Bearworks Cyclostratigraphic Trends of Δ13c in Upper Cambrian Strata
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Solar System Table of Contents Publisher's Note Editors' Introduction List of Contributors Complete List of Contents Archeaostronomy (new) Asteroids Auroras Big Bang Brown Dwarfs Callisto (new) Ceres (new) Comet Halley Comet Shoemaker-Levy 9 (new) Comets Coordinate Systems Coronal Holes and Coronal Mass Ejections (new) Cosmic Rays Cosmology Dwarf Planets (new) Earth-Moon Relations (new) Earth-Sun Relations Earth System Science Earth's Age Earth's Atmosphere Earth's Composition Earth's Core Earth's Core-Mantle Boundary Earth's Crust Earth's Crust-Mantle Boundary(new) Earth's Differentiation Earth's Magnetic Field: Origins Earth's Magnetic Field: Secular Variation Earth's Magnetic Field at Present Earth's Magnetosphere Earth's Mantle Earth's Oceans Earth's Origin Earth's Rotation Earth's Shape Earth's Structure Eclipses Electromagnetic Radiation: Thermal Emissions (new) Electromagnetic Radiation: Nonthermal Emissions (new) Enceladus (new) Eris and Dysnomia (new) Europa Extrasolar Planet Detection Methods (new) Extrasolar Planetary Systems Extraterrestrial Life in the Solar System Gamma-Ray Bursters Ganymede (new) General Relativity Gravity Measurement Greenhouse Effect Habitable Zones (new) Hertzsprung-Russell Diagram Iapetus (new) Impact Cratering Infrared Astronomy Interstellar Clouds and the Interstellar Medium Interplanetary Environment (new) Io Jovian Planets Jupiter's Atmosphere Jupiter's Great Red Spot Jupiter's Interior (new) Jupiter's Magnetic Field and Radiation Belts Jupiter's Ring System (new) Jupiter's Satellites Kuiper Belt -
Early Paleozoic Life & Extinctions (Part 1)
NJU Course Extinctions: Past, Present & Future Prof. Norman MacLeod School of Earth Sciences & Engineering, Nanjing University Extinctions: Past, Present & Future Extinctions: Past, Present & Future Course Syllabus (Revised) Section Week Title Introduction 1 Course Introduction, Intro. To Extinction Introduction 2 History of Extinction Studies Introduction 3 Evolution, Fossils, Time & Extinction Precambrian Extinctions 4 Origin of Life & Precambrian Extionctions Paleozoic Extinctions 5 Early Paleozoic World & Extinctions Paleozoic Extinctions 6 Middle Paleozoic World & Extinctions Paleozoic Extinctions 7 Late Paleozoic World & Extinctions Assessment 8 Mid-Term Examination Mesozoic Extinctions 9 Triassic-Jurassic World & Extinctions Mesozoic Extinctions 10 Labor Day Holiday Cenozoic Extinctions 11 Cretaceous World & Extinctions Cenozoic Extinctions 12 Paleogene World & Extinctions Cenozoic Extinctions 13 Neogene World & Extinctions Modern Extinctions 14 Quaternary World & Extinctions Modern Extinctions 15 Modern World: Floras, Faunas & Environment Modern Extinctions 16 Modern World: Habitats & Organisms Assessment 17 Final Examination Early Paleozoic World, Life & Extinctions Norman MacLeod School of Earth Sciences & Engineering, Nanjing University Early Paleozoic World, Life & Extinctions Objectives Understand the structure of the early Paleozoic world in terms of timescales, geography, environ- ments, and organisms. Understand the structure of early Paleozoic extinction events. Understand the major Paleozoic extinction drivers. Understand -
Four Centuries of Geomagnetic Secular Variation from Historical Records
Fourcenturies of geomagnetic secular variationfrom historical records ByAndrewJackson 1,ArtR.T. Jonkers 2 andMatthewR.W alker 1 1School ofEarth Sciences, Leeds University,Leeds LS29JT, UK 2Departmentof History, V rijeUniversiteit, Amsterdam, The Netherlands Wepresent anewmodel of the magnetic eld at the core{mantle boundary for the interval 1590{1990. Themodel, called gufm1,is based on amassive newcompilation of historical observations of the magnetic eld. The greater part of the newdataset originates from unpublished observations taken by mariners engaged in merchant and naval shipping. Considerable attention is given to both correction of data for possible mislocation (originating from poor knowledge of longitude) and to proper allocation of error in the data. Weadopt astochastic model for uncorrected positional errors that properly accounts for the nature of the noise process based on aBrownian motion model. Thevariability of navigational errors as afunction of the duration of the voyages that wehave analysed isconsistent with this model. For the period before 1800, more than 83 000 individual observations of magnetic declination wererecorded at more than 64 000 locations; more than 8000 new observations are for the 17th century alone. Thetime-dependent eld model that weconstruct from the dataset is parametrized spatially in terms of spherical harmonics and temporally in B-splines, using atotal of 36 512 parameters. Themodel has improved the resolution of the core eld, and represents the longest continuous model of the eld available. However, full exploitation of the database may demand anew modelling methodology. Keywords: Earth’score; geom agneticsec ularvariation ; magnetic¯ eld;m aritimehistory 1.Intro duction TheEarth has possessed amagnetic eld for more than 4billion years, generated in the ®uid core. -
Ediacaran and Cambrian Stratigraphy in Estonia: an Updated Review
Estonian Journal of Earth Sciences, 2017, 66, 3, 152–160 https://doi.org/10.3176/earth.2017.12 Ediacaran and Cambrian stratigraphy in Estonia: an updated review Tõnu Meidla Department of Geology, Institute of Ecology and Earth Sciences, Faculty of Science and Technology, University of Tartu, Ravila 14a, 50411 Tartu, Estonia; [email protected] Received 18 December 2015, accepted 18 May 2017, available online 6 July 2017 Abstract. Previous late Precambrian and Cambrian correlation charts of Estonia, summarizing the regional stratigraphic nomenclature of the 20th century, date back to 1997. The main aim of this review is updating these charts based on recent advances in the global Precambrian and Cambrian stratigraphy and new data from regions adjacent to Estonia. The term ‘Ediacaran’ is introduced for the latest Precambrian succession in Estonia to replace the formerly used ‘Vendian’. Correlation with the dated sections in adjacent areas suggests that only the latest 7–10 Ma of the Ediacaran is represented in the Estonian succession. The gap between the Ediacaran and Cambrian may be rather substantial. The global fourfold subdivision of the Cambrian System is introduced for Estonia. The lower boundary of Series 2 is drawn at the base of the Sõru Formation and the base of Series 3 slightly above the former lower boundary of the ‘Middle Cambrian’ in the Baltic region, marked by a gap in the Estonian succession. The base of the Furongian is located near the base of the Petseri Formation. Key words: Ediacaran, Cambrian, correlation chart, biozonation, regional stratigraphy, Estonia, East European Craton. INTRODUCTION The latest stratigraphic chart of the Cambrian System in Estonia (Mens & Pirrus 1997b, p. -
Magnetic Power Spectrum, with Application to Planetary Dynamo Radii
Earth and Planetary Science Letters 401 (2014) 347–358 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl A new model for the (geo)magnetic power spectrum, with application to planetary dynamo radii ∗ Benoit Langlais a, , Hagay Amit a, Hugo Larnier a,b, Erwan Thébault c, Antoine Mocquet a a Laboratoire de Planétologie et Géodynamique, CNRS UMR 6112, Université de Nantes, 44322 Nantes cedex 3, France b Institut de Physique du Globe de Strasbourg, UdS–CNRS UMR7516, EOST – Université de Strasbourg, 5 rue René Descartes, 67084 Strasbourg Cedex, France c Équipe de Géomagnétisme, Institut de Physique du Globe de Paris, CNRS UMR 7154, 75252 Paris cedex 5, France a r t i c l e i n f o a b s t r a c t Article history: We propose two new analytical expressions to fit the Mauersberger–Lowes geomagnetic field spectrum Received 6 November 2013 at the core–mantle boundary. These can be used to estimate the radius of the outer liquid core where the Received in revised form 23 April 2014 geodynamo operates, or more generally the radius of the planetary dynamo regions. We show that two Accepted 10 May 2014 sub-families of the geomagnetic field are independent of spherical harmonics degree n at the core–mantle Available online 9 July 2014 boundary and exhibit flat spectra. The first is the non-zonal field, i.e., for spherical harmonics order m Editor: C. Sotin different from zero. The second is the quadrupole family, i.e., n + m even. The flatness of their spectra is Keywords: motivated by the nearly axisymmetric time-average paleomagnetic field (for the non-zonal field) and the magnetic power spectrum dominance of rotational effects in core dynamics (for the quadrupole family). -
GSSP) of the Drumian Stage (Cambrian) in the Drum Mountains, Utah, USA
Articles 8585 by Loren E. Babcock1, Richard A. Robison2, Margaret N. Rees3, Shanchi Peng4, and Matthew R. Saltzman1 The Global boundary Stratotype Section and Point (GSSP) of the Drumian Stage (Cambrian) in the Drum Mountains, Utah, USA 1 School of Earth Sciences, The Ohio State University, 125 South Oval Mall, Columbus, OH 43210, USA. Email: [email protected] and [email protected] 2 Department of Geology, University of Kansas, Lawrence, KS 66045, USA. Email: [email protected] 3 Department of Geoscience, University of Nevada, Las Vegas, Las Vegas, NV 89145, USA. Email: [email protected] 4 State Key Laboratory of Palaeobiology and Stratigraphy, Nanjing Institute of Geology and Palaeontology, Chinese Academy of Sciences, 39 East Beijing Road, Nanjing 210008, China. Email: [email protected] The Global boundary Stratotype Section and Point correlated with precision through all major Cambrian regions. (GSSP) for the base of the Drumian Stage (Cambrian Among the methods that should be considered in the selection of a GSSP (Remane et al., 1996), biostratigraphic, chemostratigraphic, Series 3) is defined at the base of a limestone (cal- paleogeographic, facies-relationship, and sequence-stratigraphic cisiltite) layer 62 m above the base of the Wheeler For- information is available (e.g., Randolph, 1973; White, 1973; McGee, mation in the Stratotype Ridge section, Drum Moun- 1978; Dommer, 1980; Grannis, 1982; Robison, 1982, 1999; Rowell et al. 1982; Rees 1986; Langenburg et al., 2002a, 2002b; Babcock et tains, Utah, USA. The GSSP level contains the lowest al., 2004; Zhu et al., 2006); that information is summarized here. occurrence of the cosmopolitan agnostoid trilobite Pty- Voting members of the International Subcommission on Cam- chagnostus atavus (base of the P. -
Losing the Geomagnetic Shield: a Critical Issue for Space Settlement Philip K
Losing the Geomagnetic Shield: A Critical Issue for Space Settlement Philip K. Chapman1 February 3, 2017 Abstract. The geomagnetic field seems to be collapsing. This has happened many times in the deep past, but never since civilization began. One implication is that the cost of space settlement will increase substantially if we do not expedite deployment of initial facilities in low Earth orbit. Another implication, less certain but much more damaging, is that the collapse may lead to catastrophic global cooling before the end of this century. We must establish self-sufficient communities off Earth before that happens. 1. The ELEO Shelter As Al Globus et al have pointed out,2 the annual radiation dose in equatorial low Earth orbit (ELEO, below 600 km altitude) is less than the limit for occupational exposure that is recommended by the International Commission on Radiological Protection. The first extraterrestrial habitats and assembly plants will need little if any radiation shielding if they are located in such an orbit, reducing the mass that must be launched from Earth by orders of magnitude. These fortunate conditions create a haven in ELEO where we can develop the infrastructure for space settlement at relatively low cost. This is a major opportunity to shrink the technical and economic barriers to growth of a true interplanetary society. The most important functions of early facilities in ELEO include: 1. Assembling and launching missions to obtain radiation shielding materials at low cost (probably water or slag from a near-Earth asteroid). 2. Developing experience concerning the long-term physiological requirements for living and working in space (with or without frequent transfers to and from free fall), in order to specify acceptable rotation rates and centrifugal pseudo-gravity levels. -
New Evolutionary and Ecological Advances in Deciphering the Cambrian Explosion of Animal Life
Journal of Paleontology, 92(1), 2018, p. 1–2 Copyright © 2018, The Paleontological Society 0022-3360/18/0088-0906 doi: 10.1017/jpa.2017.140 New evolutionary and ecological advances in deciphering the Cambrian explosion of animal life Zhifei Zhang1 and Glenn A. Brock2 1Shaanxi Key Laboratory of Early Life and Environments, State Key Laboratory of Continental Dynamics and Department of Geology, Northwest University, Xi’an, 710069, China 〈[email protected]〉 2Department of Biological Sciences and Marine Research Centre, Macquarie University, Sydney, NSW, 2109, Australia 〈[email protected]〉 The Cambrian explosion represents the most profound animal the body fossil record of ecdysozoans and deuterostomes is very diversification event in Earth history. This astonishing evolu- poorly known during this time, potentially the result of a distinct tionary milieu produced arthropods with complex compound lack of exceptionally preserved faunas in the Terreneuvian eyes (Paterson et al., 2011), burrowing worms (Mángano and (Fortunian and the unnamed Stage 2). However, this taxonomic Buatois, 2017), and a variety of swift predators that could cap- ‘gap’ has been partially filled with the discovery of exceptionally ture and crush prey with tooth-rimmed jaws (Bicknell and well-preserved stem group organisms in the Kuanchuanpu Paterson, 2017). The origin and evolutionary diversification of Formation (Fortunian Stage, ca. 535 Ma) from Ningqiang County, novel animal body plans led directly to increased ecological southern Shaanxi Province of central China. High diversity and complexity, and the roots of present-day biodiversity can be disparity of soft-bodied cnidarians (see Han et al., 2017b) and traced back to this half-billion-year-old evolutionary crucible. -
Mercury's Resonant Rotation from Secular Orbital Elements
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Institute of Transport Research:Publications Mercury’s resonant rotation from secular orbital elements Alexander Stark a, Jürgen Oberst a,b, Hauke Hussmann a a German Aerospace Center, Institute of Planetary Research, D-12489 Berlin, Germany b Moscow State University for Geodesy and Cartography, RU-105064 Moscow, Russia The final publication is available at Springer via http://dx.doi.org/10.1007/s10569-015-9633-4. Abstract We used recently produced Solar System ephemerides, which incorpo- rate two years of ranging observations to the MESSENGER spacecraft, to extract the secular orbital elements for Mercury and associated uncer- tainties. As Mercury is in a stable 3:2 spin-orbit resonance these values constitute an important reference for the planet’s measured rotational pa- rameters, which in turn strongly bear on physical interpretation of Mer- cury’s interior structure. In particular, we derive a mean orbital period of (87.96934962 ± 0.00000037) days and (assuming a perfect resonance) a spin rate of (6.138506839 ± 0.000000028) ◦/day. The difference between this ro- tation rate and the currently adopted rotation rate (Archinal et al., 2011) corresponds to a longitudinal displacement of approx. 67 m per year at the equator. Moreover, we present a basic approach for the calculation of the orientation of the instantaneous Laplace and Cassini planes of Mercury. The analysis allows us to assess the uncertainties in physical parameters of the planet, when derived from observations of Mercury’s rotation. 1 1 Introduction Mercury’s orbit is not inertially stable but exposed to various perturbations which over long time scales lead to a chaotic motion (Laskar, 1989). -
(Upper Cambrian, Paibian) Trilobite Faunule in the Central Conasauga River Valley, North Georgia, Usa
Schwimmer.fm Page 31 Monday, June 18, 2012 11:54 AM SOUTHEASTERN GEOLOGY V. 49, No. 1, June 2012, p. 31-41 AN APHELASPIS ZONE (UPPER CAMBRIAN, PAIBIAN) TRILOBITE FAUNULE IN THE CENTRAL CONASAUGA RIVER VALLEY, NORTH GEORGIA, USA DAVID R. SCHWIMMER1 WILLIAM M. MONTANTE2 1Department of Chemistry & Geology Columbus State University, 4225 University Avenue, Columbus, Georgia 31907, USA <[email protected]> 2Marsh & McLennan, Inc., 3560 Lenox Road, Suite 2400, Atlanta, Georgia 30326, USA <[email protected]> ABSTRACT shelf-to-basin break, which is interpreted to be east of the Alabama Promontory and in Middle and Upper Cambrian strata the Tennessee Embayment. The preserva- (Cambrian Series 3 and Furongian) in the tion of abundant aphelaspine specimens by southernmost Appalachians (Tennessee to bioimmuration events may have been the re- Alabama) comprise the Conasauga Forma- sult of mudflows down the shelf-to-basin tion or Group. Heretofore, the youngest re- slope. ported Conasauga beds in the Valley and Ridge Province of Georgia were of the late INTRODUCTION Middle Cambrian (Series 3: Drumian) Bo- laspidella Zone, located on the western state Trilobites and associated biota from Middle boundary in the valley of the Coosa River. Cambrian beds of the Conasauga Formation in Two new localities sited eastward in the Co- northwestern Georgia have been described by nasauga River Valley, yield a diagnostic suite Walcott, 1916a, 1916b; Butts, 1926; Resser, of trilobites from the Upper Cambrian 1938; Palmer, 1962; Schwimmer, 1989; Aphelaspis Zone. Very abundant, Schwimmer and Montante, 2007. These fossils polymeroid trilobites at the primary locality and deposits come from exposures within the are referable to Aphelaspis brachyphasis, valley of the Coosa River, in Floyd County, which is a species known previously in west- Georgia, and adjoining Cherokee County, Ala- ern North America. -
Solar Activity, Earth's Rotation Rate and Climate Variations in the Secular And
Physics and Chemistry of the Earth 31 (2006) 99–108 www.elsevier.com/locate/pce Solar activity, Earth’s rotation rate and climate variations in the secular and semi-secular time scales S. Duhau * Facultad de Ciencias Exactas, Departamento de Fı´sica, Universidad de Buenos Aires, Argentina Received 17 January 2005; accepted 18 March 2005 Available online 29 March 2006 Abstract By applying the wavelet formalism to sudden storm commencements and aa geomagnetic indices and solar total irradiation, as a proxy data for solar sources of climate-forcing, we have searched the signatures of those variables on the Northern Hemisphere surface temperature. We have found that cyclical behaviour in surface temperature is not clearly related to none of these variables, so we have suggested that besides them surface temperature might be related to Earth’s rotation rate variations. Also it has been suggested that in the long-term Earth’s rotation rate variations might be excited by geomagnetic storm time variations which, in turn, depends on solar activity. The study of these phenomena and its relationships is addressed in the present paper. With this purpose we perform an analysis of the evolution during the last 350 years of the signals that conform the 11-year sunspot cycle maxima envelope for different time scales. The result is applied to analyze the relationship between long-term variations in sunspot number and excess of length of day; and to unearth the signature in surface temperature of this last from that of sudden storm commencement and aa geomagnetic indices and total solar irradiation. As solar dynamo experiments transient processes in all the time scales from seconds to centuries, Fourier analysis and its requirement for the process to be stationary is likely to produce spurious periodicities. -
Analysis of the Secular Variations of Longitudes of the Sun, Mercury and Venus from Optical Observations
Highlights of Astronomy, Vol. 12 International Astronomical Union, 2002 H. Rickman, ed. Analysis of the Secular Variations of Longitudes of the Sun, Mercury and Venus from Optical Observations Y.B. Kolesnik Institute of Astronomy of the Russian Academy of Sciences, Piatnitskaya str. 48, 109017 Moscow, Russia Abstract. About 240 000 optical observations of the Sun, Mercury and Venus, accumulated during the era of classical astrometry from Bradley up to our days, are incorporated to analyse the secular variation of the lon gitudes of innermost planets. A significant discrepancy between modern ephemerides and optical observations is discovered. The possible sources of discrepancy are discussed. The tidal acceleration of the Moon has been revised to conform the lunar theory with the ephemerides of the planets. The offset and residual rotation of Hipparcos-based system with respect to the dynamical equinox is determined. Interpretation of this rotation is given. 1. Observations and method of analysis A mass of 244960 observations of the Sun, Mercury and Venus accumulated during historical period of astronomy from 1750 to 2000 have been incorporated. In the transformation procedure a set of corrections were formed by direct comparison of standard star catalogue with ICRS-based catalogue rotated from J2000 to the respective epoch by use of modern precession constant and Hip- parcos based proper motions. The systematic differences are interpolated onto observed positions of planets and applied. Other corrections account for dif ferences in modern and historical astronomical constants. The N70E catalogue (Kolesnik 1997) rigidly rotated onto Hipparcos frame was used as a reference catalogue. Observations were compared with DE405 ephemeris.