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On the Great Plume Debate of Geophysical Fluid Dynamics at Research School of Earth Sciences, the Australian National University
NEWS & VIEWS Chinese Science Bulletin 2005 Vol. 50 No. 15 1537—1540 2 About the authors Geoff F. Davies is currently a Senior Research Fellow On the great plume debate of Geophysical Fluid Dynamics at Research School of Earth Sciences, The Australian National University. He Yaoling Niu received a B.Sc. with honours (1966) and an M.Sc. (1968) Department of Earth Sciences, Durham University, Durham DH1 3LE, UK from Monash University in Australia, and a Ph.D. from (email: [email protected]) California Institute of Technology (Caltech) in the USA DOI: 10.1360/982005-1156 (1973). His PhD thesis dealt with mineral physics titled ‘Elasticity of solids at high temperatures and pressures: 1 Introductory note Theory, measurement and geophysical application’. He held positions at Harvard University, University of Roch- Geological processes are ultimately consequences of ester and Washington University in the USA before he Earth’s thermal evolution. Plate tectonic theory, which took his present post in 1983. He is an expert on mineral explains geological phenomena along plate boundaries, physics, very knowledgeable on geology and geochemis- elegantly illustrates this concept. For example, the origin try with deep interest in dynamics and evolution of the of oceanic plates at ocean ridges, the movement and earth's mantle: plate tectonics, mantle convection and growth of these plates, and their ultimate consumption chemical evolution. He is also interested in and researches back into the Earth’s deep interior through subduction on crust-mantle interaction, early Earth process and other zones provide an efficient mechanism to cool the earth’s planets. -
DON ANDERSON Themes Developed Across Several Decades
Don L. Anderson 1933–2014 A Biographical Memoir by Thorne Lay ©2016 National Academy of Sciences. Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. DON LYNN ANDERSON March 5, 1933–December 2, 2014 Elected to the NAS, 1982 Don L. Anderson, the Eleanor and John R. McMillan Professor of Geophysics at the California Institute of Tech- nology, was a geophysicist who made numerous seminal contributions to our understanding of Earth’s origin, composition, structure and evolution. He pioneered applications of seismic anisotropy for global surface waves, contributed to discovering the seismic velocity discontinuities in the mantle’s transition zone and initi- ated their mineralogical interpretation, established deep insights into seismic attenuation, co-authored the most widely used reference Earth structure model, helped to establish the field of global tomography, and re-opened inquiry into the nature of hotspot volcanism and mantle stratification. He contributed to initiatives that upgraded By Thorne Lay global and regional seismic instrumentation. He served as Director of the Caltech Seismological Laboratory for 22 years, overseeing a prolific scientific environment, distilling many advances into his masterpiece book Theory of the Earth. His enthusiasm for debate and his phenomenal editorial efforts raised the scientific standard of students and colleagues alike. Don was a geophysicist of tremendous breadth, publishing about 325 peer-reviewed research papers between 1958 and 2014 in seismology, mineral physics, planetary science, tectonophysics, petrology and geochemistry. He had a remarkable familiarity with the literature across all these disciplines, keeping reprints sorted into a multitude of three-ring binders that he could access in an instant, uniquely positioning him to undertake the writing of his ambitious book, The Theory of the Earth, published in 1989. -
The Hawaiian SWELL Pilot Experiment—Evidence for Lithosphere Rejuvenation from Ocean Bottom Surface Wave Data
The Geological Society of America Special Paper 430 2007 The Hawaiian SWELL pilot experiment—Evidence for lithosphere rejuvenation from ocean bottom surface wave data Gabi Laske Cecil H. and Ida M. Green Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California San Diego, 9500 Gilman Drive, La Jolla, California 92093-0225, USA Jason Phipps Morgan Department of Earth & Atmospheric Sciences, Snee Hall, Cornell University, Ithaca, New York, 14853-1504 John A. Orcutt Cecil H. and Ida M. Green Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California San Diego, 9500 Gilman Drive, La Jolla, California 92093-0225, USA ABSTRACT During the roughly year-long Seismic Wave Exploration in the Lower Lithosphere (SWELL) pilot experiment in 1997/1998, eight ocean bottom instruments deployed to the southwest of the Hawaiian Islands recorded teleseismic Rayleigh waves with peri- ods between 15 and 70 s. Such data are capable of resolving structural variations in the oceanic lithosphere and upper asthenosphere and therefore help understand the mechanism that supports the Hawaiian Swell relief. The pilot experiment was a tech- nical as well as a scientific feasibility study and consisted of a hexagonal array of Scripps Low-Cost Hardware for Earth Applications and Physical Oceanography (L-CHEAPO) instruments using differential pressure sensors. The analysis of eighty- four earthquakes provided numerous high-precision phase velocity curves over an un- precedentedly wide period range. We find a rather uniform (unaltered) lid at the top of the lithosphere that is underlain by a strongly heterogeneous lower lithosphere and upper asthenosphere. Strong slow anomalies appear within ~300 km of the island chain and indicate that the lithosphere has most likely been altered by the same process that causes the Hawaiian volcanism. -
Fixity of the Iceland “Hotspot” on the Mid-Atlantic Ridge: Observational Evidence, Mechanisms, and Implications for Atlantic Volcanic Margins
Geological Society of America Special Paper 388 2005 Fixity of the Iceland “hotspot” on the Mid-Atlantic Ridge: Observational evidence, mechanisms, and implications for Atlantic volcanic margins Erik R. Lundin* Geological Survey of Norway, Leiv Erikssons vei 39, 7491 Trondheim, Norway Anthony G. Doré* Statoil UK Ltd., Statoil House, 11a Regent Street, London SW1Y 4ST, UK ABSTRACT The Iceland anomaly has been attributed to a deeply rooted and fixed mantle plume, and Early Tertiary magmatism in the North Atlantic Igneous Province (NAIP) has commonly been interpreted to relate to an ancient expression of the same plume. We challenge these concepts. A major problem with attributing the Iceland anomaly to a fixed plume is the lack of evidence for a hotspot track. Although the Greenland- Faeroe Ridge has been suggested to be the hotspot track, its symmetric and continuous construction instead suggests in situ development on the plate boundary. Magmatism in the NAIP occurred in two phases, distributed in approximately perpendicular belts. The first phase (ca. 62–58 Ma) occurred along a north-west belt through the British Volcanic Province to west Greenland. We relate this phase to a transient and failed rift, intermediate in time and space between seafloor spreading in the Labrador Sea and the northeast Atlantic. The second phase (ca. 56–53 Ma) followed the incipient north- east Atlantic plate boundary. Both magmatic phases can therefore be associated with plate tectonics. Likewise, the north Atlantic–Arctic breakup can be explained as a nat- ural outcome of plate tectonics and lithospheric strength distribution. We follow other recent research in suggesting that the voluminous magmatism during NAIP phase 2 is related to reactivation and opening along the Caledonian orogen. -
Technical Sessions
Technical Sessions Meeting policy prohibits the use of cameras A no-smoking policy has been established by the AM or sound-recording equipment at technical Program Committee and will be followed in all sessions and poster sessions. meeting rooms for technical sessions. NOTICE In the interest of public information, the Geological Society of America provides a forum for the presentation of diverse opinions and positions. The opinions (views) expressed by speakers and exhibitors at these sessions are their own and do not necessarily represent the views or policies of the Geological Society of America. SUNDAY NOTE INDEX SYSTEM * INDUSTRY TRACKS Numbers (3-4, 15-4) indicate session and Look for these icons to identify sessions relevant to applied order of presentation within that session. geoscientists: *denotes speaker Economic Geology Energy Engineering Geology Hydrogeology and Environmental Geology SUNDAY, 22 SEPTEMBER 2019 THE CAMBRIAN AND ORDOVICIAN RADIATION OF MORNING ECHINODERMS ORAL TECHNICAL SESSIONS 1-7 9:30 AM Blake, Daniel B.*; Gahn, Forest J.; Guensburg, Thomas E.: AN EARLY ORDOVICIAN (FLOIAN) ASTEROZOAN SESSION NO. 1 (ECHINODERMATA) OF PROBLEMATIC CLASS-LEVEL AFFINITIES D19. Paleontology: Invertebrate Paleobiology 1-8 9:45 AM Sumrall, Colin D.*; Botting, Joseph P.: THE OLDEST 8:00 AM, Phoenix Convention Center, Room 227ABC, North Building RECORD OF RHENOPYRGID EDRIOASTEROIDS, FROM Brandt M. Gibson and Katherine Turk, Presiding THE EARLY ORDOVICIAN FEZOUATA FORMATION OF 1-1 8:00 AM O’Neil, Gretchen R.*; Tackett, Lydia S.: PRESERVATIONAL -
Potential Effects of Hydrothermal Circulation and Magmatism on Heatflow at Hotspot Swells
The Geological Society of America Special Paper 430 2007 Potential effects of hydrothermal circulation and magmatism on heatflow at hotspot swells Carol A. Stein* Department of Earth and Environmental Sciences, University of Illinois at Chicago, 845 West Taylor Street, Chicago, Illinois 60607-7059, USA Richard P. Von Herzen* Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Clark 244B, MS#22, Woods Hole, Massachusetts 02543, USA, and Department of Earth Sciences, University of California at Santa Cruz, Earth and Marine Science Building, Santa Cruz, California 95064-1077, USA ABSTRACT The lack of high heatflow values at hotspots has been interpreted as showing that the mechanism forming the associated swells is not reheating of the lower half of oceanic lithosphere. Alternatively, it has recently been proposed that the hotspot sur- face heatflow signature is obscured by fluid circulation. We re-examine closely spaced heatflow measurements near the Hawaii, Réunion, Crozet, Cape Verde, and Bermuda hotspots. We conclude that hydrothermal circulation may redistribute heat near the swell axes, but it does not mask a large and spatially broad heatflow anomaly. There may, however, be heatflow perturbations associated with the cooling of igneous intru- sions emplaced during hotspot formation. Although such effects may raise heatflow at a few sites, the small heatflow anomalies indicate that the mechanisms producing hotspots do not significantly perturb the thermal state of the lithosphere. Keywords: heatflow, swell, hotspot, mantle plume INTRODUCTION anomalies at hotspots (e.g., Crough, 1978). A consequence of this mechanism is unusually high surface heatflow, which After the recognition that hotspots, regions of excess vol- should be measurable by established methodologies. -
Mantle Plumes from Top to Bottom
Earth-Science Reviews 77 (2006) 231–271 www.elsevier.com/locate/earscirev Mantle plumes from top to bottom Norman H. Sleep Department of Geophysics, Stanford University, Stanford, California 94305, USA Received 24 March 2005; accepted 20 March 2006 Available online 23 May 2006 Abstract Hotspots include midplate features like Hawaii and on-axis features like Iceland. Mantle plumes are a well-posed hypothesis for their formation. Starting plume heads provide an explanation of brief episodes of flood basalts, mafic intrusions, and radial dike swarms. Yet the essence of the hypothesis hides deep in the mantle. Tests independent of surface geology and geochemistry to date have been at best tantalizing. It is productive to bare the current ignorance, rather than to dump the plume hypothesis. One finds potentially fruitful lines of inquiry using simple dynamics and observations. Ancient lithospheric xenoliths may reveal heating by plumes and subsequent thermal equilibration in the past. The effect at the base of the chemical layer is modest 50–100 K for transient heating by plume heads. Thinning of nonbuoyant platform lithosphere is readily observed but not directly attributable to plumes. The plume history in Antarctica is ill constrained because of poor geological exposure. This locality provides a worst case on what is known about surface evidence of hotspots. Direct detection of plume tail conduits in the mid-mantle is now at the edge of seismic resolution. Seismology does not provide adequate resolution of the deep mantle. We do not know the extent of a chemically dense dregs layer or whether superplume regions are cooler or hotter than an adiabat in equilibrium with the asthenosphere. -
Are 'Hot Spots'
(This is a sample cover image for this issue. The actual cover is not yet available at this time.) This article appeared in a journal published by Elsevier. The attached copy is furnished to the author for internal non-commercial research and education use, including for instruction at the authors institution and sharing with colleagues. Other uses, including reproduction and distribution, or selling or licensing copies, or posting to personal, institutional or third party websites are prohibited. In most cases authors are permitted to post their version of the article (e.g. in Word or Tex form) to their personal website or institutional repository. Authors requiring further information regarding Elsevier’s archiving and manuscript policies are encouraged to visit: http://www.elsevier.com/copyright Author's personal copy Journal of Geodynamics 58 (2012) 1–28 Contents lists available at SciVerse ScienceDirect Journal of Geodynamics j ournal homepage: http://www.elsevier.com/locate/jog Review Are ‘hot spots’ hot spots? Gillian R. Foulger Department of Earth Sciences, University of Durham, Science Laboratories, South Rd., Durham DH1 3LE, UK a r t i c l e i n f o a b s t r a c t Article history: The term ‘hot spot’ emerged in the 1960s from speculations that Hawaii might have its origins in an Received 12 May 2011 unusually hot source region in the mantle. It subsequently became widely used to refer to volcanic regions Received in revised form considered to be anomalous in the then-new plate tectonic paradigm. It carried with it the implication 21 December 2011 that volcanism (a) is emplaced by a single, spatially restricted, mongenetic melt-delivery system, assumed Accepted 21 December 2011 to be a mantle plume, and (b) that the source is unusually hot. -
Mantle Reflectivity Structure Beneath Oceanic Hotspots
Geophys. J. Int. (2009) 178, 1456–1472 doi: 10.1111/j.1365-246X.2009.04242.x Mantle reflectivity structure beneath oceanic hotspots Yu Jeffrey Gu,1 Yuling An,1 Mauricio Sacchi,1 Ryan Schultz1 and Jeroen Ritsema2 1Department of Physics, University of Alberta, Edmonton, AB T6G 2G7, Canada. E-mail: [email protected] 2Department of Geological Sciences, University of Michigan, Ann Arbor, MI 48109, USA Accepted 2009 May 6. Received 2009 May 4; in original form 2008 November 30 SUMMARY This study applies high-resolution Radon transform to a large set of SS precursors and explores the mantle reflectivity structure beneath 17 potentially ‘deep-rooted’ hotspots. The combined reduced time (τ) and ray parameter (p) information effectively constrains the depth, spatial distribution and sharpness of upper-/mid-mantle reflectors. The olivine to wadsleyite phase boundary is deeper than the ocean and global averages and produces a dominant τ –p domain signal. Laterally coherent observations of the deep 410-km seismic discontinuity, thin upper mantle transition zone and weak/absent 520-km reflector beneath hotspots make compelling arguments for large-scale, hot thermal anomalies in the top 400–600 km of the mantle. On the other hand, a relatively ‘flat’ and weak reflector at ∼653 km is inconsistent with ringwoodite to silicate perovskite + magnesiowustite¨ transformation at temperatures greater than 2000 K. The lack of a negative correlation between topography and temperature implies (1) average or below-average temperatures at 600–700 km depths or (2) high temperatures and a dominating majorite garnet to Ca perovskite phase transformation. The proper choice between these two scenarios will directly impact the origin and depth of mantle plumes beneath hotspots.