Interactions and Seismicity of Indian Tectonic Plate with Its Neighboring Plates: an Overview
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
India-Asia Collision and the Cenozoic Slowdown of the Indian Plate
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 115, B03410, doi:10.1029/2009JB006634, 2010 Click Here for Full Article India-Asia collision and the Cenozoic slowdown of the Indian plate: Implications for the forces driving plate motions Alex Copley,1 Jean-Philippe Avouac,1 and Jean-Yves Royer2 Received 21 May 2009; revised 12 August 2009; accepted 25 September 2009; published 17 March 2010. [1] The plate motion of India changed dramatically between 50 and 35 Ma, with the rate of convergence between India and Asia dropping from 15 to 4 cm/yr. This change is coincident with the onset of the India-Asia collision, and with a rearrangement of plate boundaries in the Indian Ocean. On the basis of a simple model for the forces exerted upon the edges of the plate and the tractions on the base of the plate, we perform force balance calculations for the precollision and postcollision configurations. We show that the observed Euler poles for the Indian plate are well explained in terms of their locations and magnitudes if (1) the resistive force induced by mountain building in the Himalaya-Tibet area is 5–6 Â 1012 N/m, (2) the net force exerted upon the Indian plate by subduction zones is similar in magnitude to the ridge-push force (2.5 Â 1012 N/m), and (3) basal tractions exert a resisting force that is linearly proportional to the plate velocity in the hot spot reference frame. The third point implies an asthenospheric viscosity of 2–5 Â 1019 Pa s, assuming a thickness of 100–150 km. -
Africa-Arabia-Eurasia Plate Interactions and Implications for the Dynamics of Mediterranean Subduction and Red Sea Rifting
This page added by the GeoPRISMS office. Africa-Arabia-Eurasia plate interactions and implications for the dynamics of Mediterranean subduction and Red Sea rifting Authors: R. Reilinger, B. Hager, L. Royden, C. Burchfiel, R. Van der Hilst Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA USA, [email protected], Tel: (617)253 -7860 This page added by the GeoPRISMS office. Our proposed GeoPRISMS Initiative is based on the premise that understanding the mechanics of plate motions (i.e., the force balance on the plates) is necessary to develop realistic models for plate interactions, including processes at subduction and extensional (rifting) plate boundaries. Important advances are being made with new geologic and geophysical techniques and observations that are providing fundamental insights into the dynamics of these plate tectonic processes. Our proposed research addresses directly the following questions identified in the GeoPRISMS SCD Draft Science Plan: 4.2 (How does deformation across the subduction plate boundary evolve in space and time, through the seismic cycle and beyond?), 4.6 (What are the physical and chemical conditions that control subduction zone initiation and the development of mature arc systems?), and 4.7 (What are the critical feedbacks between surface processes and subduction zone mechanics and dynamics?). It has long been recognized that the Greater Mediterranean region provides a natural laboratory to study a wide range of geodynamic processes (Figure 1) including ocean subduction and continent- continent collision (Hellenic arc, Arabia-Eurasia collision), lithospheric delamination (E Turkey High Plateau, Alboran Sea/High Atlas), back-arc extension (Mediterranean basins, including Alboran, Central Mediterranean, Aegean), “escape” tectonics and associated continental transform faulting (Anatolia, North and East Anatolian faults), and active continental and ocean rifting (East African and northern Red Sea rifting, central Red Sea and Gulf of Aden young ocean rifting). -
1 Introduction Gondwana
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Sydney eScholarship Regional plate tectonic reconstructions of the Indian Ocean Thesis Submitted in fulfilment of the requirements for the degree of Doctor of Philosophy Ana Gibbons School of Geosciences 2012 Supervised by Professor R. Dietmar Müller and Dr Joanne Whittaker The University of Sydney, PhD Thesis, Ana Gibbons, 2012 - Introduction DECLARATION I declare that this thesis contains less than 100,000 words and contains no work that has been submitted for a higher degree at any other university or institution. No animal or ethical approvals were applicable to this study. The use of any published written material or data has been duly acknowledged. Ana Gibbons ii The University of Sydney, PhD Thesis, Ana Gibbons, 2012 - Introduction ACKNOWLEDGEMENTS I would like to thank my supervisors for their endless encouragement, generosity, patience, and not least of all their expertise and ingenuity. I have thoroughly benefitted from working with them and cannot imagine a better supervisory team. I also thank Maria Seton, Carmen Gaina and Sabin Zahirovic for their help and encouragement. I thank Statoil (Norway), the Petroleum Exploration Society of Australia (PESA) and the School of Geosciences, University of Sydney for support. I am extremely grateful to Udo Barckhausen, Kaj Hoernle, Reinhard Werner, Paul Van Den Bogaard and all staff and crew of the CHRISP research cruise for a very informative and fun collaboration, which greatly refined this first chapter of this thesis. I also wish to thank Dr Yatheesh Vadakkeyakath from the National Institute of Oceanography, Goa, India, for his thorough review, which considerably improved the overall model and quality of the second chapter. -
The Central Asia Collision Zone: Numerical Modelling of the Lithospheric Structure and the Present-Day Kinematics
Th e Central Asia collision zone: numerical modelling of the lithospheric structure and the present - day kinematics Lavinia Tunini A questa tesi doctoral està subjecta a l a llicència Reconeixement - NoComercial – SenseObraDerivada 3.0. Espanya de Creative Commons . Esta tesis doctoral está sujeta a la licencia Reconocimiento - NoComercial – SinObraDerivada 3.0. España de Creative Commons . Th is doctoral thesis is license d under the Creative Commons Attribution - NonCommercial - NoDerivs 3.0. Spain License . The Central Asia collision zone: numerical modelling of the lithospheric structure and the present-day kinematics Ph.D. thesis presented at the Faculty of Geology of the University of Barcelona to obtain the Degree of Doctor in Earth Sciences Ph.D. student: Lavinia Tunini 1 Supervisors: Tutor: Dra. Ivone Jiménez-Munt 1 Prof. Dr. Juan José Ledo Fernández 2 Prof. Dr. Manel Fernàndez Ortiga 1 1 Institute of Earth Sciences Jaume Almera 2 Department of Geodynamics and Geophysics of the University of Barcelona This thesis has been prepared at the Institute of Earth Sciences Jaume Almera Consejo Superior de Investigaciones Científicas (CSIC) March 2015 Alla mia famiglia La natura non ha fretta, eppure tutto si realizza. – Lao Tzu Agradecimientos En mano tenéis un trabajo de casi 4 años, 173 páginas que no hubieran podido salir a luz sin el apoyo de quienes me han ayudado durante este camino, permitiendo acabar la Tesis antes que la Tesis acabase conmigo. En primer lugar quiero agradecer mis directores de tesis, Ivone Jiménez-Munt y Manel Fernàndez. Gracias por haberme dado la oportunidad de entrar en el proyecto ATIZA, de aprender de la modelización numérica, de participar a múltiples congresos y presentaciones, y, mientras, compartir unas cervezas. -
Tsunamigenic Earthquakes
Fifteen Years of (Major to Great) Tsunamigenic Earthquakes F Romano, S Lorito, and A Piatanesi, Istituto Nazionale di Geofisica e Vulcanologia, Roma, Italy T Lay, Earth and Planetary Sciences Department, University of California Santa Cruz, Santa Cruz, CA, United States © 2020 Elsevier Inc. All rights reserved. Tsunamis, Seismically Induced 1 Fifteen Years of Major to Great Tsunamigenic Earthquakes 3 The Study of Tsunamigenic Earthquakes 3 Megathrust Tsunamigenic Earthquakes 4 The Sunda 2004–10 Sequence in the Indian Ocean 4 Peru 2007 5 Maule 2010 5 Tohoku 2011 5 Santa Cruz 2013 6 Iquique 2014 6 Illapel 2015 6 Tsunamigenic Doublets 7 Kurils 2006–07 7 Samoa 2009 7 Tsunami Earthquakes 7 Java 2006 8 Mentawai 2010 8 Recent Special Cases 8 Sumatra 2012 8 Solomon 2007 8 Haida Gwaii 2012 9 Kaikoura 2016 9 Mexico 2017 9 Palu 2018 9 Conclusions 10 References 10 Further Reading 12 Tsunamis, Seismically Induced Tsunamis are a series of long gravity waves generated by the displacement of a significant volume of water that propagating in the sea, under the action of the gravity force, returns in its original equilibrium position. Differently from the common wind waves, tsunamis are characterized by large wavelengths (ranging from tens to hundreds of km) and long periods (ranging from minutes to hours). Several natural phenomena such as earthquakes, landslides, volcanic eruptions, the rapid change of atmospheric pressure (meteotsunami), or asteroids impacts can be the source of a tsunami; among these, the most frequent is represented by the earthquakes. Most of the very tsunamigenic earthquakes occur nearby the Earth convergent boundaries (Fig. -
Greater India Basin Hypothesis and a Two-Stage Cenozoic Collision Between India and Asia
Greater India Basin hypothesis and a two-stage Cenozoic collision between India and Asia Douwe J. J. van Hinsbergena,b,1, Peter C. Lippertc,d, Guillaume Dupont-Nivete,f,g, Nadine McQuarrieh, Pavel V. Doubrovinea,b, Wim Spakmani, and Trond H. Torsvika,b,j,k aPhysics of Geological Processes, University of Oslo, Sem Sælands vei 24, NO-0316 Oslo, Norway; bCenter for Advanced Study, Norwegian Academy of Science and Letters, Drammensveien 78, 0271 Oslo, Norway; cDepartment of Geosciences, University of Arizona, Tucson, AZ 85721; dDepartment of Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064; eGéosciences Rennes, Unité Mixte de Recherche 6118, Université de Rennes 1, Campus de Beaulieu, 35042 Rennes Cedex, France; fPaleomagnetic Laboratory Fort Hoofddijk, Department of Earth Sciences, University of Utrecht, Budapestlaan 17, 3584 CD, Utrecht, The Netherlands; gKey Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, Peking University, Beijing 100871, China; hDepartment of Geology and Planetary Science, University of Pittsburgh, Pittsburgh, PA 15260; iDepartment of Earth Sciences, University of Utrecht, Budapestlaan 4, 3584 CD, Utrecht, The Netherlands; jCenter for Geodynamics, Geological Survey of Norway, Leiv Eirikssons vei 39, 7491 Trondheim, Norway; and kSchool of Geosciences, University of the Witwatersrand, WITS 2050, Johannesburg, South Africa Edited by B. Clark Burchfiel, Massachusetts Institute of Technology, Cambridge, MA, and approved March 29, 2012 (received for review October 19, 2011) Cenozoic convergence between the Indian and Asian plates pro- (Fig. 2; SI Text) as well as with an abrupt decrease in India–Asia duced the archetypical continental collision zone comprising the convergence rates beginning at 55–50 Ma, as demonstrated by Himalaya mountain belt and the Tibetan Plateau. -
Himalaya - Southern-Tibet: the Typical Continent-Continent Collision Orogen
237 Himalaya - Southern-Tibet: the typical continent-continent collision orogen When an oceanic plate is subducted beneath a continental lithosphere, an Andean mountain range develops on the edge of the continent. If the subducting plate also contains some continental lithosphere, plate convergence eventually brings both continents into juxtaposition. While the oceanic lithosphere is relatively dense and sinks into the asthenosphere, the greater sialic content of the continental lithosphere ascribes positive buoyancy in the asthenosphere, which hinders the continental lithosphere to be subducted any great distance. Consequently, a continental lithosphere arriving at a trench will confront the overriding continent. Rapid relative convergence is halted and crustal shortening forms a collision mountain range. The plane marking the locus of collision is a suture, which usually preserves slivers of the oceanic lithosphere that formerly separated the continents, known as ophiolites. The collision between the Indian subcontinent and what is now Tibet began in the Eocene. It involved and still involves north-south convergence throughout southern Tibet and the Himalayas. This youthful mountain area is the type example for studies of continental collision processes. The Himalayas Location The Himalayas form a nearly 3000 km long, 250-350 km wide range between India to the south and the huge Tibetan plateau, with a mean elevation of 5000 m, to the north. The Himalayan mountain belt has a relatively simple, arcuate, and cylindrical geometry over most of its length and terminates at both ends in nearly transverse syntaxes, i.e. areas where orogenic structures turn sharply about a vertical axis. Both syntaxes are named after the main peaks that tower above them, the Namche Barwa (7756 m) to the east and the Nanga Parbat (8138 m) to the west, in Pakistan. -
Geological Evolution of the Red Sea: Historical Background, Review and Synthesis
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/277310102 Geological Evolution of the Red Sea: Historical Background, Review and Synthesis Chapter · January 2015 DOI: 10.1007/978-3-662-45201-1_3 CITATIONS READS 6 911 1 author: William Bosworth Apache Egypt Companies 70 PUBLICATIONS 2,954 CITATIONS SEE PROFILE Some of the authors of this publication are also working on these related projects: Near and Middle East and Eastern Africa: Tectonics, geodynamics, satellite gravimetry, magnetic (airborne and satellite), paleomagnetic reconstructions, thermics, seismics, seismology, 3D gravity- magnetic field modeling, GPS, different transformations and filtering, advanced integrated examination. View project Neotectonics of the Red Sea rift system View project All content following this page was uploaded by William Bosworth on 28 May 2015. The user has requested enhancement of the downloaded file. All in-text references underlined in blue are added to the original document and are linked to publications on ResearchGate, letting you access and read them immediately. Geological Evolution of the Red Sea: Historical Background, Review, and Synthesis William Bosworth Abstract The Red Sea is part of an extensive rift system that includes from south to north the oceanic Sheba Ridge, the Gulf of Aden, the Afar region, the Red Sea, the Gulf of Aqaba, the Gulf of Suez, and the Cairo basalt province. Historical interest in this area has stemmed from many causes with diverse objectives, but it is best known as a potential model for how continental lithosphere first ruptures and then evolves to oceanic spreading, a key segment of the Wilson cycle and plate tectonics. -
Late Paleozoic and Mesozoic Evolution of the Lhasa Terrane in the Xainza MARK Area of Southern Tibet
Tectonophysics 721 (2017) 415–434 Contents lists available at ScienceDirect Tectonophysics journal homepage: www.elsevier.com/locate/tecto Late Paleozoic and Mesozoic evolution of the Lhasa Terrane in the Xainza MARK area of southern Tibet ⁎ Suoya Fana,b, , Lin Dinga, Michael A. Murphyb, Wei Yaoa, An Yinc a Key Laboratory of Continental Collision and Plateau Uplift, Institute of Tibetan Plateau Research, Chinese Academy of Sciences, Beijing 100101, China b Department of Earth and Atmospheric Sciences, University of Houston, Houston, TX 77204, USA c Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095-1567, USA ARTICLE INFO ABSTRACT Keywords: Models for the Mesozoic growth of the Tibetan plateau describe closure of the Bangong Ocean resulting in Lhasa terrane accretion of the Lhasa terrane to the Qiangtang terrane along the Bangong-Nuijiang suture zone (BNSZ). Shortening However, a more complex history is suggested by studies of ophiolitic melanges south of the BNSZ “within” the Foreland basin Lhasa terrane. One such mélange belt is the Shiquanhe-Namu Co mélange zone (SNMZ) that is coincident with Suture zone the Geren Co-Namu Co thrust (GNT). To better understand the structure, age, and provenance of rocks exposed Provenance along the SNMZ we conducted geologic mapping, sandstone petrography, and U-Pb zircon geochronology of Geochronology rocks straddling the SNMZ. The GNT is north-directed and places Paleozoic strata against the Yongzhu ophiolite and Cretaceous strata along strike. A gabbro in the Yongzhu ophiolite yielded a U-Pb zircon age of 153 Ma. Detrital zircon age data from Permian rocks in the hanging wall suggests that the Lhasa terrane has affinity with the Himalaya and Qiangtang, rather than northwest Australia. -
Arabian Peninsula from Wikipedia, the Free Encyclopedia Jump to Navigationjump to Search "Arabia" and "Arabian" Redirect Here
Arabian Peninsula From Wikipedia, the free encyclopedia Jump to navigationJump to search "Arabia" and "Arabian" redirect here. For other uses, see Arabia (disambiguation) and Arabian (disambiguation). Arabian Peninsula Area 3.2 million km2 (1.25 million mi²) Population 77,983,936 Demonym Arabian Countries Saudi Arabia Yemen Oman United Arab Emirates Kuwait Qatar Bahrain -shibhu l-jazīrati l ِش ْبهُ ا ْل َج ِزي َرةِ ا ْلعَ َربِيَّة :The Arabian Peninsula, or simply Arabia[1] (/əˈreɪbiə/; Arabic jazīratu l-ʿarab, 'Island of the Arabs'),[2] is َج ِزي َرةُ ا ْلعَ َرب ʿarabiyyah, 'Arabian peninsula' or a peninsula of Western Asia situated northeast of Africa on the Arabian plate. From a geographical perspective, it is considered a subcontinent of Asia.[3] It is the largest peninsula in the world, at 3,237,500 km2 (1,250,000 sq mi).[4][5][6][7][8] The peninsula consists of the countries Yemen, Oman, Qatar, Bahrain, Kuwait, Saudi Arabia and the United Arab Emirates.[9] The peninsula formed as a result of the rifting of the Red Sea between 56 and 23 million years ago, and is bordered by the Red Sea to the west and southwest, the Persian Gulf to the northeast, the Levant to the north and the Indian Ocean to the southeast. The peninsula plays a critical geopolitical role in the Arab world due to its vast reserves of oil and natural gas. The most populous cities on the Arabian Peninsula are Riyadh, Dubai, Jeddah, Abu Dhabi, Doha, Kuwait City, Sanaʽa, and Mecca. Before the modern era, it was divided into four distinct regions: Red Sea Coast (Tihamah), Central Plateau (Al-Yamama), Indian Ocean Coast (Hadhramaut) and Persian Gulf Coast (Al-Bahrain). -
Cathaysia, Gondwanaland, and the Paleotethys in the Evolution of Continental Southeast Asia
GEOSEA V Proceedings Vol. !!, Ceo!. Soc. Malaysia, Bullelin20, August 1986; pp. 179-199 Cathaysia, Gondwanaland, and the Paleotethys in the evolution of continental Southeast Asia YURI G. GATINSKY1 AND CHARLES S. HUTCHISO 2 1All-Union Institute of Geology of Foreign Countries, Dimitrova, 7 Moscow, 109180, U.S.S.R. 2Department of Geology, University of Malaya, 59100 Kuala Lumpur, Malaysia . Abstract: Continental Southeast A ia is dominated by Precambrian continenral blocks overlain by Late Proterozoic to Paleozoic platform successions, representing Atlantic-type rifted miogeocl inal margins. All the blocks appear to have rifted and drifted from the Australian part of Gondwanaland. The timing and extent of their eparati on is analysed by the distribution of Penni an Cathaysian Gigamop leris and Gondwana Glossop1eris floras, assisted by dated tectono-structural units, paleoclimate indicators, and good quality paleomagnetic data. Between the blocks lie narrow intensely folded Phanerozoic mobile belts, which developed on the oceanic crust of the Paleotethys ocean, characterized by pelagic-turbidite flysch equences which shallowed as the oceans narrowed. The narrowing was effected by subduction resulting in island arcs within the oceans, and cordilleran volcano-plutonic arcs along the block margin . Extinction of the bas ins resulted in collision zones containing S-type granites and utu re zones containing dismembered ophi olites. Post-consolidation pl ate readju tments resulted in wrench and rift fa ulting in several places while convergence conti nued elsewhere. The tectonic analysis has been carried out by recognizing tectonic elements (structural-formati onal unit ~) for selected Phanerozoic time frame . We also pre ent a Phanerozoic sequence of palinspatic reconstructiors for the ri fti ng and drifting of the blocks from northern Australia. -
Tectonic Setting Seismic Hazard Epicentral Region Depth Profile
U.S. DEPARTMENT OF THE INTERIOR EARTHQUAKE SUMMARY MAP XXX U.S. GEOLOGICAL SURVEY Prepared in cooperation with the Global Seismographic Network e g M6.7 Sumbawa, Indoned sia, Earthquake of 8 November 2009 i R u a l a P - Tectonic Setting u Epicentral Region V I E T N A M P h i l i p p i n e h 100° 110° F a u l t 120° 130° s 110° 112° 114° 116° 118° 120° 122° 124° 126° 128° C A M B O D I A u S u m a t r a y P Palu K Balikpapan H Kalimantan 2000 1963 1923 P H I L I P P I N E S I L P h i l i p p i n e I A N D A M A N P Barat Kalimantan Timur Sumbawa Region P B a s i n Sulawesi Tengah Gulf I 1998 S E A N 10° 10° of S O U T H E 08 November 2009 8:41:44 UTC Thailand T 2° 2° C H I N A R Palangkaraya 1965 N E Kalimantan Tengah A N W H 1919 S E A A G C 8.315° S., 118.697° E. L U A O H P R Kalimantan Depth 18.3 km T Selatan M19w38 = 6.7 (1U94S8GS) SUNDA PLATE Sulawesi Bandjermasin Maluku Selatan B R U N E I 15 km (10 miles) 1N9N50W of Raba, Sumbawa, Indonesia M 310 km (1A9m0b moniles) ENE of Mataram, Lombok, Indonesia A C e l e b e s L Kendari 2001 A B a s i n 330 km (205 miles) W of Ende, Flores, Indonesia Y S u m a t r a F a u l t 4° 4° S A I N D O N E S I A 2004 I 1335 km (830 miles) E of JAKARTA, Java, Indonesia I S A Y A L A M S I N G A P O R E S u 0° m Borneo 0° Makassar 2006 1914 a MOLUCCA 2005 tr a SEA Enggano I N D O N E S IPLATEA BIRD'S HEAD A' 1797 PLATE 6° 6° 1950 1927 AUSTRALIA J a v a 1969 PLATE J A VA S E A 1998 Semarang 1934 1833 1996 1964 1995 BANDA SEA MAOKE Jawa 1966 Greater Sunda Islands B A N D A S E A 1990 1982 I PLATE PLATE