9.06 Plate Tectonics Through Time N
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Assembly, Configuration, and Break-Up History of Rodinia
Author's personal copy Available online at www.sciencedirect.com Precambrian Research 160 (2008) 179–210 Assembly, configuration, and break-up history of Rodinia: A synthesis Z.X. Li a,g,∗, S.V. Bogdanova b, A.S. Collins c, A. Davidson d, B. De Waele a, R.E. Ernst e,f, I.C.W. Fitzsimons g, R.A. Fuck h, D.P. Gladkochub i, J. Jacobs j, K.E. Karlstrom k, S. Lu l, L.M. Natapov m, V. Pease n, S.A. Pisarevsky a, K. Thrane o, V. Vernikovsky p a Tectonics Special Research Centre, School of Earth and Geographical Sciences, The University of Western Australia, Crawley, WA 6009, Australia b Department of Geology, Lund University, Solvegatan 12, 223 62 Lund, Sweden c Continental Evolution Research Group, School of Earth and Environmental Sciences, University of Adelaide, Adelaide, SA 5005, Australia d Geological Survey of Canada (retired), 601 Booth Street, Ottawa, Canada K1A 0E8 e Ernst Geosciences, 43 Margrave Avenue, Ottawa, Canada K1T 3Y2 f Department of Earth Sciences, Carleton U., Ottawa, Canada K1S 5B6 g Tectonics Special Research Centre, Department of Applied Geology, Curtin University of Technology, GPO Box U1987, Perth, WA 6845, Australia h Universidade de Bras´ılia, 70910-000 Bras´ılia, Brazil i Institute of the Earth’s Crust SB RAS, Lermontova Street, 128, 664033 Irkutsk, Russia j Department of Earth Science, University of Bergen, Allegaten 41, N-5007 Bergen, Norway k Department of Earth and Planetary Sciences, Northrop Hall University of New Mexico, Albuquerque, NM 87131, USA l Tianjin Institute of Geology and Mineral Resources, CGS, No. -
Geophysics (3 Credits) Spring 2018
GEO 3010 – Geophysics (3 credits) Spring 2018 Lecture: FASB 250, 10:45-11:35 am, M & W Lab: FASB 250, 2:00-5:00 pm, M or W Instructor: Fan-Chi Lin (Assistant Professor, Dept. of Geology & Geophysics) Office: FASB 271 Phone: 801-581-4373 Email: [email protected] Office Hours: M, W 11:45 am - 1:00 pm. Please feel free to email me if you would like to make an appointment to meet at a different time. Teaching Assistants: Elizabeth Berg ([email protected]) FASB 288 Yadong Wang ([email protected]) FASB 288 Office Hours: T, H 1:00-3:00 pm Website: http://noise.earth.utah.edu/GEO3010/ Course Description: Prerequisite: MATH 1220 (Calculus II). Co-requisite: GEO 3080 (Earth Materials I). Recommended Prerequisite: PHYS 2220 (Phycs For Scien. & Eng. II). Fulfills Quantitative Intensive BS. Applications of physical principles to solid-earth dynamics and solid-earth structure, at both the scale of global tectonics and the smaller scale of subsurface exploration. Acquisition, modeling, and interpretation of seismic, gravity, magnetic, and electrical data in the context of exploration, geological engineering, and environmental problems. Two lectures, one lab weekly. 1. Policies Grades: Final grades are based on following weights: • Homework (25 %) • Labs (25 %) • Exam 1-3 (10% each) • Final (20 %) Homework: There will be approximately 6 homework sets. Homework must be turned in by 5 pm of the day they are due. 10 % will be marked off for each day they are late. Homework will not be accepted 3 days after the due day. Geophysics – GEO 3010 1 Labs: Do not miss labs! In general you will not have a chance to make up missed labs. -
1 John A. Tarduno
JOHN A. TARDUNO January, 2016 Professor of Geophysics Tel: 585-275-5713 Department of Earth and Environmental Sciences Fax: 585-244-5689 University of Rochester, Rochester, NY 14627 Email: [email protected] USA http://www.ees.rochester.edu/people/faculty/tarduno_john Academic Career: 2005-present Professor of Physics and Astronomy, University of Rochester, Rochester, NY. 2000-present Professor of Geophysics, University of Rochester, Rochester, NY. 1998-2006 Chair, Department of Earth and Environmental Sciences 1996 Associate Professor of Geophysics, University of Rochester, Rochester, NY. 1993 Assistant Professor of Geophysics, University of Rochester, Rochester, NY. 1990 Assistant Research Geophysicist, Scripps Institution of Oceanography, La Jolla, Ca. 1989 National Science Foundation Postdoctoral Fellow, ETH, Zürich, Switzerland 1988 JOI/USSAC Ocean Drilling Fellow, Stanford University, Stanford, Ca. 1987 Ph.D. (Geophysics), Stanford University, Stanford, Ca. 1987 M.S. (Geophysics) Stanford University, Stanford Ca. 1983 B.S. (Geophysics) Lehigh University, Bethlehem Pa. Honors and Awards: Phi Beta Kappa (1983) Fellow, Geological Society of America (1998) JOI/USSAC Distinguished Lecturer (2000-2001) Goergen Award for Distinguished Achievement and Artistry in Undergraduate Teaching (2001) Fellow, American Association for the Advancement of Science (2003) American Geophysical Union/Geomagnetism and Paleomagnetism Section Bullard Lecturer (2004) Fellow, John Simon Guggenheim Foundation (2006-2007) Edward Peck Curtis Award for -
Sediment Diagenesis
Sediment Diagenesis http://eps.mcgill.ca/~courses/c542/ SSdiedimen t Diagenes is Diagenesis refers to the sum of all the processes that bring about changes (e.g ., composition and texture) in a sediment or sedimentary rock subsequent to deposition in water. The processes may be physical, chemical, and/or biological in nature and may occur at any time subsequent to the arrival of a particle at the sediment‐water interface. The range of physical and chemical conditions included in diagenesis is 0 to 200oC, 1 to 2000 bars and water salinities from fresh water to concentrated brines. In fact, the range of diagenetic environments is potentially large and diagenesis can occur in any depositional or post‐depositional setting in which a sediment or rock may be placed by sedimentary or tectonic processes. This includes deep burial processes but excldludes more extensive hig h temperature or pressure metamorphic processes. Early diagenesis refers to changes occurring during burial up to a few hundred meters where elevated temperatures are not encountered (< 140oC) and where uplift above sea level does not occur, so that pore spaces of the sediment are continually filled with water. EElarly Diagenesi s 1. Physical effects: compaction. 2. Biological/physical/chemical influence of burrowing organisms: bioturbation and bioirrigation. 3. Formation of new minerals and modification of pre‐existing minerals. 4. Complete or partial dissolution of minerals. 5. Post‐depositional mobilization and migration of elements. 6. BtilBacterial ddtidegradation of organic matter. Physical effects and compaction (resulting from burial and overburden in the sediment column, most significant in fine-grained sediments – shale) Porosity = φ = volume of pore water/volume of total sediment EElarly Diagenesi s 1. -
Geophysical Methods Commonly Employed for Geotechnical Site Characterization TRANSPORTATION RESEARCH BOARD 2008 EXECUTIVE COMMITTEE OFFICERS
TRANSPORTATION RESEARCH Number E-C130 October 2008 Geophysical Methods Commonly Employed for Geotechnical Site Characterization TRANSPORTATION RESEARCH BOARD 2008 EXECUTIVE COMMITTEE OFFICERS Chair: Debra L. Miller, Secretary, Kansas Department of Transportation, Topeka Vice Chair: Adib K. Kanafani, Cahill Professor of Civil Engineering, University of California, Berkeley Division Chair for NRC Oversight: C. Michael Walton, Ernest H. Cockrell Centennial Chair in Engineering, University of Texas, Austin Executive Director: Robert E. Skinner, Jr., Transportation Research Board TRANSPORTATION RESEARCH BOARD 2008–2009 TECHNICAL ACTIVITIES COUNCIL Chair: Robert C. Johns, Director, Center for Transportation Studies, University of Minnesota, Minneapolis Technical Activities Director: Mark R. Norman, Transportation Research Board Paul H. Bingham, Principal, Global Insight, Inc., Washington, D.C., Freight Systems Group Chair Shelly R. Brown, Principal, Shelly Brown Associates, Seattle, Washington, Legal Resources Group Chair Cindy J. Burbank, National Planning and Environment Practice Leader, PB, Washington, D.C., Policy and Organization Group Chair James M. Crites, Executive Vice President, Operations, Dallas–Fort Worth International Airport, Texas, Aviation Group Chair Leanna Depue, Director, Highway Safety Division, Missouri Department of Transportation, Jefferson City, System Users Group Chair Arlene L. Dietz, A&C Dietz and Associates, LLC, Salem, Oregon, Marine Group Chair Robert M. Dorer, Acting Director, Office of Surface Transportation Programs, Volpe National Transportation Systems Center, Research and Innovative Technology Administration, Cambridge, Massachusetts, Rail Group Chair Karla H. Karash, Vice President, TranSystems Corporation, Medford, Massachusetts, Public Transportation Group Chair Mary Lou Ralls, Principal, Ralls Newman, LLC, Austin, Texas, Design and Construction Group Chair Katherine F. Turnbull, Associate Director, Texas Transportation Institute, Texas A&M University, College Station, Planning and Environment Group Chair Daniel S. -
Thomas Spring Thesis (PDF 7MB)
RECONSTRUCTION OF THE PHYSICAL VOLCANOLOGICAL PROCESSES AND PETROGENESIS OF THE 3.5GA WARRAWOONA GROUP PILLOW BASALT OF THE WARRALONG GREENSTONE BELT, PILBARA CRATON WESTERN AUSTRALIA Thomas Frederick David Spring Bachelor of Applied Science (Geology) Submitted in fulfilment of the requirements for the degree of Master of Applied Science (Geoscience) School of Earth, Environment and Biological Science Faculty of Science and Engineering Queensland University of Technology 2017 Abstract The formation of Earth’s continental crust initiated in the early Archean and has continued to the present day. In the early Archean, the Earth was substantially hotter than the present day leading to dramatically different tectonic processes. Early Archean tectonic processes have to be inferred from the rare well-preserved remnants of Archean crust. Models for the formation of Archean crust include large scale mantle melting associated with mantle plumes to generate thick basaltic to ultramafic crust. This crust than undergoes partial melting and internal differentiation to more felsic compositions. The Pilbara craton provides an ideal area for research into the Archean crust, with some of Earth oldest crust being preserved in relatively low strain and low metamorphosed greenstone belts. The volcanic cycles preserved in the greenstone belts of the Paleoarchean East Pilbara Terrane of the Pilbara craton represent the type example of plume-derived volcanism in the early Earth. Here I investigate the lithostratigraphy, volcanology and depositional environment of a volcanic and sedimentary succession ascribed to the Warrawoona group of the East Pilbara Supergroup from the Eastern Warralong Greenstone belt of the East Pilbara Terrane. In addition, I investigate the petrogenesis of well-preserved basaltic samples from the pillow basalt sequence ascribed to the Mt Ada Basalts in the study area. -
Geophysical Field Mapping
Presented at Short Course IX on Exploration for Geothermal Resources, organized by UNU-GTP, GDC and KenGen, at Lake Bogoria and Lake Naivasha, Kenya, Nov. 2-23, 2014. Kenya Electricity Generating Co., Ltd. GEOPHYSICAL FIELD MAPPING Anastasia W. Wanjohi, Kenya Electricity Generating Company Ltd. Olkaria Geothermal Project P.O. Box 785-20117, Naivasha KENYA [email protected] or [email protected] ABSTRACT Geophysics is the study of the earth by the quantitative observation of its physical properties. In geothermal geophysics, we measure the various parameters connected to geological structure and properties of geothermal systems. Geophysical field mapping is the process of selecting an area of interest and identifying all the geophysical aspects of the area with the purpose of preparing a detailed geophysical report. The objective of geophysical field work is to understand all physical parameters of a geothermal field and be able to relate them with geological phenomenons and come up with plausible inferences about the system. Four phases are involved and include planning/desktop studies, reconnaissance, actual data aquisition and report writing. Equipments must be prepared and calibrated well. Geophysical results should be processed, analysed and presented in the appropriate form. A detailed geophysical report should be compiled. This paper presents the reader with an overview of how to carry out geophysical mapping in a geothermal field. 1. INTRODUCTION Geophysics is the study of the earth by the quantitative observation of its physical properties. In geothermal geophysics, we measure the various parameters connected to geological structure and properties of geothermal systems. In lay man’s language, geophysics is all about x-raying the earth and involves sending signals into the earth and monitoring the outcome or monitoring natural signals from the earth. -
Mantle Flow Through the Northern Cordilleran Slab Window Revealed by Volcanic Geochemistry
Downloaded from geology.gsapubs.org on February 23, 2011 Mantle fl ow through the Northern Cordilleran slab window revealed by volcanic geochemistry Derek J. Thorkelson*, Julianne K. Madsen, and Christa L. Sluggett Department of Earth Sciences, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada ABSTRACT 180°W 135°W 90°W 45°W 0° The Northern Cordilleran slab window formed beneath west- ern Canada concurrently with the opening of the Californian slab N 60°N window beneath the southwestern United States, beginning in Late North Oligocene–Miocene time. A database of 3530 analyses from Miocene– American Holocene volcanoes along a 3500-km-long transect, from the north- Juan Vancouver Northern de ern Cascade Arc to the Aleutian Arc, was used to investigate mantle Cordilleran Fuca conditions in the Northern Cordilleran slab window. Using geochemi- Caribbean 30°N Californian Mexico Eurasian cal ratios sensitive to tectonic affi nity, such as Nb/Zr, we show that City and typical volcanic arc compositions in the Cascade and Aleutian sys- Central African American Cocos tems (derived from subduction-hydrated mantle) are separated by an Pacific 0° extensive volcanic fi eld with intraplate compositions (derived from La Paz relatively anhydrous mantle). This chemically defi ned region of intra- South Nazca American plate volcanism is spatially coincident with a geophysical model of 30°S the Northern Cordilleran slab window. We suggest that opening of Santiago the slab window triggered upwelling of anhydrous mantle and dis- Patagonian placement of the hydrous mantle wedge, which had developed during extensive early Cenozoic arc and backarc volcanism in western Can- Scotia Antarctic Antarctic 60°S ada. -
A Continuous Plate-Tectonic Model Using Geophysical Data to Estimate
GEOPHYSICAL JOURNAL INTERNATIONAL, 133, 379–389, 1998 1 A continuous plate-tectonic model using geophysical data to estimate plate margin widths, with a seismicity based example Caroline Dumoulin1, David Bercovici2, Pal˚ Wessel Department of Geology & Geophysics, School of Ocean and Earth Science and Technology, University of Hawaii, Honolulu, 96822, USA Summary A continuous kinematic model of present day plate motions is developed which 1) provides more realistic models of plate shapes than employed in the original work of Bercovici & Wessel [1994]; and 2) provides a means whereby geophysical data on intraplate deformation is used to estimate plate margin widths for all plates. A given plate’s shape function (which is unity within the plate, zero outside the plate) can be represented by analytic functions so long as the distance from a point inside the plate to the plate’s boundary can be expressed as a single valued function of azimuth (i.e., a single-valued polar function). To allow sufficient realism to the plate boundaries, without the excessive smoothing used by Bercovici and Wessel, the plates are divided along pseudoboundaries; the boundaries of plate sections are then simple enough to be modelled as single-valued polar functions. Moreover, the pseudoboundaries have little or no effect on the final results. The plate shape function for each plate also includes a plate margin function which can be constrained by geophysical data on intraplate deformation. We demonstrate how this margin function can be determined by using, as an example data set, the global seismicity distribution for shallow (depths less than 29km) earthquakes of magnitude greater than 4. -
The Reunification of Seismology and Geophysics Brad Artman Exploration Geophysics – a Brief History
The Reunification of Seismology and Geophysics Brad Artman Exploration geophysics – a brief history J.C. Karcher patents the reflection seismic method, focused the exploration geophysicist for the next century Beno Guttenberg becomes a professor of seismology Gas research institute, Teledyne Geotech, & Sandia National Labs develop equipment and techniques for microseismic monitoring to illuminate hydraulic fracturing 1920 1930 1940 1950 1960 1970 1980 1990 2000 2010 2013 Rapid advances in computational capabilities allow processing of ever-larger data volumes with more complete physics Exploration geophysics begins (re) learning earthquake seismology to commercialize microseismic monitoring Today, we have the opportunity to capitalize on the strengths of 100 yrs of development in both communities © Spectraseis Inc. 2013 2 Strength comparison To extract the full Seismology Geophysics potential from these Better sensors More sensors measurements, Better physics More compute horsepower we must capture the best of both Bigger events Smaller domain knowledge bases. Seismologists use cheap computers (grad. students) to do very thorough analysis on small numbers of traces. Geophysicists use cheap computers (clusters) to do good- enough approximations on very large numbers of traces. The merger of these fields is an historic opportunity to do exciting and valuable work © Spectraseis Inc. 2013 3 Agenda Sensor selection Survey design Processing algorithms and computer requirements Conclusions © Spectraseis Inc. 2013 4 Fracture mechanisms Compensated Linear Isotropic Double Couple Vector Dipole (explosion) (DC) (CLVD) P-waves only P- and S-waves P- and S-waves All fractures can be decomposed into these three mechanisms © Spectraseis Inc. 2013 5 DC radiation and particle motion Particle motion of P waves is compressional and in the same direction direction to the traveling wavefront. -
Part 629 – Glossary of Landform and Geologic Terms
Title 430 – National Soil Survey Handbook Part 629 – Glossary of Landform and Geologic Terms Subpart A – General Information 629.0 Definition and Purpose This glossary provides the NCSS soil survey program, soil scientists, and natural resource specialists with landform, geologic, and related terms and their definitions to— (1) Improve soil landscape description with a standard, single source landform and geologic glossary. (2) Enhance geomorphic content and clarity of soil map unit descriptions by use of accurate, defined terms. (3) Establish consistent geomorphic term usage in soil science and the National Cooperative Soil Survey (NCSS). (4) Provide standard geomorphic definitions for databases and soil survey technical publications. (5) Train soil scientists and related professionals in soils as landscape and geomorphic entities. 629.1 Responsibilities This glossary serves as the official NCSS reference for landform, geologic, and related terms. The staff of the National Soil Survey Center, located in Lincoln, NE, is responsible for maintaining and updating this glossary. Soil Science Division staff and NCSS participants are encouraged to propose additions and changes to the glossary for use in pedon descriptions, soil map unit descriptions, and soil survey publications. The Glossary of Geology (GG, 2005) serves as a major source for many glossary terms. The American Geologic Institute (AGI) granted the USDA Natural Resources Conservation Service (formerly the Soil Conservation Service) permission (in letters dated September 11, 1985, and September 22, 1993) to use existing definitions. Sources of, and modifications to, original definitions are explained immediately below. 629.2 Definitions A. Reference Codes Sources from which definitions were taken, whole or in part, are identified by a code (e.g., GG) following each definition. -
Sterngeryatctnphys18.Pdf
Tectonophysics 746 (2018) 173–198 Contents lists available at ScienceDirect Tectonophysics journal homepage: www.elsevier.com/locate/tecto Subduction initiation in nature and models: A review T ⁎ Robert J. Sterna, , Taras Geryab a Geosciences Dept., U Texas at Dallas, Richardson, TX 75080, USA b Institute of Geophysics, Dept. of Earth Sciences, ETH, Sonneggstrasse 5, 8092 Zurich, Switzerland ARTICLE INFO ABSTRACT Keywords: How new subduction zones form is an emerging field of scientific research with important implications for our Plate tectonics understanding of lithospheric strength, the driving force of plate tectonics, and Earth's tectonic history. We are Subduction making good progress towards understanding how new subduction zones form by combining field studies to Lithosphere identify candidates and reconstruct their timing and magmatic evolution and undertaking numerical modeling (informed by rheological constraints) to test hypotheses. Here, we review the state of the art by combining and comparing results coming from natural observations and numerical models of SI. Two modes of subduction initiation (SI) can be identified in both nature and models, spontaneous and induced. Induced SI occurs when pre-existing plate convergence causes a new subduction zone to form whereas spontaneous SI occurs without pre-existing plate motion when large lateral density contrasts occur across profound lithospheric weaknesses of various origin. We have good natural examples of 3 modes of subduction initiation, one type by induced nu- cleation of a subduction zone (polarity reversal) and two types of spontaneous nucleation of a subduction zone (transform collapse and plumehead margin collapse). In contrast, two proposed types of subduction initiation are not well supported by natural observations: (induced) transference and (spontaneous) passive margin collapse.