us your blessings! Despite being kicked always with our feet! Yet, you make us walk thousands and thousands of feet! Touching thy feet! Maa...I salute you with these words Forgive us and give us your blessings! Kshamayaa Dharithri! Rakshathu! Samrakshathu!! Parirakshathu!!! 1 2 Disaster Management: Hazard and Risk Awareness Namo Prithvee Matha! – Namo Prithvee Natha!! The God (Prithvee Nath) created PrithveePrithvee Matha, ‘The Earth’ as the most beautiful planet! No other planet has all the requisites for living-hood except the Earth.
    [Show full text]
  • Interior Parts of the Earth in Reference to Seismology
    INTERNAL STRUCTURE OF THE EARTH IN REFERENCE TO SEISMOLOGY SEISMILOGY • Disturbance within Earth's interior, which is in a constant state of movement, result in the release of energy in packets known as seismic waves. An area of geophysics known as seismology is the study of these waves and their effects, which often can be devastating when experienced in the form of earthquakes. The latter do not only take lives and destroy buildings, but they also produce secondary effects, most often in the form of a tsunami, or tidal wave. Using seismographs and seismometers, seismologists study earthquakes and other seismic phenomena, including volcanoes and even explosions resulting from nuclear testing. They measure earthquakes according to their magnitude or energy as well as their intensity or human impact. Seismology also is used to study Earth's interior, about which it has revealed a great deal. SEISMIC WAVES • When an earthquake occurs the seismic waves (P and S waves) spread out in all directions through the Earth's interior. Seismic stations located at increasing distances from the earthquake epicenter will record seismic waves that have traveled through increasing depths in the Earth. • Seismic velocities depend on the material properties such as composition, mineral phase and packing structure, temperature, and pressure of the media through which seismic waves pass. Seismic waves travel more quickly through denser materials and therefore generally travel more quickly with depth. Anomalously hot areas slow down seismic waves. Seismic waves move more slowly through a liquid than a solid. Molten areas within the Earth slow down P waves and stop S waves because their shearing motion cannot be transmitted through a liquid.
    [Show full text]
  • Oceanic Mantle Dynamics Implementation Plan: Report of a Community Workshop
    Oceanic Mantle Dynamics Implementation Plan: Report of a Community Workshop Snowbird, Utah September 18-20, 2002 Executive Summary and Workshop Recommendations The plate tectonics revolution in the earth sciences three decades ago provided a descriptive, or kinematic model for processes at the earth’s surface. The underlying mantle flow and dynamics behind this governing paradigm for the earth sciences have been far harder to elucidate. One of the greatest difficulties has been that seismic data, the primary imaging tool for the earth’s interior, have been collected primarily on the continents, while most of the earth’s interior lies beneath the sea floor. Recent advances in sea floor seismic instrumentation and geodynamic modeling, combined with constraints from other fields of geophysics and geochemistry, now provide unprecedented opportunities to understand the structure and circulation of the earth’s mantle. The advances require an integrated, interdisciplinary approach on a large scale, far beyond the planning and resources of individual investigators. Therefore a decade-long program in Oceanic Mantle Dynamics (OMD) is needed. This program will permit major advances in our understanding of every type of tectonic setting found in the ocean basins, will yield much higher resolution global imaging of the earth’s mantle, and in combination with continental USArray seismic data, will elucidate the great unanswered questions regarding the nature of the continent–ocean transition. A multidisciplinary approach centered around experiments made possible by a new generation of ocean-bottom seismometer (OBS) instrumentation could move beyond the kinematic revolution of plate tectonics towards testing and refining geodynamic models of mantle flow.
    [Show full text]
  • The Lehmann Discontinuity Due to Dehydration of Subducted Sediment Shigeaki Ono*,1,2
    The Open Mineralogy Journal, 2007, 1, 1-4 1 The Lehmann Discontinuity Due to Dehydration of Subducted Sediment Shigeaki Ono*,1,2 1Institute for Research on Earth Evolution, Japan Agency for Marine-Earth Science and Technology, 2-15 Natsushima-cho, Yokosuka-shi, Kanagawa 237-0061, Japan 2Department of Earth Sciences, University College London, Gower Street, London WC1E 6BT, UK Abstract: Recent high-pressure experiments have led to the conclusion that water release from subducted sediments lying under continents in subduction regions occurs at about 220 km depth. This dehydration reaction is in good agreement with the seismological signature of the discontinuity indicating that sediment dehydration causes the Lehmann discontinuity in the upper mantle. Keywords: Lehmann discontinuity, high pressure, water, dehydration, 220 km, sediment. 1. INTRODUCTION the upper mantle, whereas most observations are under con- tinents. It is therefore impossible to explain the local occur- The Lehmann discontinuity was first observed in Europe rence of the discontinuity using this concept. and North America from seismic refraction studies beneath continents [1, 2]. The discontinuity is characterized by the In the case of the silica phase transition, if the coesite- following features: (1) The depth of the seismic discontinuity stishovite transformation occurs at 220 km depth, the tem- is around 220 km depth. (2) A regionally varying negative perature of the upper mantle would be about 800 K; far too seismological Clapeyron slope (dP/dT) of the discontinuity low a typical temperature for this depth. Although both depth has been estimated [3]. (3) The discontinuity has not phase transitions have a positive Clapeyron slope, such a been detected everywhere at around 220 km depth [4].
    [Show full text]