Isostasy, Flexure, and Dynamic Topography
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Geophysical Abstracts 156-159 January-December 1954
Geophysical Abstracts 156-159 January-December 1954 GEOLOGICAL SURVEY BULLETIN 1022 Abstracts of current literature pertaining to the physics of the solid earth and geophysicq,l exploration UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1955 UNITED STATESlDEPARTMENT OF THE INTERIOR Douglas McKay, Secretary GEOLOGICAL SURVEY W. ~· Wrather, Director CONTENTS [The letters in parentheses are those used to designate the chapters for separate publication] Page (A) Geophysical Abstracts 156, January-March------------------------ 1 (B) Geophysical Abstracts 157, April-June---------------------------- 71 (C) Geophysical Abstracts 158, July-September________________________ 135 (D) Geophysical Abstracts 159, October-December_____________________ 205 Under department orders, Geophysical Abstracts have been published at different times by the Bureau of Mines or the Geological Survey as noted below: 1-86, May 1929-June· 1936, Bureau of Mines Information Circulars. [Mimeo- graphed] 87, July-December 1936, Geological Survey Bulletin 887. 88-91, January-December 1937, Geological Survey Bulletin 895. 92-95, January-December 1938, Geological Survey Bulletin 909. 96-99, January-December 1939, Geological Survey Bulletin 915. 100-103, January-December 1940, Geological Survey Bulletin 925. 104-107, January-December 1941, Geological Survey Bulletin 932. 108-111, January-December 1942, Geological Survey Bulletin 939. 112-127, January 1943-December 1946, Bureau of Mines Information Circulars. [Mimeographed] 128-131, January-December 1947, Geological Survey Bulletin 957. 132-135, January-December 1948, Geological Survey Bulletin 959. 136-139, January-December 1949, Geological Survey Bulletin 966. 140-143, January-December 1950, Geological Survey Bulletin 976. 144-147, January-December 1951, Geological Survey Bulletin 981. 148-151, January-December 1952, Geological Survey Bulletin 991. 152-155, January-December 1953, Geological Survey Bulletin 1002. -
Oceanic Residual Depth Measurements, the Plate Cooling 10.1002/2016JB013457 Model, and Global Dynamic Topography
Journal of Geophysical Research: Solid Earth RESEARCH ARTICLE Oceanic residual depth measurements, the plate cooling 10.1002/2016JB013457 model, and global dynamic topography Key Points: • 1936 academic and industrial Mark J. Hoggard1 , Jeff Winterbourne2 , Karol Czarnota3, and Nicky White1 seismic surveys from oceanic crust have been analyzed 1Department of Earth Sciences, Bullard Laboratories, Cambridge, UK, 2BP Exploration Operating Co. Ltd, Middlesex, UK, • Oceanic residual depth anomalies 3 have wavelengths of thousands of Geoscience Australia, Canberra, ACT, Australia kilometers and amplitudes of ±1km • Correlation with gravity anomalies, magmatism, and seismic tomography Abstract Convective circulation of the mantle causes deflections of the Earth’s surface that vary as imply convective origin a function of space and time. Accurate measurements of this dynamic topography are complicated by the need to isolate and remove other sources of elevation, arising from flexure and lithospheric isostasy. Supporting Information: The complex architecture of continental lithosphere means that measurement of present-day dynamic • Supporting Information S1 topography is more straightforward in the oceanic realm. Here we present an updated methodology for •DataSetS1 calculating oceanic residual bathymetry, which is a proxy for dynamic topography. Corrections are applied •DataSetS2 •DataSetS3 that account for the effects of sedimentary loading and compaction, for anomalous crustal thickness •DataSetS4 variations, for subsidence of oceanic lithosphere as a function of age and for non-hydrostatic geoid •DataSetS5 height variations. Errors are formally propagated to estimate measurement uncertainties. We apply this •DataSetS6 •DataSetS7 methodology to a global database of 1936 seismic surveys located on oceanic crust and generate 2297 spot •DataSetS8 measurements of residual topography, including 1161 with crustal corrections. -
The Nature of Lunar Isostasy
45th Lunar and Planetary Science Conference (2014) 1630.pdf THE NATURE OF LUNAR ISOSTASY. Michael M. Sori1 and Maria T. Zuber1. 1Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA ([email protected]). Introduction: One way planetary topography can A key assumption in investigating the role of Pratt be supported is isostatic compensation, in which isostasy by looking at the relationship between crustal overburden pressure of rock is balanced at some depth. density and topography is that the density one observes The regions of the Moon that are not associated with near the surface is representative of the underlying maria or basins are generally isostatically compensated crustal column. We justify that assumption here by [1], an observation that was made when the first noting that calculation of the effective density of the detailed lunar gravity maps were constructed [2] and lunar crust as a function of spherical harmonic degree has held with each subsequently more precise data set considered results in a linear trend [14], supporting the [e.g., 3]. notion of a single-layer crust. There are two models of isostasy commonly Results: We make scatter plots of crustal density considered. In the Airy isostasy model [4], crustal as a function of elevation. One such scatter plot, for thickness is varied such that overburden pressures are the South Pole-Aitken basin, is shown in Figure 1. equal at some depth of compensation. The crust is a Points are sampled in a grid every ~8 km. For each layer of uniform density overlaying a mantle of higher scatter plot, we make a least-squared fit to the data and uniform density. -
Glacial Isostatic Adjustment and Sea-Level Change – State of the Art Report Technical Report TR-09-11
Glacial isostatic adjustment and sea-level change – State of the art report Glacial isostatic adjustment and sea-level change Technical Report TR-09-11 Glacial isostatic adjustment and sea-level change State of the art report Pippa Whitehouse, Durham University April 2009 Svensk Kärnbränslehantering AB Swedish Nuclear Fuel and Waste Management Co Box 250, SE-101 24 Stockholm Phone +46 8 459 84 00 TR-09-11 ISSN 1404-0344 CM Gruppen AB, Bromma, 2009 Tänd ett lager: P, R eller TR. Glacial isostatic adjustment and sea-level change State of the art report Pippa Whitehouse, Durham University April 2009 This report concerns a study which was conducted for SKB. The conclusions and viewpoints presented in the report are those of the author and do not necessarily coincide with those of the client. A pdf version of this document can be downloaded from www.skb.se. Preface This document contains information on the process of glacial isostatic adjustment (GIA) and how this affects sea-level and shore-line displacement, and the methods which are employed by researchers to study and understand these processes. The information will be used in e.g. the report “Climate and climate-related issues for the safety assessment SR-Site”. Stockholm, April 2009 Jens-Ove Näslund Person in charge of the SKB climate programme Contents 1 Introduction 7 1.1 Structure and purpose of this report 7 1.2 A brief introduction to GIA 7 1.2.1 Overview/general description 7 1.2.2 Governing factors 8 1.2.3 Observations of glacial isostatic adjustment 9 1.2.4 Time scales 9 2 Glacial -
Eroding Dynamic Topography J Braun, X Robert, T Simon-Labric
Eroding dynamic topography J Braun, X Robert, T Simon-Labric To cite this version: J Braun, X Robert, T Simon-Labric. Eroding dynamic topography. Geophysical Research Letters, American Geophysical Union, 2013, 40 (8), pp.1494 - 1499. 10.1002/grl.50310. hal-03135812 HAL Id: hal-03135812 https://hal.archives-ouvertes.fr/hal-03135812 Submitted on 9 Feb 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. GEOPHYSICAL RESEARCH LETTERS, VOL. 40, 1–6, doi:10.1002/grl.50310, 2013 Eroding dynamic topography J. Braun,1 X. Robert,1 and T. Simon-Labric1 Received 10 January 2013; revised 28 February 2013; accepted 28 February 2013. [1] Geological observations of mantle flow-driven dynamic perturbation to oceanic circulation [Poore and White, 2011], topography are numerous, especially in the stratigraphy large scale continental drainage reorganizations [Shephard of sedimentary basins; on the contrary, when it leads et al., 2010] or the formation of major geomorphic features to subaerial exposure of rocks, dynamic topography must such as the Grand Canyon [Karlstrom et al., 2008]. be substantially eroded to leave a noticeable trace in the [4] Interestingly, quantifying the amplitude and scale geological record. -
Isostasy and Flexure of the Lithosphere
Isostasy and Flexure of the Lithosphere A. B. WATTS Department of Earth Sciences, Oxford University Oxford, United Kingdom PUBLISHED BY THE PRESS SYNDICATE OF THE UNIVERSITY OF CAMBRIDGE The Pitt Building, Trumpington Street, Cambridge, United Kingdom CAMBRIDGE UNIVERSITY PRESS The Edinburgh Building, Cambridge, United Kingdom http://www.cup.cam.ac.uk 40 West 20th Street, New York, NY 10011–4211, USA http://www.cup.org 10 Stamford Road, Oakleigh, Melbourne 3166, Australia Ruiz de Alarco´ n 13, 28014 Madrid, Spain # Cambridge University Press 2001 This book is in copyright. Subject to statutory exception and to the provisions of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. First published 2001 Printed in the United States of America Typeface Times Ten PS 10/12.5 System 3B2 [KW] A catalogue record for this book is available from the British Library Library of Congress Cataloging-in-Publication Data Watts, A. B. (Anthony Brian), 1945– Isostasy and flexure of the lithosphere / A. B. Watts. p. cm. Includes bibliographical references and index. ISBN 0-521-62272 – ISBN 0-521-00600-7 (pb) 1. Isostasy. 2. Earth – Crust. I. Title. QE511.W38 2001 551 – dc21 00-065146 ISBN 0 521 62272 7 hardback ISBN 0 521 00600 7 paperback Contents Preface page xi Acknowledgments xiii Notation xvii 1 The Development of the Concept of Isostasy 1 1.1 Introduction 1 1.2 First Isostatic Ideas 2 1.3 The Deflection of the Vertical in India 9 1.4 Isostasy According to Airy -
Isostasy, Dynamic Topography, and the Elevation of the Apennines of Italy ∗ Claudio Faccenna A, , Thorsten W
Earth and Planetary Science Letters 407 (2014) 163–174 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Isostasy, dynamic topography, and the elevation of the Apennines of Italy ∗ Claudio Faccenna a, , Thorsten W. Becker b, Meghan S. Miller b, Enrico Serpelloni c, Sean D. Willett d a Laboratory Experimental Tectonics, Università Roma TRE, Roma, Italy b Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA c Istituto Nazionale Geofisica e Vulcanologia, Centro Nazionale Terremoti, Bologna, Italy d Department of Earth Sciences, Swiss Federal Institute of Technology, Zurich, Switzerland a r t i c l e i n f o a b s t r a c t Article history: The elevation of an orogenic belt is commonly related to crustal/lithosphere thickening. Here, we discuss Received 19 March 2014 the Apennines as an example to show that topography at a plate margin may be controlled not only by Received in revised form 28 August 2014 isostatic adjustment but also by dynamic, mantle-driven processes. Using recent structural constraints for Accepted 14 September 2014 the crust and mantle we find that the expected crustal isostatic component explains only a fraction of Available online xxxx the topography of the belt, indicating positive residual topography in the central Apennines and negative Editor: Y. Ricard residual topography in the northern Apennines and Calabria. The trend of the residual topography Keywords: matches the mantle flow induced dynamic topography estimated from regional tomography models. Apennines We infer that a large fraction of the Apennines topography is related to mantle dynamics, producing elevation relative upwellings in the central Apennines and downwellings in the northern Apennines and Calabria subduction where subduction is still ongoing. -
Isostasy and Its Meaning
SVENSKA GEOFYSISKA FORENINGEN VOLUME I, NUMBER 3 Te I L u s AUGUST 1949 A QUARTERLY JOURNAL OF GEOPHYSICS Isostasy and its Meaning By B. GUTENBERG, California Institute of Technology1 (Manuscript received June 25, 1949) Abstract The theory of isostasy supposes that, in regions which have not been disturbed recently, each vertical column of the earth's crust with a certain minimum radius and extending to a depth of about IOO km has approximately the same mass. To find the deviation from this approximation in a given region, the density must be assumed as a function of depth. Such assumptions used at present for calculations are discussed critically. The resulting errors are greater than it is normally beleaved; errors in the calculated isostatic gravity anomalies exceeding ten milligals must be expected in certain regions. Systematic errors result from the usual assumption in routine calculations that the mean density in the earth's crustal layers under the bottom of the Pacific and in the continental areas is the same, and that in both the difference between the density of the layers above about 30 km and the layers below this depth is 0.6. The processes producing and maintaining isostatic equilibrium are discussed. In the theory of isostasy it is assumed that available, there are two ways to approach this in regions that have not been disturbed re- uestion. The first is, to use observations of cently each vertical column of the earth's crust tx e density and distribution of rocks in the with a given radius (at least, say, 10 km) and earth's crust and of gravity at the earth's surface extending down to a sufficient specified depth and to calculate the residuals (the so-called (apparently at least 60 km), has approximately gravity anomalies) against an assumed equili- the same mass, regardless of the surface condi- brium condition; the second is to consider the tion (continental or oceanic) or of the surface processes involved in establishing isostasy. -
Application to the Mid-Norwegian Continental Margin
Downloaded from http://sp.lyellcollection.org/ by guest on September 28, 2021 Isostasy as a tool to validate interpretations of regional geophysical datasets – application to the mid-Norwegian continental margin SOFIE GRADMANN1*, CLAUDIA HAASE1 &JO¨ RG EBBING1,2 1Geological Survey of Norway, Leiv Eirikssons vei 39, 7040 Trondheim, Norway 2Present address: Department of Geosciences, Kiel University, 24118 Kiel, Germany *Correspondence: sofi[email protected] Abstract: Isostasy is a well understood concept, yet rarely applied to its full capacity in regional interpretations of crustal structures. In this study, we utilize a recent density model for the entire NE Atlantic, based on refraction seismic data and gravity inversion, to calculate isostatically balanced bathymetry along the mid-Norwegian margin. Since gravity and isostatically balanced elevation are independent observables but both depend on the underlying density model, consis- tencies and discrepancies point towards model deficits, erroneously interpreted or poorly understood areas. Four areas of large isostatic residuals are identified. Along the outer Vøring Margin, a mass deficit points to more extensive high-density bodies or a shallower Moho than currently mapped. Farther seaward, along the Vøring Marginal High, a mass excess indicates inaccurate mapping of the continent–ocean boundary and surrounding structures. A number of eclogitic bodies along the proximal mid-Norwegian margin have been described in recent publications and their presence is now also confirmed by isostatic calculations. Major elevation and gravity residuals along the transition between the Vøring and Møre margins signify that the structure of this region is poorly understood and modifications to the mapped continent–ocean transition may be required. -
Dynamic Topography, Gravity and the Role of Lateral Viscosity Variations From
1 Geophysical Journal International Advance Access published September 6, 2016 Dynamic topography, gravity and the role of lateral viscosity variations from inversion of global mantle flow Ting Yang and Michael Gurnis Seismological Laboratory California Institute of Technology Downloaded from Pasadena, CA 91125 http://gji.oxfordjournals.org/ Abstract. Lateral viscosity variations (LVVs) in the mantle influence geodynamic processes and their surface expressions. With the observed long-wavelength geoid, at California Institute of Technology on September 7, 2016 free-air anomaly, gravity gradient in three directions and discrete, high-accuracy residual topography, we invert for depth- and temperature-dependent and tectonically regionalized mantle viscosity with a mantle flow model. The inversions suggest that: long-wavelength gravitational and topographic signals are mainly controlled by the radial viscosity profile; the pre-Cambrian lithosphere viscosity is slightly (~ one order of magnitude) higher than that of oceanic and Phanerozoic lithosphere; plate margins are substantially weaker than plate interiors; and viscosity has only a weak apparent, dependence on temperature, suggesting either a balancing between factors or a smoothing of actual higher amplitude, but short wavelength, LVVs. The predicted large-scale lithospheric stress regime (compression or extension) is consistent with the world stress map (thrust or normal faulting). Both recent compiled high-accuracy 2 residual topography and the predicted dynamic topography yield ~1 km amplitude long-wavelength dynamic topography, inconsistent with recent studies suggesting amplitudes of ~100 to ~500 m. Such studies use a constant, positive admittance (transfer function between topography and gravity), in contrast to the evidence which shows that the earth has a spatially- and wavelength-dependent admittance, with large, 4 negative admittances between ~4000 - ~10 km wavelengths. -
Linking Plate Tectonics and Mantle Flow to Earth's Topography FOCUS
RESEARCH FOCUS: Linking plate tectonics and mantle flow to Earth’s topography Nicolas Flament Earthbyte Group, School of Geosciences, The University of Sydney, Sydney, NSW 2006, Australia It has long been known that solid-state convection within Earth’s man- (Davies and Pribac, 1993). As for the South Atlantic Ocean, it would be tle should result in deformation of its surface (Pekeris, 1935), a phenomenon shallower to the east of Argentina (Shephard et al., 2012) and deeper to the referred to as dynamic topography. This topography is relatively elusive: it west of southern Africa (Nyblade and Robinson, 1994)—in other words, is transient over time scales of 1–10 m.y., it occurs over spatial scales cover- the South Atlantic would not be as asymmetric (Flament et al., 2014). ing a few hundred to a few thousand kilometers, and its amplitude is on the Because a large portion of Earth’s continents lies at low elevations order of 1 km at long wavelengths. This amplitude is small in comparison (as reflected by the difference between the equal-area arithmetic mean, to the secular bimodal topography of Earth (the average elevation contrast 529 m, and median, 178 m, of elevations above -200 m), changes in long- between oceans and continents is ~4.5 km), mostly because of thickness wavelength dynamic topography cause significant shifts in coastlines and density contrasts at crustal and lithospheric depths, that is modulated by despite the small amplitude of the signal. In Figure 1B, this is reflected by tectonic processes, resulting in mountain belts up to several kilometers high. -
Concepts of Isostasy
Unit 3 Interior of the Earth: Structure and Composition .................................................................................................................................................................................................................................... UNIT 4 CONCEPTS OF ISOSTASY Structure 4.1 Introduction 4.4 Views on Isostasy Expected Learning Outcomes Airy’s Theory 4.2 Basic Principles Pratt’s Theory Hayford and Bowie Principle of Buoyancy Joly Density Heiskanen Lithospheric Flexure Vening-Meinesz or Flexural The Concept of Equilibrium Isostasy The Isostatic Adjustments Isostasy v/s No Isostasy 4.3 Development of the Concept of 4.5 Summary Isostasy 4.6 Terminal Questions Determination of Latitudes Isostasy as the Earth’s Balance 4.7 Answers Isostatic Effects 4.8 References/Further Reading 4.1 INTRODUCTION In the previous units of this course, you have learnt about the origin of the Earth, its internal structure and composition as well as the life forms it supports. You must have realized that it is a very complex system. Now we turn our attention to understand how and which features of the Earth helps in achieving this delicate balance. In particular, this unit is devoted to the discussion of isostasy, which gives us information about the mechanical stability between the upstanding features and low lying basins of the Earth. In this unit, we will trace the evolution of the concept of isostasy, which originated in a survey initiated to determine the shape of the Earth. 65 Block 1 GEO-Tectonics .................................................................................................................................................................................................................................... You might have visited different places in India as well as abroad and observed some relief features present on the Earth’s surface, such as mountains, plains, plateaus, valleys, lakes and oceans etc. You might have also noticed that such features are of different shapes and sizes.